EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN)

 CERN-EP-2021-046 LHCb-PAPER-2021-002 Sep 13, 2021

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LHCb collaboration†††Authors are listed at the end of this paper.

The first search for the doubly heavy baryon and a search for the baryon are
performed using $pp$ collision data collected via the LHCb experiment from
2016 to 2018 at a centre-of-mass energy of $13\text{\,Te\kern-1.00006ptV}$,
corresponding to an integrated luminosity of 5.2$\text{\,fb}^{-1}$. The
baryons are reconstructed via their decays to
${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ and
${{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$. No significant excess is found for
invariant masses between 6700 and 7300$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$,
in a rapidity range from 2.0 to 4.5 and a transverse momentum range from 2 to
20$\text{\,Ge\kern-1.00006ptV\\!/}c$. Upper limits are set on the ratio of the
and production cross-section times the branching fraction to
${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ (${\Xi}^{+}_{\mathrm{c}}$
${\uppi}^{-}$) relative to that of the ${{\Lambda}^{0}_{\mathrm{b}}}$
($\Xibn$) baryon, for different lifetime hypotheses, at $95\%$ confidence
level. The upper limits range from $0.5\times 10^{-4}$ to $2.5\times 10^{-4}$
for the  () decay, and from $1.4\times 10^{-3}$ to $6.9\times 10^{-3}$ for the
() decay, depending on the considered mass and lifetime of the () baryon.

Published in Chin. Phys. C45 (2021) 093002

© 2024 CERN for the benefit of the LHCb collaboration. CC BY 4.0 licence.

##  1 Introduction

The constituent quark model was initially proposed by Murray Gell-Mann
[GellMann:1964nj] and George Zweig [Zweig:1964jf] for classification of
hadrons formed from light quarks ($\mathrm{u}$, $\mathrm{d}$, $\mathrm{s}$)
and understanding their quantum numbers. It was later extended to hadrons
containing heavy $\mathrm{c}$ or $\mathrm{b}$ quarks [Fleck:1988vm]. In
addition to baryons containing a single heavy quark, the theory also predicts
baryons comprising two heavy quarks. Such doubly heavy baryons provide a
unique probe for quantum chromodynamics, the gauge theory of strong
interactions. In 2017, the LHCb collaboration reported the first observation
of the ${\Xi}^{++}_{{\mathrm{c}}{\mathrm{c}}}$ baryon containing two charm
quarks through the decay
${{\Xi}^{++}_{{\mathrm{c}}{\mathrm{c}}}}\rightarrow{{\Lambda}^{+}_{\mathrm{c}}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}{{\uppi}^{+}}$
[LHCb-PAPER-2017-018].111The inclusion of charge-conjugate modes is implied
throughout this paper. The ${{\Xi}^{++}_{{\mathrm{c}}{\mathrm{c}}}}$ state was
later confirmed in the decay to ${{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{+}}$ [LHCb-
PAPER-2018-026]. Its lifetime, mass and production cross-section were
subsequently measured [LHCb-PAPER-2018-019, LHCb-PAPER-2019-035, LHCb-
PAPER-2019-037]. To date, no baryons containing one $\mathrm{b}$ and one
$\mathrm{c}$ quark, or two $\mathrm{b}$ quarks, have been observed
experimentally. An observation would enrich our knowledge of baryon
spectroscopy and improve our understanding of the quark structure inside
baryons.

The ground-state baryons containing one $\mathrm{b}$ and one $\mathrm{c}$
quark, the ($\mathrm{b}$ $\mathrm{c}$ $\mathrm{s}$), ($\mathrm{b}$
$\mathrm{c}$ $\mathrm{d}$) and ($\mathrm{b}$ $\mathrm{c}$ $\mathrm{u}$)
states, have been considered within various theoretical models. Most studies
predict the masses of the and baryons to be between 6700 and
7200$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ [Bagan:1992za, Roncaglia:1995az,
Lichtenberg:1995kg, Ebert:1996ec, SilvestreBrac:1996wp, Kiselev:2001fw,
Anikeev:2001rk, Ebert:2002ig, He:2004px, Albertus:2006ya, Roberts:2007ni,
Zhang:2008rt, Gerasyuta:2008zy, Azizi:2014jxa, Karliner:2014gca, Shah:2017liu,
Brown:2014ena].

The lifetime of the baryon is predicted to be $0.22\pm 0.04\text{\,ps}$
[Kiselev:2001fw], while the lifetime of is predicted to be in the range of
0.09 to 0.28 ps [Kiselev:2001fw, Karliner:2014gca, Kiselev:1999kh,
Cheng:2019sxr]. The production cross-section of the baryon in proton-proton
(${\mathrm{p}}{\mathrm{p}}$) collisions at a centre-of-mass energy
$\sqrt{s}=14\text{\,Te\kern-1.00006ptV}$ is expected to lie in the range
between 19 to 39 nb, derived from Ref. [Zhang:2011hi], in the pseudorapidity
($\eta$) range of $1.9<\eta<4.9$, depending on the required minimum value of
the momentum component transverse to the beam direction ($p_{\mathrm{T}}$) of
the particle. Recently, the LHCb experiment found no significant baryon signal
in the predicted mass range using the $\Xibcn\rightarrow
D^{0}p{{\mathrm{K}}^{-}}$ decay mode [LHCb-PAPER-2020-014].

This article reports the first search for the baryon and a new search for the
baryon, both via decay chains ${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ with
${{\Lambda}^{+}_{\mathrm{c}}}\rightarrow{\mathrm{p}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}$
or ${{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ with
${{\Xi}^{+}_{\mathrm{c}}}\rightarrow{\mathrm{p}}{{\mathrm{K}}^{-}}{{\uppi}^{+}}$
in the LHCb experiment. Examples of Feynman diagram of the four signal decay
modes are shown in Fig. 1. There are few theoretical predictions on the
branching fractions of these decay modes. Ref. [Wang:2017mqp] predicts the
branching fractions of the  and  decays to be $1.6\times 10^{-7}$ and
$3.0\times 10^{-7}$, respectively. However, uncertainties are not quoted.
Inputs from experimental studies are necessary to deepen our understanding of
the properties of and baryons, and can provide valuable reference for future
searches. Besides, the distinct experimental signatures of these decays make
it promising to search for them in the LHCb experiment considering the high
detection efficiency of the LHCb detector.

The and baryons are not differentiated and are collectively denoted as
hereafter, unless otherwise stated. The production cross-section times
branching fraction of  () decay is measured relative to that of the control
channel (). This takes advantage of identical final-state particles and
similar topology. The search is performed in the mass range between $6700$ and
$7300\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ using the
${\mathrm{p}}{\mathrm{p}}$ collision data collected with the LHCb experiment
at $\sqrt{s}=13\text{\,Te\kern-1.00006ptV}$, corresponding to an integrated
luminosity of $5.2\text{\,fb}^{-1}$. The baryons are reconstructed in the
fiducial region of rapidity ($y$) between $2.0$ and $4.5$ and with
$p_{\mathrm{T}}$ between $2$ and $20\text{\,Ge\kern-1.00006ptV\\!/}c$.

Figure 1: Examples of Feynman diagrams for the $\OmegabcnLcdecay$,
$\OmegabcnXicdecay$, $\XibcnLcdecay$ and $\XibcnXicdecay$ decays.

##  2 Detector and simulation

The LHCb detector [LHCb-DP-2008-001, LHCb-DP-2014-002] is a single-arm forward
spectrometer covering the pseudorapidity range $2<\eta<5$, designed for the
study of particles containing $\mathrm{b}$ or $\mathrm{c}$ quarks. The
detector includes a high-precision tracking system consisting of a silicon-
strip vertex detector surrounding the $pp$ interaction region [LHCb-
DP-2014-001], a large-area silicon-strip detector located upstream of a dipole
magnet with a bending power of approximately $4{\mathrm{\,Tm}}$, and three
stations of silicon-strip detectors and straw drift tubes [LHCb-DP-2017-001]
placed downstream of the magnet. The tracking system provides a measurement of
the momentum, $p$, of charged particles with a relative uncertainty that
varies from 0.5% at low momentum to 1.0% at
200$\text{\,Ge\kern-1.00006ptV\\!/}c$. The minimum distance of a track to a
primary $pp$ collision vertex (PV), the impact parameter (IP), is measured
with a resolution of $(15+29/p_{\mathrm{T}})\,\mu\text{m}$, where
$p_{\mathrm{T}}$ is in $\text{\,Ge\kern-1.00006ptV\\!/}c$. Different types of
charged hadrons are distinguished using information from two ring-imaging
Cherenkov detectors [LHCb-DP-2012-003]. Photons, electrons, and hadrons are
identified by a calorimeter system consisting of scintillating-pad and
preshower detectors, and an electromagnetic and a hadronic calorimeter. Muons
are identified by a system composed of alternating layers of iron and
multiwire proportional chambers [LHCb-DP-2012-002]. The online event selection
is performed by a trigger [LHCb-DP-2012-004], which consists of a hardware
stage, based on information from the calorimeter and muon systems, followed by
a software stage, which applies a full event reconstruction. At the hardware
trigger stage, events are required to have at least one hadron with
$E_{\mathrm{T}}$ larger than 3.5 GeV. The software trigger requires a two-,
three- or four-track secondary vertex with a significant displacement from any
PV. At least one charged particle must have
$p_{\mathrm{T}}>1.6\text{\,Ge\kern-1.00006ptV\\!/}c$ and be inconsistent with
originating from any PV. A multivariate algorithm [BBDT, LHCb-PROC-2015-018]
is used for the identification of secondary vertices consistent with the decay
of a $\mathrm{b}$ hadron.

Simulated samples are produced to model the effects of the detector acceptance
and the imposed selection requirements. In the simulation, $pp$ collisions are
generated using Pythia [Sjostrand:2007gs, Sjostrand:2006za] with a specific
LHCb configuration [LHCb-PROC-2010-056]. A dedicated generator, , is used to
simulate the baryon production [Chang:2009va], with the mass and lifetime of
the baryon set to $m(\Hbcn)=6900\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ and
$\tau(\Hbcn)=0.4\text{\,ps}$. Simulation samples with different mass
(6700–7300$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$) and lifetime (0.2–0.4 ps)
hypotheses are obtained using a weighting technique with the generator level
information on signal. Decays of unstable particles are described by EvtGen
[Lange:2001uf], in which final-state radiation is generated using Photos
[Davidson:2010ew]. The interaction of the generated particles with the
detector, and its response, is implemented using the Geant4 toolkit
[Allison:2006ve, Agostinelli:2002hh] as described in Ref. [LHCb-
PROC-2011-006]. For the two control channels,  and , Pythia is used to
simulate the $pp$ collisions and the production of the
${\Lambda}^{0}_{\mathrm{b}}$ and baryons.

##  3 Reconstruction and selection

For both the signal and the control channels, the
${{\Lambda}^{+}_{\mathrm{c}}},{{\Xi}^{+}_{\mathrm{c}}}\rightarrow
p{{\mathrm{K}}^{-}}{{\uppi}^{+}}$ candidates are reconstructed from three
charged particles identified as a proton, kaon and pion, respectively. The
tracks are required to have good quality, and to be inconsistent with
originating from any PV in the event. The tracks must also form a common
vertex of good fit quality. The ${\Lambda}^{+}_{\mathrm{c}}$
(${\Xi}^{+}_{\mathrm{c}}$) candidate is required to have an invariant mass in
the range 2271–2301$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$
(2450–2488$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$), corresponding to
approximately six times the ${\Lambda}^{+}_{\mathrm{c}}$
(${\Xi}^{+}_{\mathrm{c}}$) mass resolution, and to be inconsistent with
originating from any PV. In the sample of selected
${\Lambda}^{+}_{\mathrm{c}}$ (${\Xi}^{+}_{\mathrm{c}}$) candidates, there is a
sizable background contamination from decays of other particles, such as
${{\mathrm{D}}^{+}}$ (${{\mathrm{D}}^{+}_{\mathrm{s}}}$) decays to
${{\mathrm{K}}^{-}}{{\uppi}^{+}}{{\uppi}^{+}}$
(${{\mathrm{K}}^{-}}{{\mathrm{K}}^{+}}{{\uppi}^{+}}$) with a charged pion
(kaon) misidentified as a proton, and background from $\phi{{\uppi}^{+}}$
combinations where in $\phi\rightarrow{{\mathrm{K}}^{-}}{{\mathrm{K}}^{+}}$
decays a kaon is misidentified as a proton. Such background candidates are
rejected if the ${{\mathrm{K}}^{-}}{{\uppi}^{+}}{{\uppi}^{+}}$,
${{\mathrm{K}}^{-}}{{\mathrm{K}}^{+}}{{\uppi}^{+}}$ or
${{\mathrm{K}}^{-}}{{\mathrm{K}}^{+}}$ invariant mass is consistent with the
known ${{\mathrm{D}}^{+}}$, ${{\mathrm{D}}^{+}_{\mathrm{s}}}$ or $\phi$ mass
[PDG2020], respectively, when a charged pion (kaon) hypothesis is assigned to
the proton candidate.

An additional charged particle identified as a pion and, with $p_{\mathrm{T}}$
greater than 0.2$\text{\,Ge\kern-1.00006ptV\\!/}c$, is combined with the
${\Lambda}^{+}_{\mathrm{c}}$ (${\Xi}^{+}_{\mathrm{c}}$) candidate to form an
candidate. The candidates must have a vertex with good fit quality, a decay
time larger than 0.05 ps, a $p_{\mathrm{T}}$ greater than
2$\text{\,Ge\kern-1.00006ptV\\!/}c$ and a scalar sum of the $p_{\mathrm{T}}$
of the final-state particles greater than 5$\text{\,Ge\kern-1.00006ptV\\!/}c$.
Furthermore, the candidates are required to be consistent with originating
from a PV. To avoid contributions from duplicate tracks, the selected
candidates are rejected if the angle between any pair of the final-state
particle tracks with same charge is smaller than 0.5 mrad.

A boosted decision tree (BDT) classifier [Breiman, AdaBoost] implemented in
the TMVA toolkit [Hocker:2007ht, TMVA4] is used to further suppress
combinatorial background. A simulated signal sample in the mass range
6846–6954$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ and a background sample formed
by candidates in an upper mass sideband region
(7500–9000$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$) are used to train the BDT
classifier. Four different categories of variable are used as the BDT input.
The first category exploits the non-zero lifetime of baryons and a
displacement of their vertices from any PV in the event. The variables
comprise the $\chi^{2}_{\text{IP}}$ of all final-state particles forming the
${\Lambda}^{+}_{\mathrm{c}}$ (${\Xi}^{+}_{\mathrm{c}}$) and candidates with
respect to their associated PV, where $\chi^{2}_{\text{IP}}$ is defined as the
difference in the vertex-fit $\chi^{2}$ of a given PV reconstructed with and
without the particle under consideration, and the associated PV is the one
with respect to which the candidate has the smallest $\chi^{2}_{\text{IP}}$;
the sum of $\chi^{2}_{\text{IP}}$ of the four final-state particles; and
$\chi^{2}$ of the flight distance of the ${\Lambda}^{+}_{\mathrm{c}}$
(${\Xi}^{+}_{\mathrm{c}}$) and candidates. The second category consists of
kinematic variables, including $p_{\mathrm{T}}$ of the final-state particles
and the ${\Lambda}^{+}_{\mathrm{c}}$ (${\Xi}^{+}_{\mathrm{c}}$) and
candidates, and the angle between the momentum vector and the displacement
vector pointing from the associated PV to the decay vertex. The third category
comprises the vertex-fit $\chi^{2}$ of the ${\Lambda}^{+}_{\mathrm{c}}$
(${\Xi}^{+}_{\mathrm{c}}$) and candidates, and $\chi^{2}$ of a kinematic fit
[Hulsbergen:2005pu] of the signal decay chain constraining the candidate to
originate from the associated PV. The fourth category consists of
identification variables of the final-state particles.

The BDT threshold is chosen to maximize the figure of merit,
$\varepsilon/(\tfrac{\alpha}{2}+\sqrt{B})$ [Punzi:2003bu]. Here, $\varepsilon$
is the selection efficiency of signal candidates determined from simulation,
$B$ is the expected background number in the signal mass region, and
$\alpha=5$ is the signal significance. This threshold is estimated using the
signal sample simulated with the default mass and lifetime values. The same
selection is applied to the control modes.

##  4 Yield determination

To improve the resolution of the mass of the candidates, the
${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$
(${{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$) invariant mass is calculated after
constraining the ${{\Lambda}^{+}_{\mathrm{c}}}$ (${\Xi}^{+}_{\mathrm{c}}$)
mass to its known value [PDG2020] and requiring the candidate to be consistent
with originating from its associated PV. The obtained invariant mass
distributions of candidates, $m({{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$
and $m({{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$, are shown in Fig. 2. To search
for the signals, the mass distributions are fitted using an unbinned maximum-
likelihood fit. A double-sided Crystal Ball function [Skwarnicki:1986xj] is
used to model the signal, with tail parameters fixed from simulation, and the
peak position and width allowed to vary in the fit. The background shape is
interpolated from a double-exponential fit to a lower
(6100–6650$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$) and an upper
(7500–9000$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$) sideband region of the
${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$
(${{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$) mass distribution. No significant
excess is observed across the searched mass range.

The ${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ and
${{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ invariant mass distributions of the
selected  and  candidates are shown in Fig. 3. The yields are obtained from
unbinned maximum-likelihood fits to the invariant mass distributions, using
the fit model described above. The yields are determined to be $191\,000\pm
500$ and $5\,490\pm 80$ for  and , respectively.

Figure 2: Invariant mass distributions of selected (left) and (right)
candidates (black points), together with results of the background only fit
(brown dashed line).

Figure 3: Invariant mass distributions of (left)  and (right)  candidates with
the fit results overlaid (blue solid line). The black points represent the
data, the red dashed line represents the signal contribution, and the gray
dashed line represents the combinatorial background.

##  5 Ratio of production cross-sections

The ratio $\cal{R}$ of the baryon production cross-section multiplied by the
branching fraction of the $\HbcnLcdecay$ () decay relative to that of the
${{\Lambda}^{0}_{\mathrm{b}}}$ ($\Xibn$) baryon can be written as

$\displaystyle{\cal{R}}({{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$
$\displaystyle\equiv$ $\displaystyle\frac{\sigma(pp\rightarrow\Hbcn X)\
{\mathcal{B}}\left(\HbcnLcFullDecay\right)}{\sigma(pp\rightarrow{{\Lambda}^{0}_{\mathrm{b}}}X)\
{\mathcal{B}}\left(\LbnLcFullDecay\right)}$ $\displaystyle=$
$\displaystyle\frac{N(\HbcnLcdecay)}{N(\LbnLcdecay)}\cdot\frac{\varepsilon({{\Lambda}^{0}_{\mathrm{b}}})}{\varepsilon(\Hbcn)},$
$\displaystyle{\cal{R}}({{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$
$\displaystyle\equiv$ $\displaystyle\frac{\sigma(pp\rightarrow\Hbcn X)\
{\mathcal{B}}\left(\HbcnXicFullDecay\right)}{\sigma(pp\rightarrow\Xibn X)\
{\mathcal{B}}\left(\XibnXicFullDecay\right)}$ $\displaystyle=$
$\displaystyle\frac{N(\HbcnXicdecay)}{N(\XibnXicdecay)}\cdot\frac{\varepsilon(\Xibn)}{\varepsilon(\Hbcn)},$

where $N$ and $\varepsilon$ are the signal yield and the efficiency for the
corresponding decay modes, respectively The efficiency accounts for the
geometrical acceptance, trigger, reconstruction, and event selection. The
$\cal{R}$ is determined in the fiducial region $2<y<4.5$ and
$2<p_{\mathrm{T}}<20\text{\,Ge\kern-1.00006ptV\\!/}c$.

Efficiencies are determined from the simulated samples. The $p_{\mathrm{T}}$
distributions of ${\Lambda}^{0}_{\mathrm{b}}$ and baryons are not well modeled
in simulation. To improve the description, a gradient boosted weighting method
[Rogozhnikov:2016bdp] is used to apply a kinematic correction on the
$p_{\mathrm{T}}$ distributions of the ${\Lambda}^{0}_{\mathrm{b}}$ and decay
products of the simulated control samples. With this correction, a good
agreement on the ${\Lambda}^{0}_{\mathrm{b}}$ and $p_{\mathrm{T}}$
distribution is seen between the data and simulation. The track detection and
particle identification efficiencies are calibrated with the data [LHCB-
DP-2013-002, LHCB-PUB-2016-021, LHCb-DP-2018-001]. The imperfect modeling of
input variables used in the BDT training can bias the efficiency estimation.
To suppress such effects, ratios between the BDT response distribution of the
background-subtracted data sample and that of the simulated sample are
calculated using the control channel. The background subtraction is performed
using the sPlot method [Pivk:2004ty] with
$m({{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$ and
$m({{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$ as discriminating variables. These
ratios are applied as correction weights to the simulated samples for all
reconstructed decay modes.

The total efficiency ratio
$\varepsilon({{\Lambda}^{0}_{\mathrm{b}}})/\varepsilon(\Hbcn)$ is determined
to be $3.18\pm 0.05$, and $\varepsilon(\Xibn)/\varepsilon(\Hbcn)$ is
calculated to be $3.00\pm 0.02$ for
$m(\Hbcn)=6900\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ and
$\tau(\Hbcn)=0.4\text{\,ps}$. The efficiency is larger for the control mode,
mainly due to the longer lifetime of the ${\Lambda}^{0}_{\mathrm{b}}$ and
baryons. The efficiency depends on the mass and lifetime hypotheses of the
state, and is evaluated from simulation. The kinematic properties of the fully
simulated samples are weighted to match those of the generator-level sample to
calculate the efficiency for different mass and lifetime assumptions.

##  6 Systematic uncertainties

Various sources of systematic uncertainties on ${\cal{R}}$ are estimated and
combined in quadrature. The effect of imperfect description of the mass
distributions on the yield estimates is studied using alternative signal and
background models. For the signal model, the Hypatia [Santos:2013gra] function
is used instead of the nominal double-sided Crystal Ball function. For the
background model of the control modes, the nominal double-exponential function
is replaced by a first-order polynomial function. As the background model for
the decay modes is interpolated from the sidebands, its uncertainty is
evaluated by both replacing the nominal function with an exponential function
and varying the sideband regions. The largest deviation with respect to the
nominal result is taken as the corresponding uncertainty. In total, the
associated systematic uncertainty is estimated to be $0.1\%$ and $0.9\%$ for
and  decays, respectively.

In the ${\cal{R}}$ ratios, systematic uncertainties arising from the track
detection efficiency largely cancel, and the uncertainty due to limited size
of simulation samples is determined to be 1.6% (0.7%) on
${\cal{R}}({{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$
(${\cal{R}}({{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$). The particle
identification efficiency is determined in bins of particle momentum,
pseudorapidity, and track multiplicity using control channels in the data
[LHCb-DP-2018-001]. As the particle identification variables have large
dependencies on the momentum of the final-state particles, there are sizeable
differences in these efficiencies between the control and signal channels,
which do not cancel in the ratio measurement. Systematic effects arising from
the choice of binning scheme are evaluated by varying the bin sizes and
reevaluating the efficiency. The largest deviations from the nominal result,
1.7% and 2.1%, are assigned as the systematic uncertainty for the  and
decays, respectively.

The ${\Lambda}^{+}_{\mathrm{c}}$ (${\Xi}^{+}_{\mathrm{c}}$) mass resolution
shows a difference between data and simulation, which affects the selection
efficiency. It results in a 0.2% systematic uncertainty contribution for the
decay, while the contribution for the  decay is below 0.1%. This systematic
uncertainty is negligible compared to other sources.

The imperfect simulation of the signal and control modes are considered by
applying corrections to the BDT response and kinematic properties of the
simulated control mode samples. To assess the systematic uncertainty in these
corrections, the correcting weights are varied within their uncertainties. The
largest deviation from the nominal result is taken as the systematic
uncertainty. Combining the uncertainties from the BDT response correction and
the kinematic modeling of the simulated control samples gives an uncertainty
of 1.6% for the  channel, and 3.0% for the  channel. The analysis relies on
the $p_{\mathrm{T}}$ model implemented in simulation. No systematic
uncertainty is assigned to this model.

The algorithm used to compute the $\chi^{2}_{\text{IP}}$ was updated during
data collection, which causes a mismatch between data and simulation and
introduces systematic effects in the efficiency estimation. The corresponding
uncertainty was found to be $5\%$ in the previous $\Xibcn$ search [LHCb-
PAPER-2020-014]. Checks by varying the $\chi^{2}_{\text{IP}}$-related
requirements show that the uncertainty well covers the change of result.
Therefore, a $5\%$ systematic uncertainty is assigned.

The systematic uncertainties are summarized in Table 1. The total systematic
uncertainty is $5.7\%$ for  and $6.3\%$ for , for a mass of
6900$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ and lifetime of 0.4 ps. These
values of systematic uncertainties are also used for other assumed lifetime
and mass hypotheses.

Table 1: Sources of systematic uncertainty obtained for an mass of 6900$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ and lifetime of 0.4 ps. The total is the quadratic sum of the individual systematic uncertainties. |  |
---|---|---
Fit model | $0.1\%$ | $0.9\%$
Size of simulated samples | 1.6% | 0.7%
Particle identification efficiency | $1.7\%$ | $2.1\%$
Mass resolution | $<0.1\%~{}~{}~{}$ | $0.2\%$
Simulation model | $1.6\%$ | $3.0\%$
$\chi^{2}_{\text{IP}}$ simulation | 5.0% | 5.0%
Total | $5.7\%$ | $6.3\%$

##  7 Results

No evidence for a or a baryon is observed in the inspected mass range. Upper
limits are set at 95% confidence level on the ratios
${\cal{R}}({{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$ and
${\cal{R}}({{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}})$ under different mass and
lifetime hypotheses for the $\Omegabcn$ and $\Xibcn$ baryons, using the
asymptotic method implemented in the framework [Moneta:2010pm, Cowan:2010js]
considering the systematic uncertainties. The assumed masses of the
$\Omegabcn$ and $\Xibcn$ baryons are varied from 6700 to
7300$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ with a step size of
4$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$, and the lifetime values of 0.2 ps,
0.3 ps, and 0.4 ps are considered. The calculated upper limits are shown in
Fig. 4, as a function of the mass. These results are obtained for the sum of
the and production and as such hold for the two individually.

Figure 4: Upper limits (dotted lines) on the ratio of production cross-section
for and via decays to (left) ${\Lambda}^{+}_{\mathrm{c}}$ ${\uppi}^{-}$ and
(right) ${\Xi}^{+}_{\mathrm{c}}$ ${\uppi}^{-}$ to that of control channels
and . The dotted (dashed) colored lines represent the observed (expected)
upper limits. The assumed lifetime hypotheses for the () are 0.2 ps (red
filled circles), 0.3 ps (blue triangles), and 0.4 ps (magenta open circles).

##  8 Conclusions

The first search for the doubly heavy baryon and a new search for the baryon
in the mass range from 6700 to 7300$\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ are
presented, using $pp$ collision data collected at a centre-of-mass energy
$\sqrt{s}=13\text{\,Te\kern-1.00006ptV}$ with the LHCb experiment. The data
set corresponds to an integrated luminosity of 5.2$\text{\,fb}^{-1}$. The ()
baryon is reconstructed in the ${{\Lambda}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ and
${{\Xi}^{+}_{\mathrm{c}}}{{\uppi}^{-}}$ decay modes. No evidence of a signal
is found. Upper limits at 95% confidence level on the ratio of the ()
production cross-section times its branching fraction relative to that of the
${{\Lambda}^{0}_{\mathrm{b}}}$ () baryon are calculated in the rapidity range
$2.0<y<4.5$ and transverse momentum range
$2<p_{\mathrm{T}}<20\text{\,Ge\kern-1.00006ptV\\!/}c$ under different () mass
and lifetime hypotheses. The upper limits range from $0.5\times 10^{-4}$ to
$2.5\times 10^{-4}$ for the () decay, and from $1.4\times 10^{-3}$ to
$6.9\times 10^{-3}$ for the () decay, for the considered lifetime and mass
hypotheses. These results constitute the first limit on the production of the
baryon. Further measurements will be possible with the larger data samples
expected at the upgraded LHCb experiments [Bediaga:2018lhg] and with
additional decay modes.

## Acknowledgements

We express our gratitude to our colleagues in the CERN accelerator departments
for the excellent performance of the LHC. We thank the technical and
administrative staff at the LHCb institutes. We acknowledge support from CERN
and from the national agencies: CAPES, CNPq, FAPERJ and FINEP (Brazil); MOST
and NSFC (China); CNRS/IN2P3 (France); BMBF, DFG and MPG (Germany); INFN
(Italy); NWO (Netherlands); MNiSW and NCN (Poland); MEN/IFA (Romania); MSHE
(Russia); MICINN (Spain); SNSF and SER (Switzerland); NASU (Ukraine); STFC
(United Kingdom); DOE NP and NSF (USA). We acknowledge the computing resources
that are provided by CERN, IN2P3 (France), KIT and DESY (Germany), INFN
(Italy), SURF (Netherlands), PIC (Spain), GridPP (United Kingdom), RRCKI and
Yandex LLC (Russia), CSCS (Switzerland), IFIN-HH (Romania), CBPF (Brazil), PL-
GRID (Poland) and NERSC (USA). We are indebted to the communities behind the
multiple open-source software packages on which we depend. Individual groups
or members have received support from ARC and ARDC (Australia); AvH Foundation
(Germany); EPLANET, Marie Skłodowska-Curie Actions and ERC (European Union);
A*MIDEX, ANR, Labex P2IO and OCEVU, and Région Auvergne-Rhône-Alpes (France);
Key Research Program of Frontier Sciences of CAS, CAS PIFI, CAS CCEPP,
Fundamental Research Funds for the Central Universities, and Sci. & Tech.
Program of Guangzhou (China); RFBR, RSF and Yandex LLC (Russia); GVA, XuntaGal
and GENCAT (Spain); the Leverhulme Trust, the Royal Society and UKRI (United
Kingdom).

##  9 Inclusion of supplementary material

Three types of supplementary material should be distinguished:

  * •

A regular appendix: lengthy equations or long tables are sometimes better put
in an appendix in order not to interrupt the main flow of a paper. Appendices
will appear in the final paper, on arXiv and on the CDS record and should be
considered integral part of a paper, and are thus to be reviewed like the rest
of the paper. An example of an LHCb paper with an appendix is Ref. [LHCb-
PAPER-2013-070].

  * •

Supplementary material for CDS: plots or tables that would make the paper
exceed the page limit or are not appropriate to include in the paper itself,
but are desirable to be shown in public should be added to the paper drafts in
an appendix, and removed from the paper before submitting to arXiv or the
journal. See Appendix D for further instructions. Examples are: comparison
plots of the new result with older results, plots that illustrate cross-
checks. An example of an LHCb paper with supplementary material for CDS is
Ref. [LHCb-PAPER-2013-035]. Supplementary material for CDS cannot be
referenced in the paper. Supplementary material should be included in the
draft paper to be reviewed by the collaboration.

  * •

Supplementary material for the paper. This is usually called “supplemental
material”, which distinguishes it from supplementary material for CDS only.
Most journals allow to submit files along with the paper that will not be part
of the text of the article, but will be stored on the journal server. Examples
are plain text files with numerical data corresponding to the plots in the
paper. The supplemental material should be cited in the paper by including a
reference which should say “See supplemental material at [link] for [give
brief description of material].” The journal will insert a specific link for
[link]. The arXiv version will usually include the supplemental material as
part of the paper and so should not contain the words “at [link]”.
Supplemental material should be included in the draft paper to be reviewed by
the collaboration. An example of an LHCb paper with supplemental material is
Ref. [LHCb-PAPER-2015-029]

## Appendices

##  Appendix A Standard References

Below is a list of common references, as well as a list of all LHCb
publications. As they are already in prepared bib files, they can be used as
simply as \cite{LHCb-DP-2008-001} to get the LHCb detector paper. The
references are defined in the files main.bib, LHCb-PAPER.bib, LHCb-CONF.bib,
LHCb-DP.bib LHCb-TDR.bib files, with obvious contents. Each of these have
their LHCb-ZZZ-20XX-0YY number as their cite code. If you believe there is a
problem with the formatting or content of one of the entries, then get in
contact with the Editorial Board rather than just editing it in your local
file, since you are likely to need the latest version just before submitting
the article.

Table 2: Standard references. Description |  Ref. cite code
---|---
Lee, Weinberg, Zumino |  [Lee:1967iu] Lee:1967iu
Cabibbo, Kobayashi, Maskawa |  [Cabibbo:1963yz, *Kobayashi:1973fv] Cabibbo:1963yz,*Kobayashi:1973fv
Gell-Mann, Zweig |  [GellMann:1964nj, *Zweig:352337] GellMann:1964nj,*Zweig:352337
Baryon asymmetry & SM $C\\!P$ |  [Gavela:1994dt] Gavela:1994dt
Baryon asymmetry & SM $C\\!P$ |  [Gavela:1993ts] Gavela:1993ts
EW Baryogenesis & $C\\!P$ |  [Huet:1994jb] Huet:1994jb
Dalitz Plot222Dalitz invented the method, Fabri added relativistic corrections. |  [Dalitz:1953cp, *Fabri:1954zz] Dalitz:1953cp,*Fabri:1954zz
PDG 2020 |  [PDG2020] PDG2020
PDG 2019 |  [PDG2019] PDG2019
PDG 2018 |  [PDG2018] PDG2018
PDG 2016 |  [PDG2016] PDG2016
PDG 2014 |  [PDG2014] PDG2014
HFlav 2018 |  [HFLAV18] HFLAV18
HFlav 2016 |  [HFLAV16] HFLAV16
HFlav (pre-2016) |  [Amhis:2014hma] Amhis:2014hma
CKMfitter group |  [CKMfitter2005] CKMfitter2005
CKMfitter group |  [CKMfitter2015] CKMfitter2015
UTfit (Standard Model/CKM) |  [UTfit-UT] UTfit-UT
UTfit (New Physics) |  [UTfit-NP] UTfit-NP
Pythia |  [Sjostrand:2007gs, *Sjostrand:2006za] Sjostrand:2007gs,*Sjostrand:2006za
LHCb Pythia tuning |  [LHCb-PROC-2010-056] LHCb-PROC-2010-056
EvtGen |  [Lange:2001uf] Lange:2001uf
Photos |  [Golonka:2005pn] Golonka:2005pn
Geant4 |  [Allison:2006ve, *Agostinelli:2002hh] Allison:2006ve, *Agostinelli:2002hh
LHCb simulation |  [LHCb-PROC-2011-006] LHCb-PROC-2011-006
RapidSim |  [Cowan:2016tnm] Cowan:2016tnm
Dirac |  [Tsaregorodtsev:2010zz, *BelleDIRAC] Tsaregorodtsev:2010zz,*BelleDIRAC
HLT2 topological trigger |  [BBDT] BBDT
Topological trigger reoptimization — Run 2 |  [LHCb-PROC-2015-018] LHCb-PROC-2015-018
Turbo and real-time alignment — Run 2 |  [LHCb-PROC-2015-011] LHCb-PROC-2015-011
TisTos method |  [LHCb-PUB-2014-039] LHCb-PUB-2014-039
Allen |  [Aaij:2019zbu] Aaij:2019zbu
PIDCalib (for Run 1) |  [LHCb-PUB-2016-021] LHCb-PUB-2016-021
Ghost probability |  [DeCian:2255039] DeCian:2255039
Primary vertex reconstruction |  [Kucharczyk:1756296] Kucharczyk:1756296
DecayTreeFitter |  [Hulsbergen:2005pu] Hulsbergen:2005pu
SMOG |  [FerroLuzzi:2005em] FerroLuzzi:2005em
Run-2 tagging |  [Fazzini:2018dyq] Fazzini:2018dyq
OS $\mathrm{K}$, $\upmu$, $\mathrm{e}$ and VS tagging |  [LHCb-PAPER-2011-027] LHCb-PAPER-2011-027
OS charm tagging |  [LHCb-PAPER-2015-027] LHCb-PAPER-2015-027
SS kaon tagging |  [LHCb-PAPER-2015-056] LHCb-PAPER-2015-056
SS proton and pion tagging |  [LHCb-PAPER-2016-039] LHCb-PAPER-2016-039
Reommendations for multiple candidates |  [Koppenburg:2017zsh] Koppenburg:2017zsh
See also Table LABEL:tab:LHCb-DPs for LHCb performance references.
sPlot |  [Pivk:2004ty] Pivk:2004ty
sFit |  [Xie:2009rka] Xie:2009rka
Punzi’s optimization |  [Punzi:2003bu] Punzi:2003bu
BDT |  [Breiman] Breiman
BDT training |  [AdaBoost] AdaBoost
TMVA333Do not cite this instead of the actual reference for the MVA being used. |  [Hocker:2007ht, *TMVA4] Hocker:2007ht,*TMVA4
RooUnfold |  [Adye:2011gm] Adye:2011gm
scikit-learn |  [Scikit-learn-paper] Scikit-learn-paper
Laura++ |  [Back:2017zqt] Back:2017zqt
hep_ml |  [Rogozhnikov:2016bdp] Rogozhnikov:2016bdp
root_numpy |  [root-numpy] root-numpy
GammaCombo444Always cite this along with Ref. [LHCb-PAPER-2016-032] as \cite{GammaCombo,*LHCb-PAPER-2016-032} (unless LHCb-PAPER-2016-032 is cited elsewhere). |  [GammaCombo] GammaCombo
Crystal Ball function555A valid alternative for most papers where the normalisation is not critical is to use the expression“Gaussian function with a low-mass power-law tail” or “Gaussian function with power-law tails”. In that case, no citation is needed |  [Skwarnicki:1986xj] Skwarnicki:1986xj
Hypatia function |  [Santos:2013gra] Santos:2013gra
Modified Novosibirsk function |  [Ikeda:1999aq] Ikeda:1999aq
Bukin function |  [Bukin:2007] Bukin:2007
Wilks’ theorem |  [Wilks:1938dza] Wilks:1938dza
CLs method |  [CLs] CLs
BLUE method |  [Nisius:2020jmf] Nisius:2020jmf
Bootstrapping |  [efron:1979] efron:1979
Blatt–Weisskopf barrier |  [Blatt:1952ije] Blatt:1952ije
$f_{s}/f_{d}$ at 7–8 TeV |  [fsfd] fsfd
LHC beam energy uncertainty |  [PhysRevAccelBeams.20.081003] PhysRevAccelBeams.20.081003
Table 3: LHCb detector performance papers. LHCb-DP number | Title
---|---
LHCb-DP-2019-004 [LHCb-DP-2019-004] | Diphoton discrimination
LHCb-DP-2019-003 [LHCb-DP-2019-003] | Electron reconstruction efficiency
LHCb-DP-2019-002 [LHCb-DP-2019-002] | Real-Time analysis
LHCb-DP-2019-001 [LHCb-DP-2019-001] | Run 2 trigger performance
LHCb-DP-2018-004 [LHCb-DP-2018-004] | ReDecay
LHCb-DP-2018-003 [LHCb-DP-2018-003] | Radiation damage in TT
LHCb-DP-2018-002 [LHCb-DP-2018-002] | VeLo material map using SMOG
LHCb-DP-2018-001 [LHCb-DP-2018-001] | PIDCalib for Run 2 (use Ref. [LHCb-PUB-2016-021] for Run 1)
LHCb-DP-2017-001 [LHCb-DP-2017-001] | Performance of the Outer Tracker — Run 2
LHCb-DP-2016-003 [LHCb-DP-2016-003] | HeRSCheL
LHCb-DP-2016-001 [LHCb-DP-2016-001] | TESLA project — Run 2
LHCb-DP-2014-002 [LHCb-DP-2014-002] | LHCb detector performance
LHCb-DP-2014-001 [LHCb-DP-2014-001] | Performance of the LHCb Vertex Locator
LHCb-DP-2013-003 [LHCb-DP-2013-003] | Performance of the LHCb Outer Tracker — Run 1
LHCb-DP-2013-002 [LHCb-DP-2013-002] | Measurement of the track reconstruction efficiency at LHCb
LHCb-DP-2013-001 [LHCb-DP-2013-001] | Performance of the muon identification at LHCb
LHCb-DP-2012-005 [LHCb-DP-2012-005] | Radiation damage in the LHCb Vertex Locator
LHCb-DP-2012-004 [LHCb-DP-2012-004] | The LHCb trigger and its performance in 2011
LHCb-DP-2012-003 [LHCb-DP-2012-003] | Performance of the LHCb RICH detector at the LHC
LHCb-DP-2012-002 [LHCb-DP-2012-002] | Performance of the LHCb muon system
LHCb-DP-2012-001 [LHCb-DP-2012-001] | Radiation hardness of the LHCb Outer Tracker
LHCb-DP-2011-002 [LHCb-DP-2011-002] | Simulation of machine induced background …
LHCb-DP-2011-001 [LHCb-DP-2011-001] | Performance of the LHCb muon system with cosmic rays
LHCb-DP-2010-001 [LHCb-DP-2010-001] | First spatial alignment of the LHCb VELO …
LHCb-DP-2008-001 [LHCb-DP-2008-001] |  LHCb detector
Table 4: LHCb TDRs. LHCb-TDR number | Title
---|---
LHCb-TDR-021 [LHCb-TDR-021] | Allen
LHCb-TDR-020 [LHCb-TDR-020] | SMOG Upgrade
LHCb-TDR-018 [LHCb-TDR-018] | Upgrade computing model
LHCb-PII-Physics [LHCb-PII-Physics] | Phase-II upgrade physics case
LHCb-PII-EoI [LHCb-PII-EoI] | Expression of interest for Phase-II upgrade
LHCb-TDR-017 [LHCb-TDR-017] | Upgrade software and computing
LHCb-TDR-016 [LHCb-TDR-016] | Trigger and online upgrade
LHCb-TDR-015 [LHCb-TDR-015] | Tracker upgrade
LHCb-TDR-014 [LHCb-TDR-014] | PID upgrade
LHCb-TDR-013 [LHCb-TDR-013] | VELO upgrade
LHCb-TDR-012 [LHCb-TDR-012] | Framework TDR for the upgrade
LHCb-TDR-011 [LHCb-TDR-011] | Computing
LHCb-TDR-010 [LHCb-TDR-010] | Trigger
LHCb-TDR-009 [LHCb-TDR-009] | Reoptimized detector
LHCb-TDR-008 [LHCb-TDR-008] | Inner Tracker
LHCb-TDR-007 [LHCb-TDR-007] | Online, DAQ, ECS
LHCb-TDR-006 [LHCb-TDR-006] | Outer Tracker
LHCb-TDR-005 [LHCb-TDR-005] | VELO
LHCb-TDR-004 [LHCb-TDR-004] | Muon system
LHCb-TDR-003 [LHCb-TDR-003] | RICH
LHCb-TDR-002 [LHCb-TDR-002] | Calorimeters
LHCb-TDR-001 [LHCb-TDR-001] | Magnet
Table 5: LHCb-PAPERs (which have their identifier as their cite code). DNE: Does not exist.  LHCb-PAPER-2020-045 [LHCb-PAPER-2020-045] |  LHCb-PAPER-2020-044 [LHCb-PAPER-2020-044] |  LHCb-PAPER-2020-043 [LHCb-PAPER-2020-043] |  LHCb-PAPER-2020-042 [LHCb-PAPER-2020-042] |  LHCb-PAPER-2020-041 [LHCb-PAPER-2020-041]
---|---|---|---|---
LHCb-PAPER-2020-040 [LHCb-PAPER-2020-040] |  LHCb-PAPER-2020-039 [LHCb-PAPER-2020-039] |  LHCb-PAPER-2020-038 [LHCb-PAPER-2020-038] |  LHCb-PAPER-2020-037 [LHCb-PAPER-2020-037] |  LHCb-PAPER-2020-036 [LHCb-PAPER-2020-036]
LHCb-PAPER-2020-035 [LHCb-PAPER-2020-035] |  LHCb-PAPER-2020-034 [LHCb-PAPER-2020-034] |  LHCb-PAPER-2020-033 [LHCb-PAPER-2020-033] |  LHCb-PAPER-2020-032 [LHCb-PAPER-2020-032] |  LHCb-PAPER-2020-031 [LHCb-PAPER-2020-031]
LHCb-PAPER-2020-030 [LHCb-PAPER-2020-030] |  LHCb-PAPER-2020-029 [LHCb-PAPER-2020-029] |  LHCb-PAPER-2020-028 [LHCb-PAPER-2020-028] |  LHCb-PAPER-2020-027 [LHCb-PAPER-2020-027] |  LHCb-PAPER-2020-026 [LHCb-PAPER-2020-026]
LHCb-PAPER-2020-025 [LHCb-PAPER-2020-025] |  LHCb-PAPER-2020-024 [LHCb-PAPER-2020-024] |  LHCb-PAPER-2020-023 [LHCb-PAPER-2020-023] |  LHCb-PAPER-2020-022 [LHCb-PAPER-2020-022] |  LHCb-PAPER-2020-021 [LHCb-PAPER-2020-021]
LHCb-PAPER-2020-020 [LHCb-PAPER-2020-020] |  LHCb-PAPER-2020-019 [LHCb-PAPER-2020-019] |  LHCb-PAPER-2020-018 [LHCb-PAPER-2020-018] |  LHCb-PAPER-2020-017 [LHCb-PAPER-2020-017] |  LHCb-PAPER-2020-016 [LHCb-PAPER-2020-016]
LHCb-PAPER-2020-015 [LHCb-PAPER-2020-015] |  LHCb-PAPER-2020-014 [LHCb-PAPER-2020-014] |  LHCb-PAPER-2020-013 [LHCb-PAPER-2020-013] |  LHCb-PAPER-2020-012 [LHCb-PAPER-2020-012] |  LHCb-PAPER-2020-011 [LHCb-PAPER-2020-011]
LHCb-PAPER-2020-010 [LHCb-PAPER-2020-010] |  LHCb-PAPER-2020-009 [LHCb-PAPER-2020-009] |  LHCb-PAPER-2020-008 [LHCb-PAPER-2020-008] |  LHCb-PAPER-2020-007 [LHCb-PAPER-2020-007] |  LHCb-PAPER-2020-006 [LHCb-PAPER-2020-006]
LHCb-PAPER-2020-005 [LHCb-PAPER-2020-005] |  LHCb-PAPER-2020-004 [LHCb-PAPER-2020-004] |  LHCb-PAPER-2020-003 [LHCb-PAPER-2020-003] |  LHCb-PAPER-2020-002 [LHCb-PAPER-2020-002] |  LHCb-PAPER-2020-001 [LHCb-PAPER-2020-001]
LHCb-PAPER-2019-046 [LHCb-PAPER-2019-046] |  |  |  |
LHCb-PAPER-2019-045 [LHCb-PAPER-2019-045] |  LHCb-PAPER-2019-044 [LHCb-PAPER-2019-044] |  LHCb-PAPER-2019-043 [LHCb-PAPER-2019-043] |  LHCb-PAPER-2019-042 [LHCb-PAPER-2019-042] |  LHCb-PAPER-2019-041 [LHCb-PAPER-2019-041]
LHCb-PAPER-2019-040 [LHCb-PAPER-2019-040] |  LHCb-PAPER-2019-039 [LHCb-PAPER-2019-039] |  LHCb-PAPER-2019-038 [LHCb-PAPER-2019-038] |  LHCb-PAPER-2019-037 [LHCb-PAPER-2019-037] |  LHCb-PAPER-2019-036 [LHCb-PAPER-2019-036]
LHCb-PAPER-2019-035 [LHCb-PAPER-2019-035] |  LHCb-PAPER-2019-034 [LHCb-PAPER-2019-034] |  LHCb-PAPER-2019-033 [LHCb-PAPER-2019-033] |  LHCb-PAPER-2019-032 [LHCb-PAPER-2019-032] |  LHCb-PAPER-2019-031 [LHCb-PAPER-2019-031]
LHCb-PAPER-2019-030 [LHCb-PAPER-2019-030] |  LHCb-PAPER-2019-029 [LHCb-PAPER-2019-029] |  LHCb-PAPER-2019-028 [LHCb-PAPER-2019-028] |  LHCb-PAPER-2019-027 [LHCb-PAPER-2019-027] |  LHCb-PAPER-2019-026 [LHCb-PAPER-2019-026]
LHCb-PAPER-2019-025 [LHCb-PAPER-2019-025] |  LHCb-PAPER-2019-024 [LHCb-PAPER-2019-024] |  LHCb-PAPER-2019-023 [LHCb-PAPER-2019-023] |  LHCb-PAPER-2019-022 [LHCb-PAPER-2019-022] |  LHCb-PAPER-2019-021 [LHCb-PAPER-2019-021]
LHCb-PAPER-2019-020 [LHCb-PAPER-2019-020] |  LHCb-PAPER-2019-019 [LHCb-PAPER-2019-019] |  LHCb-PAPER-2019-018 [LHCb-PAPER-2019-018] |  LHCb-PAPER-2019-017 [LHCb-PAPER-2019-017] |  LHCb-PAPER-2019-016 [LHCb-PAPER-2019-016]
LHCb-PAPER-2019-015 [LHCb-PAPER-2019-015] |  LHCb-PAPER-2019-014 [LHCb-PAPER-2019-014] |  LHCb-PAPER-2019-013 [LHCb-PAPER-2019-013] |  LHCb-PAPER-2019-012 [LHCb-PAPER-2019-012] |  LHCb-PAPER-2019-011 [LHCb-PAPER-2019-011]
LHCb-PAPER-2019-010 [LHCb-PAPER-2019-010] |  LHCb-PAPER-2019-009 [LHCb-PAPER-2019-009] |  LHCb-PAPER-2019-008 [LHCb-PAPER-2019-008] |  LHCb-PAPER-2019-007 [LHCb-PAPER-2019-007] |  LHCb-PAPER-2019-006 [LHCb-PAPER-2019-006]
LHCb-PAPER-2019-005 [LHCb-PAPER-2019-005] |  LHCb-PAPER-2019-004 [LHCb-PAPER-2019-004] |  LHCb-PAPER-2019-003 [LHCb-PAPER-2019-003] |  LHCb-PAPER-2019-002 [LHCb-PAPER-2019-002] |  LHCb-PAPER-2019-001 [LHCb-PAPER-2019-001]
LHCb-PAPER-2018-051 [LHCb-PAPER-2018-051] |  |  |  |
LHCb-PAPER-2018-050 [LHCb-PAPER-2018-050] |  LHCb-PAPER-2018-049 [LHCb-PAPER-2018-049] |  LHCb-PAPER-2018-048 [LHCb-PAPER-2018-048] |  LHCb-PAPER-2018-047 [LHCb-PAPER-2018-047] |  LHCb-PAPER-2018-046 [LHCb-PAPER-2018-046]
LHCb-PAPER-2018-045 [LHCb-PAPER-2018-045] |  LHCb-PAPER-2018-044 [LHCb-PAPER-2018-044] |  LHCb-PAPER-2018-043 [LHCb-PAPER-2018-043] |  LHCb-PAPER-2018-042 [LHCb-PAPER-2018-042] |  LHCb-PAPER-2018-041 [LHCb-PAPER-2018-041]
LHCb-PAPER-2018-040 [LHCb-PAPER-2018-040] |  LHCb-PAPER-2018-039 [LHCb-PAPER-2018-039] |  LHCb-PAPER-2018-038 [LHCb-PAPER-2018-038] |  LHCb-PAPER-2018-037 [LHCb-PAPER-2018-037] |  LHCb-PAPER-2018-036 [LHCb-PAPER-2018-036]
LHCb-PAPER-2018-035 [LHCb-PAPER-2018-035] |  LHCb-PAPER-2018-034 [LHCb-PAPER-2018-034] |  LHCb-PAPER-2018-033 [LHCb-PAPER-2018-033] |  LHCb-PAPER-2018-032 [LHCb-PAPER-2018-032] |  LHCb-PAPER-2018-031 [LHCb-PAPER-2018-031]
LHCb-PAPER-2018-030 [LHCb-PAPER-2018-030] |  LHCb-PAPER-2018-029 [LHCb-PAPER-2018-029] |  LHCb-PAPER-2018-028 [LHCb-PAPER-2018-028] |  LHCb-PAPER-2018-027 [LHCb-PAPER-2018-027] |  LHCb-PAPER-2018-026 [LHCb-PAPER-2018-026]
LHCb-PAPER-2018-025 [LHCb-PAPER-2018-025] |  LHCb-PAPER-2018-024 [LHCb-PAPER-2018-024] |  LHCb-PAPER-2018-023 [LHCb-PAPER-2018-023] |  LHCb-PAPER-2018-022 [LHCb-PAPER-2018-022] |  LHCb-PAPER-2018-021 [LHCb-PAPER-2018-021]
LHCb-PAPER-2018-020 [LHCb-PAPER-2018-020] |  LHCb-PAPER-2018-019 [LHCb-PAPER-2018-019] |  LHCb-PAPER-2018-018 [LHCb-PAPER-2018-018] |  LHCb-PAPER-2018-017 [LHCb-PAPER-2018-017] |  LHCb-PAPER-2018-016 [LHCb-PAPER-2018-016]
LHCb-PAPER-2018-015 [LHCb-PAPER-2018-015] |  LHCb-PAPER-2018-014 [LHCb-PAPER-2018-014] |  LHCb-PAPER-2018-013 [LHCb-PAPER-2018-013] |  LHCb-PAPER-2018-012 [LHCb-PAPER-2018-012] |  LHCb-PAPER-2018-011 [LHCb-PAPER-2018-011]
LHCb-PAPER-2018-010 [LHCb-PAPER-2018-010] |  LHCb-PAPER-2018-009 [LHCb-PAPER-2018-009] |  LHCb-PAPER-2018-008 [LHCb-PAPER-2018-008] |  LHCb-PAPER-2018-007 [LHCb-PAPER-2018-007] |  LHCb-PAPER-2018-006 [LHCb-PAPER-2018-006]
LHCb-PAPER-2018-005 [LHCb-PAPER-2018-005] |  LHCb-PAPER-2018-004 [LHCb-PAPER-2018-004] |  LHCb-PAPER-2018-003 [LHCb-PAPER-2018-003] |  LHCb-PAPER-2018-002 [LHCb-PAPER-2018-002] |  LHCb-PAPER-2018-001 [LHCb-PAPER-2018-001]
LHCb-PAPER-2017-050 [LHCb-PAPER-2017-050] |  LHCb-PAPER-2017-049 [LHCb-PAPER-2017-049] |  LHCb-PAPER-2017-048 [LHCb-PAPER-2017-048] |  LHCb-PAPER-2017-047 [LHCb-PAPER-2017-047] |  LHCb-PAPER-2017-046 [LHCb-PAPER-2017-046]
LHCb-PAPER-2017-045 [LHCb-PAPER-2017-045] |  LHCb-PAPER-2017-044 [LHCb-PAPER-2017-044] |  LHCb-PAPER-2017-043 [LHCb-PAPER-2017-043] |  LHCb-PAPER-2017-042 [LHCb-PAPER-2017-042] |  LHCb-PAPER-2017-041 [LHCb-PAPER-2017-041]
LHCb-PAPER-2017-040 [LHCb-PAPER-2017-040] |  LHCb-PAPER-2017-039 [LHCb-PAPER-2017-039] |  LHCb-PAPER-2017-038 [LHCb-PAPER-2017-038] |  LHCb-PAPER-2017-037 [LHCb-PAPER-2017-037] |  LHCb-PAPER-2017-036 [LHCb-PAPER-2017-036]
LHCb-PAPER-2017-035 [LHCb-PAPER-2017-035] |  LHCb-PAPER-2017-034 [LHCb-PAPER-2017-034] |  LHCb-PAPER-2017-033 [LHCb-PAPER-2017-033] |  LHCb-PAPER-2017-032 [LHCb-PAPER-2017-032] |  LHCb-PAPER-2017-031 [LHCb-PAPER-2017-031]
LHCb-PAPER-2017-030 [LHCb-PAPER-2017-030] |  LHCb-PAPER-2017-029 [LHCb-PAPER-2017-029] |  LHCb-PAPER-2017-028 [LHCb-PAPER-2017-028] |  LHCb-PAPER-2017-027 [LHCb-PAPER-2017-027] |  LHCb-PAPER-2017-026 [LHCb-PAPER-2017-026]
LHCb-PAPER-2017-025 [LHCb-PAPER-2017-025] |  LHCb-PAPER-2017-024 [LHCb-PAPER-2017-024] |  LHCb-PAPER-2017-023 [LHCb-PAPER-2017-023] |  LHCb-PAPER-2017-022 [LHCb-PAPER-2017-022] |  LHCb-PAPER-2017-021 [LHCb-PAPER-2017-021]
LHCb-PAPER-2017-020 [LHCb-PAPER-2017-020] |  LHCb-PAPER-2017-019 [LHCb-PAPER-2017-019] |  LHCb-PAPER-2017-018 [LHCb-PAPER-2017-018] |  LHCb-PAPER-2017-017 [LHCb-PAPER-2017-017] |  LHCb-PAPER-2017-016 [LHCb-PAPER-2017-016]
LHCb-PAPER-2017-015 [LHCb-PAPER-2017-015] |  LHCb-PAPER-2017-014 [LHCb-PAPER-2017-014] |  LHCb-PAPER-2017-013 [LHCb-PAPER-2017-013] |  LHCb-PAPER-2017-012 [LHCb-PAPER-2017-012] |  LHCb-PAPER-2017-011 [LHCb-PAPER-2017-011]
LHCb-PAPER-2017-010 [LHCb-PAPER-2017-010] |  LHCb-PAPER-2017-009 [LHCb-PAPER-2017-009] |  LHCb-PAPER-2017-008 [LHCb-PAPER-2017-008] |  LHCb-PAPER-2017-007 [LHCb-PAPER-2017-007] |  LHCb-PAPER-2017-006 [LHCb-PAPER-2017-006]
LHCb-PAPER-2017-005 [LHCb-PAPER-2017-005] |  LHCb-PAPER-2017-004 [LHCb-PAPER-2017-004] |  LHCb-PAPER-2017-003 [LHCb-PAPER-2017-003] |  LHCb-PAPER-2017-002 [LHCb-PAPER-2017-002] |  LHCb-PAPER-2017-001 [LHCb-PAPER-2017-001]
LHCb-PAPER-2016-065 [LHCb-PAPER-2016-065] |  LHCb-PAPER-2016-064 [LHCb-PAPER-2016-064] |  LHCb-PAPER-2016-063 [LHCb-PAPER-2016-063] |  LHCb-PAPER-2016-062 [LHCb-PAPER-2016-062] |  LHCb-PAPER-2016-061 [LHCb-PAPER-2016-061]
LHCb-PAPER-2016-060 [LHCb-PAPER-2016-060] |  LHCb-PAPER-2016-059 [LHCb-PAPER-2016-059] |  LHCb-PAPER-2016-058 [LHCb-PAPER-2016-058] |  LHCb-PAPER-2016-057 [LHCb-PAPER-2016-057] |  LHCb-PAPER-2016-056 [LHCb-PAPER-2016-056]
LHCb-PAPER-2016-055 [LHCb-PAPER-2016-055] |  LHCb-PAPER-2016-054 [LHCb-PAPER-2016-054] |  LHCb-PAPER-2016-053 [LHCb-PAPER-2016-053] |  LHCb-PAPER-2016-052 [LHCb-PAPER-2016-052] |  LHCb-PAPER-2016-051 [LHCb-PAPER-2016-051]
LHCb-PAPER-2016-050 [LHCb-PAPER-2016-050] |  LHCb-PAPER-2016-049 [LHCb-PAPER-2016-049] |  LHCb-PAPER-2016-048 [LHCb-PAPER-2016-048] |  LHCb-PAPER-2016-047 [LHCb-PAPER-2016-047] |  LHCb-PAPER-2016-046 [LHCb-PAPER-2016-046]
LHCb-PAPER-2016-045 [LHCb-PAPER-2016-045] |  LHCb-PAPER-2016-044 [LHCb-PAPER-2016-044] |  LHCb-PAPER-2016-043 [LHCb-PAPER-2016-043] |  LHCb-PAPER-2016-042 [LHCb-PAPER-2016-042] |  LHCb-PAPER-2016-041 [LHCb-PAPER-2016-041]
LHCb-PAPER-2016-040 [LHCb-PAPER-2016-040] |  LHCb-PAPER-2016-039 [LHCb-PAPER-2016-039] |  LHCb-PAPER-2016-038 [LHCb-PAPER-2016-038] |  LHCb-PAPER-2016-037 [LHCb-PAPER-2016-037] |  LHCb-PAPER-2016-036 [LHCb-PAPER-2016-036]
LHCb-PAPER-2016-035 [LHCb-PAPER-2016-035] |  LHCb-PAPER-2016-034 [LHCb-PAPER-2016-034] |  LHCb-PAPER-2016-033 [LHCb-PAPER-2016-033] |  LHCb-PAPER-2016-032 [LHCb-PAPER-2016-032] |  LHCb-PAPER-2016-031 [LHCb-PAPER-2016-031]
LHCb-PAPER-2016-030 [LHCb-PAPER-2016-030] |  LHCb-PAPER-2016-029 [LHCb-PAPER-2016-029] |  LHCb-PAPER-2016-028 [LHCb-PAPER-2016-028] |  LHCb-PAPER-2016-027 [LHCb-PAPER-2016-027] |  LHCb-PAPER-2016-026 [LHCb-PAPER-2016-026]
LHCb-PAPER-2016-025 [LHCb-PAPER-2016-025] |  LHCb-PAPER-2016-024 [LHCb-PAPER-2016-024] |  LHCb-PAPER-2016-023 [LHCb-PAPER-2016-023] |  LHCb-PAPER-2016-022 [LHCb-PAPER-2016-022] |  LHCb-PAPER-2016-021 [LHCb-PAPER-2016-021]
LHCb-PAPER-2016-020 [LHCb-PAPER-2016-020] |  LHCb-PAPER-2016-019 [LHCb-PAPER-2016-019] |  LHCb-PAPER-2016-018 [LHCb-PAPER-2016-018] |  LHCb-PAPER-2016-017 [LHCb-PAPER-2016-017] |  LHCb-PAPER-2016-016 [LHCb-PAPER-2016-016]
LHCb-PAPER-2016-015 [LHCb-PAPER-2016-015] |  LHCb-PAPER-2016-014 [LHCb-PAPER-2016-014] |  LHCb-PAPER-2016-013 [LHCb-PAPER-2016-013] |  LHCb-PAPER-2016-012 [LHCb-PAPER-2016-012] |  LHCb-PAPER-2016-011 [LHCb-PAPER-2016-011]
LHCb-PAPER-2016-010 [LHCb-PAPER-2016-010] |  LHCb-PAPER-2016-009 [LHCb-PAPER-2016-009] |  LHCb-PAPER-2016-008 [LHCb-PAPER-2016-008] |  LHCb-PAPER-2016-007 [LHCb-PAPER-2016-007] |  LHCb-PAPER-2016-006 [LHCb-PAPER-2016-006]
LHCb-PAPER-2016-005 [LHCb-PAPER-2016-005] |  LHCb-PAPER-2016-004 [LHCb-PAPER-2016-004] |  LHCb-PAPER-2016-003 [LHCb-PAPER-2016-003] |  LHCb-PAPER-2016-002 [LHCb-PAPER-2016-002] |  LHCb-PAPER-2016-001 [LHCb-PAPER-2016-001]
LHCb-PAPER-2015-060 [LHCb-PAPER-2015-060] |  LHCb-PAPER-2015-059 [LHCb-PAPER-2015-059] |  LHCb-PAPER-2015-058 [LHCb-PAPER-2015-058] |  LHCb-PAPER-2015-057 [LHCb-PAPER-2015-057] |  LHCb-PAPER-2015-056 [LHCb-PAPER-2015-056]
LHCb-PAPER-2015-055 [LHCb-PAPER-2015-055] |  LHCb-PAPER-2015-054 [LHCb-PAPER-2015-054] |  LHCb-PAPER-2015-053 [LHCb-PAPER-2015-053] |  LHCb-PAPER-2015-052 [LHCb-PAPER-2015-052] |  LHCb-PAPER-2015-051 [LHCb-PAPER-2015-051]
LHCb-PAPER-2015-050 [LHCb-PAPER-2015-050] |  LHCb-PAPER-2015-049 [LHCb-PAPER-2015-049] |  LHCb-PAPER-2015-048 [LHCb-PAPER-2015-048] |  LHCb-PAPER-2015-047 [LHCb-PAPER-2015-047] |  LHCb-PAPER-2015-046 [LHCb-PAPER-2015-046]
LHCb-PAPER-2015-045 [LHCb-PAPER-2015-045] |  LHCb-PAPER-2015-044 [LHCb-PAPER-2015-044] |  LHCb-PAPER-2015-043 [LHCb-PAPER-2015-043] |  LHCb-PAPER-2015-042 [LHCb-PAPER-2015-042] |  LHCb-PAPER-2015-041 [LHCb-PAPER-2015-041]
LHCb-PAPER-2015-040 [LHCb-PAPER-2015-040] |  LHCb-PAPER-2015-039 [LHCb-PAPER-2015-039] |  LHCb-PAPER-2015-038 [LHCb-PAPER-2015-038] |  LHCb-PAPER-2015-037 [LHCb-PAPER-2015-037] |  LHCb-PAPER-2015-036 [LHCb-PAPER-2015-036]
LHCb-PAPER-2015-035 [LHCb-PAPER-2015-035] |  LHCb-PAPER-2015-034 [LHCb-PAPER-2015-034] |  LHCb-PAPER-2015-033 [LHCb-PAPER-2015-033] |  LHCb-PAPER-2015-032 [LHCb-PAPER-2015-032] |  LHCb-PAPER-2015-031 [LHCb-PAPER-2015-031]
LHCb-PAPER-2015-030 [LHCb-PAPER-2015-030] |  LHCb-PAPER-2015-029 [LHCb-PAPER-2015-029] |  LHCb-PAPER-2015-028 [LHCb-PAPER-2015-028] |  LHCb-PAPER-2015-027 [LHCb-PAPER-2015-027] |  LHCb-PAPER-2015-026 [LHCb-PAPER-2015-026]
LHCb-PAPER-2015-025 [LHCb-PAPER-2015-025] |  LHCb-PAPER-2015-024 [LHCb-PAPER-2015-024] |  LHCb-PAPER-2015-023 [LHCb-PAPER-2015-023] |  LHCb-PAPER-2015-022 [LHCb-PAPER-2015-022] |  LHCb-PAPER-2015-021 [LHCb-PAPER-2015-021]
LHCb-PAPER-2015-020 [LHCb-PAPER-2015-020] |  LHCb-PAPER-2015-019 [LHCb-PAPER-2015-019] |  LHCb-PAPER-2015-018 [LHCb-PAPER-2015-018] |  LHCb-PAPER-2015-017 [LHCb-PAPER-2015-017] |  LHCb-PAPER-2015-016 [LHCb-PAPER-2015-016]
LHCb-PAPER-2015-015 [LHCb-PAPER-2015-015] |  LHCb-PAPER-2015-014 [LHCb-PAPER-2015-014] |  LHCb-PAPER-2015-013 [LHCb-PAPER-2015-013] |  LHCb-PAPER-2015-012 [LHCb-PAPER-2015-012] |  LHCb-PAPER-2015-011 [LHCb-PAPER-2015-011]
LHCb-PAPER-2015-010 [LHCb-PAPER-2015-010] |  LHCb-PAPER-2015-009 [LHCb-PAPER-2015-009] |  LHCb-PAPER-2015-008 [LHCb-PAPER-2015-008] |  LHCb-PAPER-2015-007 [LHCb-PAPER-2015-007] |  LHCb-PAPER-2015-006 [LHCb-PAPER-2015-006]
LHCb-PAPER-2015-005 [LHCb-PAPER-2015-005] |  LHCb-PAPER-2015-004 [LHCb-PAPER-2015-004] |  LHCb-PAPER-2015-003 [LHCb-PAPER-2015-003] |  LHCb-PAPER-2015-002 [LHCb-PAPER-2015-002] |  LHCb-PAPER-2015-001 [LHCb-PAPER-2015-001]
LHCb-PAPER-2014-070 [LHCb-PAPER-2014-070] |  LHCb-PAPER-2014-069 [LHCb-PAPER-2014-069] |  LHCb-PAPER-2014-068 [LHCb-PAPER-2014-068] |  LHCb-PAPER-2014-067 [LHCb-PAPER-2014-067] |  LHCb-PAPER-2014-066 [LHCb-PAPER-2014-066]
LHCb-PAPER-2014-065 [LHCb-PAPER-2014-065] |  LHCb-PAPER-2014-064 [LHCb-PAPER-2014-064] |  LHCb-PAPER-2014-063 [LHCb-PAPER-2014-063] |  LHCb-PAPER-2014-062 [LHCb-PAPER-2014-062] |  LHCb-PAPER-2014-061 [LHCb-PAPER-2014-061]
LHCb-PAPER-2014-060 [LHCb-PAPER-2014-060] |  LHCb-PAPER-2014-059 [LHCb-PAPER-2014-059] |  LHCb-PAPER-2014-058 [LHCb-PAPER-2014-058] |  LHCb-PAPER-2014-057 [LHCb-PAPER-2014-057] |  LHCb-PAPER-2014-056 [LHCb-PAPER-2014-056]
LHCb-PAPER-2014-055 [LHCb-PAPER-2014-055] |  LHCb-PAPER-2014-054 [LHCb-PAPER-2014-054] |  LHCb-PAPER-2014-053 [LHCb-PAPER-2014-053] |  LHCb-PAPER-2014-052 [LHCb-PAPER-2014-052] |  LHCb-PAPER-2014-051 [LHCb-PAPER-2014-051]
LHCb-PAPER-2014-050 [LHCb-PAPER-2014-050] |  LHCb-PAPER-2014-049 [LHCb-PAPER-2014-049] |  LHCb-PAPER-2014-048 [LHCb-PAPER-2014-048] |  LHCb-PAPER-2014-047 [LHCb-PAPER-2014-047] |  LHCb-PAPER-2014-046 [LHCb-PAPER-2014-046]
LHCb-PAPER-2014-045 [LHCb-PAPER-2014-045] |  LHCb-PAPER-2014-044 [LHCb-PAPER-2014-044] |  LHCb-PAPER-2014-043 [LHCb-PAPER-2014-043] |  LHCb-PAPER-2014-042 [LHCb-PAPER-2014-042] |  LHCb-PAPER-2014-041 [LHCb-PAPER-2014-041]
LHCb-PAPER-2014-040 [LHCb-PAPER-2014-040] |  LHCb-PAPER-2014-039 [LHCb-PAPER-2014-039] |  LHCb-PAPER-2014-038 [LHCb-PAPER-2014-038] |  LHCb-PAPER-2014-037 [LHCb-PAPER-2014-037] |  LHCb-PAPER-2014-036 [LHCb-PAPER-2014-036]
LHCb-PAPER-2014-035 [LHCb-PAPER-2014-035] |  LHCb-PAPER-2014-034 [LHCb-PAPER-2014-034] |  LHCb-PAPER-2014-033 [LHCb-PAPER-2014-033] |  LHCb-PAPER-2014-032 [LHCb-PAPER-2014-032] |  LHCb-PAPER-2014-031 [LHCb-PAPER-2014-031]
LHCb-PAPER-2014-030 [LHCb-PAPER-2014-030] |  LHCb-PAPER-2014-029 [LHCb-PAPER-2014-029] |  LHCb-PAPER-2014-028 [LHCb-PAPER-2014-028] |  LHCb-PAPER-2014-027 [LHCb-PAPER-2014-027] |  LHCb-PAPER-2014-026 [LHCb-PAPER-2014-026]
LHCb-PAPER-2014-025 [LHCb-PAPER-2014-025] |  LHCb-PAPER-2014-024 [LHCb-PAPER-2014-024] |  LHCb-PAPER-2014-023 [LHCb-PAPER-2014-023] |  LHCb-PAPER-2014-022 [LHCb-PAPER-2014-022] |  LHCb-PAPER-2014-021 [LHCb-PAPER-2014-021]
LHCb-PAPER-2014-020 [LHCb-PAPER-2014-020] |  LHCb-PAPER-2014-019 [LHCb-PAPER-2014-019] |  LHCb-PAPER-2014-018 [LHCb-PAPER-2014-018] |  LHCb-PAPER-2014-017 [LHCb-PAPER-2014-017] |  LHCb-PAPER-2014-016 [LHCb-PAPER-2014-016]
LHCb-PAPER-2014-015 [LHCb-PAPER-2014-015] |  LHCb-PAPER-2014-014 [LHCb-PAPER-2014-014] |  LHCb-PAPER-2014-013 [LHCb-PAPER-2014-013] |  LHCb-PAPER-2014-012 [LHCb-PAPER-2014-012] |  LHCb-PAPER-2014-011 [LHCb-PAPER-2014-011]
LHCb-PAPER-2014-010 [LHCb-PAPER-2014-010] |  LHCb-PAPER-2014-009 [LHCb-PAPER-2014-009] |  LHCb-PAPER-2014-008 [LHCb-PAPER-2014-008] |  LHCb-PAPER-2014-007 [LHCb-PAPER-2014-007] |  LHCb-PAPER-2014-006 [LHCb-PAPER-2014-006]
LHCb-PAPER-2014-005 [LHCb-PAPER-2014-005] |  LHCb-PAPER-2014-004 [LHCb-PAPER-2014-004] |  LHCb-PAPER-2014-003 [LHCb-PAPER-2014-003] |  LHCb-PAPER-2014-002 [LHCb-PAPER-2014-002] |  LHCb-PAPER-2014-001 [LHCb-PAPER-2014-001]
LHCb-PAPER-2013-070 [LHCb-PAPER-2013-070] |  LHCb-PAPER-2013-069 [LHCb-PAPER-2013-069] |  LHCb-PAPER-2013-068 [LHCb-PAPER-2013-068] |  LHCb-PAPER-2013-067 [LHCb-PAPER-2013-067] |  LHCb-PAPER-2013-066 [LHCb-PAPER-2013-066]
LHCb-PAPER-2013-065 [LHCb-PAPER-2013-065] |  LHCb-PAPER-2013-064 [LHCb-PAPER-2013-064] |  LHCb-PAPER-2013-063 [LHCb-PAPER-2013-063] |  LHCb-PAPER-2013-062 [LHCb-PAPER-2013-062] |  LHCb-PAPER-2013-061 [LHCb-PAPER-2013-061]
LHCb-PAPER-2013-060 [LHCb-PAPER-2013-060] |  LHCb-PAPER-2013-059 [LHCb-PAPER-2013-059] |  LHCb-PAPER-2013-058 [LHCb-PAPER-2013-058] |  LHCb-PAPER-2013-057 [LHCb-PAPER-2013-057] |  LHCb-PAPER-2013-056 [LHCb-PAPER-2013-056]
LHCb-PAPER-2013-055 [LHCb-PAPER-2013-055] |  LHCb-PAPER-2013-054 [LHCb-PAPER-2013-054] |  LHCb-PAPER-2013-053 [LHCb-PAPER-2013-053] |  LHCb-PAPER-2013-052 [LHCb-PAPER-2013-052] |  LHCb-PAPER-2013-051 [LHCb-PAPER-2013-051]
LHCb-PAPER-2013-050 [LHCb-PAPER-2013-050] |  LHCb-PAPER-2013-049 [LHCb-PAPER-2013-049] |  LHCb-PAPER-2013-048 [LHCb-PAPER-2013-048] |  LHCb-PAPER-2013-047 [LHCb-PAPER-2013-047] |  LHCb-PAPER-2013-046 [LHCb-PAPER-2013-046]
LHCb-PAPER-2013-045 [LHCb-PAPER-2013-045] |  LHCb-PAPER-2013-044 [LHCb-PAPER-2013-044] |  LHCb-PAPER-2013-043 [LHCb-PAPER-2013-043] |  LHCb-PAPER-2013-042 [LHCb-PAPER-2013-042] |  LHCb-PAPER-2013-041 [LHCb-PAPER-2013-041]
LHCb-PAPER-2013-040 [LHCb-PAPER-2013-040] |  LHCb-PAPER-2013-039 [LHCb-PAPER-2013-039] |  LHCb-PAPER-2013-038 [LHCb-PAPER-2013-038] |  LHCb-PAPER-2013-037 [LHCb-PAPER-2013-037] |  LHCb-PAPER-2013-036 [LHCb-PAPER-2013-036]
LHCb-PAPER-2013-035 [LHCb-PAPER-2013-035] |  LHCb-PAPER-2013-034 [LHCb-PAPER-2013-034] |  LHCb-PAPER-2013-033 [LHCb-PAPER-2013-033] |  LHCb-PAPER-2013-032 [LHCb-PAPER-2013-032] |  LHCb-PAPER-2013-031 [LHCb-PAPER-2013-031]
LHCb-PAPER-2013-030 [LHCb-PAPER-2013-030] |  LHCb-PAPER-2013-029 [LHCb-PAPER-2013-029] |  LHCb-PAPER-2013-028 [LHCb-PAPER-2013-028] |  LHCb-PAPER-2013-027 [LHCb-PAPER-2013-027] |  LHCb-PAPER-2013-026 [LHCb-PAPER-2013-026]
LHCb-PAPER-2013-025 [LHCb-PAPER-2013-025] |  LHCb-PAPER-2013-024 [LHCb-PAPER-2013-024] |  LHCb-PAPER-2013-023 [LHCb-PAPER-2013-023] |  LHCb-PAPER-2013-022 [LHCb-PAPER-2013-022] |  LHCb-PAPER-2013-021 [LHCb-PAPER-2013-021]
LHCb-PAPER-2013-020 [LHCb-PAPER-2013-020] |  LHCb-PAPER-2013-019 [LHCb-PAPER-2013-019] |  LHCb-PAPER-2013-018 [LHCb-PAPER-2013-018] |  LHCb-PAPER-2013-017 [LHCb-PAPER-2013-017] |  LHCb-PAPER-2013-016 [LHCb-PAPER-2013-016]
LHCb-PAPER-2013-015 [LHCb-PAPER-2013-015] |  LHCb-PAPER-2013-014 [LHCb-PAPER-2013-014] |  LHCb-PAPER-2013-013 [LHCb-PAPER-2013-013] |  LHCb-PAPER-2013-012 [LHCb-PAPER-2013-012] |  LHCb-PAPER-2013-011 [LHCb-PAPER-2013-011]
LHCb-PAPER-2013-010 [LHCb-PAPER-2013-010] |  LHCb-PAPER-2013-009 [LHCb-PAPER-2013-009] |  LHCb-PAPER-2013-008 [LHCb-PAPER-2013-008] |  LHCb-PAPER-2013-007 [LHCb-PAPER-2013-007] |  LHCb-PAPER-2013-006 [LHCb-PAPER-2013-006]
LHCb-PAPER-2013-005 [LHCb-PAPER-2013-005] |  LHCb-PAPER-2013-004 [LHCb-PAPER-2013-004] |  LHCb-PAPER-2013-003 [LHCb-PAPER-2013-003] |  LHCb-PAPER-2013-002 [LHCb-PAPER-2013-002] |  LHCb-PAPER-2013-001 [LHCb-PAPER-2013-001]
LHCb-PAPER-2012-057 [LHCb-PAPER-2012-057] |  LHCb-PAPER-2012-056 [LHCb-PAPER-2012-056] |  |  |
LHCb-PAPER-2012-055 [LHCb-PAPER-2012-055] |  LHCb-PAPER-2012-054 [LHCb-PAPER-2012-054] |  LHCb-PAPER-2012-053 [LHCb-PAPER-2012-053] |  LHCb-PAPER-2012-052 [LHCb-PAPER-2012-052] |  LHCb-PAPER-2012-051 [LHCb-PAPER-2012-051]
LHCb-PAPER-2012-050 [LHCb-PAPER-2012-050] |  LHCb-PAPER-2012-049 [LHCb-PAPER-2012-049] |  LHCb-PAPER-2012-048 [LHCb-PAPER-2012-048] |  LHCb-PAPER-2012-047 [LHCb-PAPER-2012-047] |  LHCb-PAPER-2012-046 [LHCb-PAPER-2012-046]
LHCb-PAPER-2012-045 [LHCb-PAPER-2012-045] |  LHCb-PAPER-2012-044 [LHCb-PAPER-2012-044] |  LHCb-PAPER-2012-043 [LHCb-PAPER-2012-043] |  LHCb-PAPER-2012-042 [LHCb-PAPER-2012-042] |  LHCb-PAPER-2012-041 [LHCb-PAPER-2012-041]
LHCb-PAPER-2012-040 [LHCb-PAPER-2012-040] |  LHCb-PAPER-2012-039 [LHCb-PAPER-2012-039] |  LHCb-PAPER-2012-038 [LHCb-PAPER-2012-038] |  LHCb-PAPER-2012-037 [LHCb-PAPER-2012-037] |  LHCb-PAPER-2012-036 [LHCb-PAPER-2012-036]
LHCb-PAPER-2012-035 [LHCb-PAPER-2012-035] |  LHCb-PAPER-2012-034 [LHCb-PAPER-2012-034] |  LHCb-PAPER-2012-033 [LHCb-PAPER-2012-033] |  LHCb-PAPER-2012-032 [LHCb-PAPER-2012-032] |  LHCb-PAPER-2012-031 [LHCb-PAPER-2012-031]
LHCb-PAPER-2012-030 [LHCb-PAPER-2012-030] |  LHCb-PAPER-2012-029 [LHCb-PAPER-2012-029] |  LHCb-PAPER-2012-028 [LHCb-PAPER-2012-028] |  LHCb-PAPER-2012-027 [LHCb-PAPER-2012-027] |  LHCb-PAPER-2012-026 [LHCb-PAPER-2012-026]
LHCb-PAPER-2012-025 [LHCb-PAPER-2012-025] |  LHCb-PAPER-2012-024 [LHCb-PAPER-2012-024] |  LHCb-PAPER-2012-023 [LHCb-PAPER-2012-023] |  LHCb-PAPER-2012-022 [LHCb-PAPER-2012-022] |  LHCb-PAPER-2012-021 [LHCb-PAPER-2012-021]
LHCb-PAPER-2012-020 [LHCb-PAPER-2012-020] |  LHCb-PAPER-2012-019 [LHCb-PAPER-2012-019] |  LHCb-PAPER-2012-018 [LHCb-PAPER-2012-018] |  LHCb-PAPER-2012-017 [LHCb-PAPER-2012-017] |  LHCb-PAPER-2012-016 [LHCb-PAPER-2012-016]
LHCb-PAPER-2012-015 [LHCb-PAPER-2012-015] |  LHCb-PAPER-2012-014 [LHCb-PAPER-2012-014] |  LHCb-PAPER-2012-013 [LHCb-PAPER-2012-013] |  LHCb-PAPER-2012-012 [LHCb-PAPER-2012-012] |  LHCb-PAPER-2012-011 [LHCb-PAPER-2012-011]
LHCb-PAPER-2012-010 [LHCb-PAPER-2012-010] |  LHCb-PAPER-2012-009 [LHCb-PAPER-2012-009] |  LHCb-PAPER-2012-008 [LHCb-PAPER-2012-008] |  LHCb-PAPER-2012-007 [LHCb-PAPER-2012-007] |  LHCb-PAPER-2012-006 [LHCb-PAPER-2012-006]
LHCb-PAPER-2012-005 [LHCb-PAPER-2012-005] |  LHCb-PAPER-2012-004 [LHCb-PAPER-2012-004] |  LHCb-PAPER-2012-003 [LHCb-PAPER-2012-003] |  LHCb-PAPER-2012-002 [LHCb-PAPER-2012-002] |  LHCb-PAPER-2012-001 [LHCb-PAPER-2012-001]
LHCb-PAPER-2011-045 [LHCb-PAPER-2011-045] |  LHCb-PAPER-2011-044 [LHCb-PAPER-2011-044] |  LHCb-PAPER-2011-043 [LHCb-PAPER-2011-043] |  LHCb-PAPER-2011-042 [LHCb-PAPER-2011-042] |  LHCb-PAPER-2011-041 [LHCb-PAPER-2011-041]
LHCb-PAPER-2011-040 [LHCb-PAPER-2011-040] | LHCb-PAPER-2011-039666LHCb-PAPER-2011-039 does not exist. |  LHCb-PAPER-2011-038 [LHCb-PAPER-2011-038] |  LHCb-PAPER-2011-037 [LHCb-PAPER-2011-037] |  LHCb-PAPER-2011-036 [LHCb-PAPER-2011-036]
LHCb-PAPER-2011-035 [LHCb-PAPER-2011-035] |  LHCb-PAPER-2011-034 [LHCb-PAPER-2011-034] |  LHCb-PAPER-2011-033 [LHCb-PAPER-2011-033] |  LHCb-PAPER-2011-032 [LHCb-PAPER-2011-032] |  LHCb-PAPER-2011-031 [LHCb-PAPER-2011-031]
LHCb-PAPER-2011-030 [LHCb-PAPER-2011-030] |  LHCb-PAPER-2011-029 [LHCb-PAPER-2011-029] |  LHCb-PAPER-2011-028 [LHCb-PAPER-2011-028] |  LHCb-PAPER-2011-027 [LHCb-PAPER-2011-027] |  LHCb-PAPER-2011-026 [LHCb-PAPER-2011-026]
LHCb-PAPER-2011-025 [LHCb-PAPER-2011-025] |  LHCb-PAPER-2011-024 [LHCb-PAPER-2011-024] |  LHCb-PAPER-2011-023 [LHCb-PAPER-2011-023] |  LHCb-PAPER-2011-022 [LHCb-PAPER-2011-022] |  LHCb-PAPER-2011-021 [LHCb-PAPER-2011-021]
LHCb-PAPER-2011-020 [LHCb-PAPER-2011-020] |  LHCb-PAPER-2011-019 [LHCb-PAPER-2011-019] |  LHCb-PAPER-2011-018 [LHCb-PAPER-2011-018] |  LHCb-PAPER-2011-017 [LHCb-PAPER-2011-017] |  LHCb-PAPER-2011-016 [LHCb-PAPER-2011-016]
LHCb-PAPER-2011-015 [LHCb-PAPER-2011-015] |  LHCb-PAPER-2011-014 [LHCb-PAPER-2011-014] |  LHCb-PAPER-2011-013 [LHCb-PAPER-2011-013] |  LHCb-PAPER-2011-012 [LHCb-PAPER-2011-012] |  LHCb-PAPER-2011-011 [LHCb-PAPER-2011-011]
LHCb-PAPER-2011-010 [LHCb-PAPER-2011-010] |  LHCb-PAPER-2011-009 [LHCb-PAPER-2011-009] |  LHCb-PAPER-2011-008 [LHCb-PAPER-2011-008] |  LHCb-PAPER-2011-007 [LHCb-PAPER-2011-007] |  LHCb-PAPER-2011-006 [LHCb-PAPER-2011-006]
LHCb-PAPER-2011-005 [LHCb-PAPER-2011-005] |  LHCb-PAPER-2011-004 [LHCb-PAPER-2011-004] |  LHCb-PAPER-2011-003 [LHCb-PAPER-2011-003] |  LHCb-PAPER-2011-002 [LHCb-PAPER-2011-002] |  LHCb-PAPER-2011-001 [LHCb-PAPER-2011-001]
LHCb-PAPER-2010-002 [LHCb-PAPER-2010-002] |  LHCb-PAPER-2010-001 [LHCb-PAPER-2010-001] |  |  |
Table 6: LHCb-CONFs (which have their identifier as their cite code). Most CONF notes have been superseded by a paper and are thus retired. This is indicated in the bibtex entry. Do not cite retired CONF notes. DNE: Does not exist.  LHCb-CONF-2020-005 [LHCb-CONF-2020-005] |  LHCb-CONF-2020-004 [LHCb-CONF-2020-004] |  LHCb-CONF-2020-003 [LHCb-CONF-2020-003] |  LHCb-CONF-2020-002 [LHCb-CONF-2020-002] |  LHCb-CONF-2020-001 [LHCb-CONF-2020-001]
---|---|---|---|---
LHCb-CONF-2019-005 [LHCb-CONF-2019-005] |  LHCb-CONF-2019-004 [LHCb-CONF-2019-004] |  LHCb-CONF-2019-003 [LHCb-CONF-2019-003] |  LHCb-CONF-2019-002 [LHCb-CONF-2019-002] |  LHCb-CONF-2019-001 [LHCb-CONF-2019-001]
LHCb-CONF-2018-006 [LHCb-CONF-2018-006] |  |  |  |
LHCb-CONF-2018-005 [LHCb-CONF-2018-005] |  LHCb-CONF-2018-004 [LHCb-CONF-2018-004] |  LHCb-CONF-2018-003 [LHCb-CONF-2018-003] |  LHCb-CONF-2018-002 [LHCb-CONF-2018-002]777If you cite the gamma combination, always also cite the latest gamma paper as \cite{LHCb-PAPER-2013-020,*LHCb-CONF-2018-002} (unless you cite LHCb-PAPER-2013-020 separately too). |  LHCb-CONF-2018-001 [LHCb-CONF-2018-001]
LHCb-CONF-2017-005 [LHCb-CONF-2017-005] |  LHCb-CONF-2017-004 [LHCb-CONF-2017-004] |  LHCb-CONF-2017-003 [LHCb-CONF-2017-003] |  LHCb-CONF-2017-002 [LHCb-CONF-2017-002] |  LHCb-CONF-2017-001 [LHCb-CONF-2017-001]
LHCb-CONF-2016-018 [LHCb-CONF-2016-018] |  LHCb-CONF-2016-016 [LHCb-CONF-2016-016] |  |  |
LHCb-CONF-2016-015 [LHCb-CONF-2016-015] |  LHCb-CONF-2016-014 [LHCb-CONF-2016-014] |  LHCb-CONF-2016-013 [LHCb-CONF-2016-013] |  LHCb-CONF-2016-012 [LHCb-CONF-2016-012] |  LHCb-CONF-2016-011 [LHCb-CONF-2016-011]
LHCb-CONF-2016-010 [LHCb-CONF-2016-010] |  LHCb-CONF-2016-009 [LHCb-CONF-2016-009] |  LHCb-CONF-2016-008 [LHCb-CONF-2016-008] |  LHCb-CONF-2016-007 [LHCb-CONF-2016-007] |  LHCb-CONF-2016-006 [LHCb-CONF-2016-006]
LHCb-CONF-2016-005 [LHCb-CONF-2016-005] |  LHCb-CONF-2016-004 [LHCb-CONF-2016-004] |  LHCb-CONF-2016-003 [LHCb-CONF-2016-003] |  LHCb-CONF-2016-002 [LHCb-CONF-2016-002] |  LHCb-CONF-2016-001 [LHCb-CONF-2016-001]
LHCb-CONF-2015-005 [LHCb-CONF-2015-005] |  LHCb-CONF-2015-004 [LHCb-CONF-2015-004] |  LHCb-CONF-2015-003 [LHCb-CONF-2015-003] |  LHCb-CONF-2015-002 [LHCb-CONF-2015-002] |  LHCb-CONF-2015-001 [LHCb-CONF-2015-001]
LHCb-CONF-2014-004 [LHCb-CONF-2014-004] |  LHCb-CONF-2014-003 [LHCb-CONF-2014-003] |  LHCb-CONF-2014-002 [LHCb-CONF-2014-002] |  LHCb-CONF-2014-001 [LHCb-CONF-2014-001] |
LHCb-CONF-2013-013 [LHCb-CONF-2013-013] |  LHCb-CONF-2013-012 [LHCb-CONF-2013-012] |  LHCb-CONF-2013-011 [LHCb-CONF-2013-011] |  |
LHCb-CONF-2013-010 [LHCb-CONF-2013-010] |  LHCb-CONF-2013-009 [LHCb-CONF-2013-009] |  LHCb-CONF-2013-008 [LHCb-CONF-2013-008] |  LHCb-CONF-2013-007 [LHCb-CONF-2013-007] |  LHCb-CONF-2013-006 [LHCb-CONF-2013-006]
LHCb-CONF-2013-005 [LHCb-CONF-2013-005] |  LHCb-CONF-2013-004 [LHCb-CONF-2013-004] |  LHCb-CONF-2013-003 [LHCb-CONF-2013-003] |  LHCb-CONF-2013-002 [LHCb-CONF-2013-002] |  LHCb-CONF-2013-001 [LHCb-CONF-2013-001]
LHCb-CONF-2012-034 [LHCb-CONF-2012-034] |  LHCb-CONF-2012-033 [LHCb-CONF-2012-033] |  LHCb-CONF-2012-032 [LHCb-CONF-2012-032] |  LHCb-CONF-2012-031 [LHCb-CONF-2012-031] |
LHCb-CONF-2012-030 [LHCb-CONF-2012-030] |  LHCb-CONF-2012-029 [LHCb-CONF-2012-029] |  LHCb-CONF-2012-028 [LHCb-CONF-2012-028] |  LHCb-CONF-2012-027 [LHCb-CONF-2012-027] |  LHCb-CONF-2012-026 [LHCb-CONF-2012-026]
LHCb-CONF-2012-025 [LHCb-CONF-2012-025] |  LHCb-CONF-2012-024 [LHCb-CONF-2012-024] |  LHCb-CONF-2012-023 [LHCb-CONF-2012-023] |  LHCb-CONF-2012-022 [LHCb-CONF-2012-022] |  LHCb-CONF-2012-021 [LHCb-CONF-2012-021]
LHCb-CONF-2012-020 [LHCb-CONF-2012-020] |  LHCb-CONF-2012-019 [LHCb-CONF-2012-019] |  LHCb-CONF-2012-018 [LHCb-CONF-2012-018] |  LHCb-CONF-2012-017 [LHCb-CONF-2012-017] |  LHCb-CONF-2012-016 [LHCb-CONF-2012-016]
LHCb-CONF-2012-015 [LHCb-CONF-2012-015] |  LHCb-CONF-2012-014 [LHCb-CONF-2012-014] |  LHCb-CONF-2012-013 [LHCb-CONF-2012-013] |  LHCb-CONF-2012-012 [LHCb-CONF-2012-012] |  LHCb-CONF-2012-011 [LHCb-CONF-2012-011]
LHCb-CONF-2012-010 [LHCb-CONF-2012-010] |  LHCb-CONF-2012-009 [LHCb-CONF-2012-009] |  LHCb-CONF-2012-008 [LHCb-CONF-2012-008] |  LHCb-CONF-2012-007 [LHCb-CONF-2012-007] |  LHCb-CONF-2012-006 [LHCb-CONF-2012-006]
LHCb-CONF-2012-005 [LHCb-CONF-2012-005] |  LHCb-CONF-2012-004 [LHCb-CONF-2012-004] |  LHCb-CONF-2012-003 [LHCb-CONF-2012-003] |  LHCb-CONF-2012-002 [LHCb-CONF-2012-002] |  LHCb-CONF-2012-001 [LHCb-CONF-2012-001]
LHCb-CONF-2011-062 [LHCb-CONF-2011-062] |  LHCb-CONF-2011-061 [LHCb-CONF-2011-061] |  |  |
LHCb-CONF-2011-060 [LHCb-CONF-2011-060] |  LHCb-CONF-2011-059 [LHCb-CONF-2011-059] |  LHCb-CONF-2011-058 [LHCb-CONF-2011-058] |  LHCb-CONF-2011-057 [LHCb-CONF-2011-057] |  LHCb-CONF-2011-056 [LHCb-CONF-2011-056]
LHCb-CONF-2011-055 [LHCb-CONF-2011-055] |  LHCb-CONF-2011-054 [LHCb-CONF-2011-054] |  LHCb-CONF-2011-053 [LHCb-CONF-2011-053] |  LHCb-CONF-2011-052 [LHCb-CONF-2011-052] |  LHCb-CONF-2011-051 [LHCb-CONF-2011-051]
LHCb-CONF-2011-050 [LHCb-CONF-2011-050] |  LHCb-CONF-2011-049 [LHCb-CONF-2011-049] |  LHCb-CONF-2011-048 [LHCb-CONF-2011-048] |  LHCb-CONF-2011-047 [LHCb-CONF-2011-047] |  LHCb-CONF-2011-046 [LHCb-CONF-2011-046]
LHCb-CONF-2011-045 [LHCb-CONF-2011-045] |  LHCb-CONF-2011-044 [LHCb-CONF-2011-044] |  LHCb-CONF-2011-043 [LHCb-CONF-2011-043] |  LHCb-CONF-2011-042 [LHCb-CONF-2011-042] |  LHCb-CONF-2011-041 [LHCb-CONF-2011-041]
LHCb-CONF-2011-040 [LHCb-CONF-2011-040] |  LHCb-CONF-2011-039 [LHCb-CONF-2011-039] |  LHCb-CONF-2011-038 [LHCb-CONF-2011-038] |  LHCb-CONF-2011-037 [LHCb-CONF-2011-037] |  LHCb-CONF-2011-036 [LHCb-CONF-2011-036]
LHCb-CONF-2011-035 [LHCb-CONF-2011-035] |  LHCb-CONF-2011-034 [LHCb-CONF-2011-034] |  LHCb-CONF-2011-033 [LHCb-CONF-2011-033] |  LHCb-CONF-2011-032 DNE |  LHCb-CONF-2011-031 [LHCb-CONF-2011-031]
LHCb-CONF-2011-030 [LHCb-CONF-2011-030] |  LHCb-CONF-2011-029 [LHCb-CONF-2011-029] |  LHCb-CONF-2011-028 [LHCb-CONF-2011-028] |  LHCb-CONF-2011-027 [LHCb-CONF-2011-027] |  LHCb-CONF-2011-026 [LHCb-CONF-2011-026]
LHCb-CONF-2011-025 [LHCb-CONF-2011-025] |  LHCb-CONF-2011-024 [LHCb-CONF-2011-024] |  LHCb-CONF-2011-023 [LHCb-CONF-2011-023] |  LHCb-CONF-2011-022 [LHCb-CONF-2011-022] |  LHCb-CONF-2011-021 [LHCb-CONF-2011-021]
LHCb-CONF-2011-020 [LHCb-CONF-2011-020] |  LHCb-CONF-2011-019 [LHCb-CONF-2011-019] |  LHCb-CONF-2011-018 [LHCb-CONF-2011-018] |  LHCb-CONF-2011-017 [LHCb-CONF-2011-017] |  LHCb-CONF-2011-016 [LHCb-CONF-2011-016]
LHCb-CONF-2011-015 [LHCb-CONF-2011-015] |  LHCb-CONF-2011-014 [LHCb-CONF-2011-014] |  LHCb-CONF-2011-013 [LHCb-CONF-2011-013] |  LHCb-CONF-2011-012 [LHCb-CONF-2011-012] |  LHCb-CONF-2011-011 [LHCb-CONF-2011-011]
LHCb-CONF-2011-010 [LHCb-CONF-2011-010] |  LHCb-CONF-2011-009 [LHCb-CONF-2011-009] |  LHCb-CONF-2011-008 [LHCb-CONF-2011-008] |  LHCb-CONF-2011-007 [LHCb-CONF-2011-007] |  LHCb-CONF-2011-006 [LHCb-CONF-2011-006]
LHCb-CONF-2011-005 [LHCb-CONF-2011-005] |  LHCb-CONF-2011-004 [LHCb-CONF-2011-004] |  LHCb-CONF-2011-003 [LHCb-CONF-2011-003] |  LHCb-CONF-2011-002 [LHCb-CONF-2011-002] |  LHCb-CONF-2011-001 [LHCb-CONF-2011-001]
LHCb-CONF-2010-014 [LHCb-CONF-2010-014] |  LHCb-CONF-2010-013 [LHCb-CONF-2010-013] |  LHCb-CONF-2010-012 [LHCb-CONF-2010-012] |  LHCb-CONF-2010-011 [LHCb-CONF-2010-011] |
LHCb-CONF-2010-010 [LHCb-CONF-2010-010] |  LHCb-CONF-2010-009 [LHCb-CONF-2010-009] |  LHCb-CONF-2010-008 [LHCb-CONF-2010-008] |  |
Earlier documents in LHCb-CONF series are actually proceedings.

##  Appendix B Standard symbols

As explained in Sect. LABEL:sec:typography this appendix contains standard
typesetting of symbols, particle names, units etc. in LHCb documents.

In the file lhcb-symbols-def.tex, which is included, a large number of symbols
is defined. While they can lead to quicker typing, the main reason is to
ensure a uniform notation within a document and between different LHCb
documents. If a symbol like \CP to typeset $C\\!P$ violation is available for
a unit, particle name, process or whatever, it should be used. If you do not
agree with the notation you should ask to get the definition in lhcb-symbols-
def.tex changed rather than just ignoring it.

All the main particles have been given symbols. The $\mathrm{B}$ mesons are
thus named ${{\mathrm{B}}^{+}}$, ${\mathrm{B}}^{0}$,
${\mathrm{B}}^{0}_{\mathrm{s}}$, and ${\mathrm{B}}_{\mathrm{c}}^{+}$. There is
no need to go into math mode to use particle names, thus saving the typing of
many $ signs. By default particle names are typeset in italic type to agree
with the PDG preference. To get roman particle names you can just change
\setboolean{uprightparticles}{false} to true at the top of this template.

There is a large number of units typeset that ensures the correct use of
fonts, capitals and spacing. As an example we have
${m_{{{\mathrm{B}}^{0}_{\mathrm{s}}}}}=5366.3\pm
0.6\text{\,Me\kern-1.00006ptV\\!/}c^{2}$. Note that $\,\mu\text{m}$ is typeset
with an upright $\upmu$, even if the particle names have slanted Greek
letters.

A set of useful symbols are defined for working groups. More of these symbols
can be included later. As an example in the Rare Decay group we have several
different analyses looking for a measurement of
$\mathcal{C}_{7}^{{}^{\prime}\mathrm{(eff)}}$ and
$\mathcal{O}_{7.}^{{}^{\prime}}$

##  Appendix C List of all symbols

###  C.1 Experiments

\lhcb | LHCb | \atlas | ATLAS | \cms | CMS
---|---|---|---|---|---
\alice | ALICE | \babar | BaBar | \belle | Belle
\belletwo | Belle II | \besiii | BESIII | \cleo | CLEO
\cdf | CDF | \dzero | D0 | \aleph | ALEPH
\delphi | DELPHI | \opal | OPAL | \lthree | L3
\sld | SLD | \cern | CERN | \lhc | LHC
\lep | LEP | \tevatron | Tevatron | \bfactories | $\mathrm{B}$ Factories
\bfactory | $\mathrm{B}$ Factory | \upgradeone | Upgrade I | \upgradetwo | Upgrade II

####  C.1.1 LHCb sub-detectors and sub-systems

\velo | VELO | \rich | RICH | \richone | RICH1
---|---|---|---|---|---
\richtwo | RICH2 | \ttracker | TT | \intr | IT
\st | ST | \ot | OT | \herschel | HeRSCheL
\spd | SPD | \presh | PS | \ecal | ECAL
\hcal | HCAL | \MagUp | MagUp | \MagDown | MagDown
\ode | ODE | \daq | DAQ | \tfc | TFC
\ecs | ECS | \lone | L0 | \hlt | HLT
\hltone | HLT1 | \hlttwo | HLT2 |  |

###  C.2 Particles

####  C.2.1 Leptons

\electron | $\mathrm{e}$ | \en | $\mathrm{e}^{-}$ | \ep | $\mathrm{e}^{+}$
---|---|---|---|---|---
\epm | $\mathrm{e}^{\pm}$ | \emp | $\mathrm{e}^{\mp}$ | \epem | $\mathrm{e}^{+}\mathrm{e}^{-}$
\muon | $\upmu$ | \mup | $\upmu^{+}$ | \mun | $\upmu^{-}$
\mupm | $\upmu^{\pm}$ | \mump | $\upmu^{\mp}$ | \mumu | $\upmu^{+}\upmu^{-}$
\tauon | $\uptau$ | \taup | $\uptau^{+}$ | \taum | $\uptau^{-}$
\taupm | $\uptau^{\pm}$ | \taump | $\uptau^{\mp}$ | \tautau | $\uptau^{+}\uptau^{-}$
\lepton | $\ell$ | \ellm | $\ell^{-}$ | \ellp | $\ell^{+}$
\ellpm | $\ell^{\pm}$ | \ellmp | $\ell^{\mp}$ | \ellell | $\ell^{+}\ell^{-}$
\neu | $\upnu$ | \neub | $\overline{\upnu}$ | \neue | ${\upnu}_{e}$
\neueb | ${\overline{\upnu}}_{e}$ | \neum | ${\upnu}_{\mu}$ | \neumb | ${\overline{\upnu}}_{\mu}$
\neut | ${\upnu}_{\tau}$ | \neutb | ${\overline{\upnu}}_{\tau}$ | \neul | ${\upnu}_{\ell}$
\neulb | ${\overline{\upnu}}_{\ell}$ |  |  |  |

####  C.2.2 Gauge bosons and scalars

\g | $\upgamma$ | \H | $\mathrm{H}^{0}$ | \Hp | $\mathrm{H}^{+}$
---|---|---|---|---|---
\Hm | $\mathrm{H}^{-}$ | \Hpm | $\mathrm{H}^{\pm}$ | \W | $\mathrm{W}$
\Wp | $\mathrm{W}^{+}$ | \Wm | $\mathrm{W}^{-}$ | \Wpm | $\mathrm{W}^{\pm}$
\Z | $\mathrm{Z}$ |  |  |  |

####  C.2.3 Quarks

\quark | $\mathrm{q}$ | \quarkbar | $\overline{\mathrm{q}}$ | \qqbar | ${\mathrm{q}}{\overline{\mathrm{q}}}$
---|---|---|---|---|---
\uquark | $\mathrm{u}$ | \uquarkbar | $\overline{\mathrm{u}}$ | \uubar | ${\mathrm{u}}{\overline{\mathrm{u}}}$
\dquark | $\mathrm{d}$ | \dquarkbar | $\overline{\mathrm{d}}$ | \ddbar | ${\mathrm{d}}{\overline{\mathrm{d}}}$
\squark | $\mathrm{s}$ | \squarkbar | $\overline{\mathrm{s}}$ | \ssbar | ${\mathrm{s}}{\overline{\mathrm{s}}}$
\cquark | $\mathrm{c}$ | \cquarkbar | $\overline{\mathrm{c}}$ | \ccbar | ${\mathrm{c}}{\overline{\mathrm{c}}}$
\bquark | $\mathrm{b}$ | \bquarkbar | $\overline{\mathrm{b}}$ | \bbbar | ${\mathrm{b}}{\overline{\mathrm{b}}}$
\tquark | $\mathrm{t}$ | \tquarkbar | $\overline{\mathrm{t}}$ | \ttbar | ${\mathrm{t}}{\overline{\mathrm{t}}}$

####  C.2.4 Light mesons

\hadron | $\mathrm{h}$ | \pion | $\uppi$ | \piz | ${\uppi}^{0}$
---|---|---|---|---|---
\pip | ${\uppi}^{+}$ | \pim | ${\uppi}^{-}$ | \pipm | ${\uppi}^{\pm}$
\pimp | ${\uppi}^{\mp}$ | \rhomeson | $\uprho$ | \rhoz | ${\uprho}^{0}$
\rhop | ${\uprho}^{+}$ | \rhom | ${\uprho}^{-}$ | \rhopm | ${\uprho}^{\pm}$
\rhomp | ${\uprho}^{\mp}$ | \kaon | $\mathrm{K}$ | \Kbar | $\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}$
\Kb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}$ | \KorKbar |  ( ) [-.7ex] $\kern 0.0pt\mathrm{K}$ | \Kz | ${\mathrm{K}}^{0}$
\Kzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{0}$ | \Kp | ${\mathrm{K}}^{+}$ | \Km | ${\mathrm{K}}^{-}$
\Kpm | ${\mathrm{K}}^{\pm}$ | \Kmp | ${\mathrm{K}}^{\mp}$ | \KS | ${\mathrm{K}}^{0}_{\mathrm{S}}$
\Vzero | $V^{0}$ | \KL | ${\mathrm{K}}^{0}_{\mathrm{L}}$ | \Kstarz | ${\mathrm{K}}^{*0}$
\Kstarzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}$ | \Kstar | ${\mathrm{K}}^{*}$ | \Kstarb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*}$
\Kstarp | ${\mathrm{K}}^{*+}$ | \Kstarm | ${\mathrm{K}}^{*-}$ | \Kstarpm | ${\mathrm{K}}^{*\pm}$
\Kstarmp | ${\mathrm{K}}^{*\mp}$ | \KorKbarz | $\kern 0.0pt\shortstack{{(\rule[2.15277pt]{12.50002pt}{0.51212pt})} \\\ [-.7ex] $\kern 0.0pt\mathrm{K}$}{}^{0}$ | \etaz | $\upeta$
\etapr | $\upeta^{\prime}$ | \phiz | $\upphi$ | \omegaz | $\upomega$

####  C.2.5 Charmed mesons

\Dbar | $\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}$ | \D | $\mathrm{D}$ | \Db | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}$
---|---|---|---|---|---
\DorDbar |  ( ) [-.7ex] $\kern 0.0pt\mathrm{D}$ | \Dz | ${\mathrm{D}}^{0}$ | \Dzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{0}$
\Dp | ${\mathrm{D}}^{+}$ | \Dm | ${\mathrm{D}}^{-}$ | \Dpm | ${\mathrm{D}}^{\pm}$
\Dmp | ${\mathrm{D}}^{\mp}$ | \DpDm | ${{\mathrm{D}}^{+}}{\kern-1.60004pt{{\mathrm{D}}^{-}}}$ | \Dstar | ${\mathrm{D}}^{*}$
\Dstarb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{*}$ | \Dstarz | ${\mathrm{D}}^{*0}$ | \Dstarzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}{}^{*0}$
\theDstarz | ${\mathrm{D}}^{*}(2007)^{0}$ | \theDstarzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{D}}}^{*}(2007)^{0}$ | \Dstarp | ${\mathrm{D}}^{*+}$
\Dstarm | ${\mathrm{D}}^{*-}$ | \Dstarpm | ${\mathrm{D}}^{*\pm}$ | \Dstarmp | ${\mathrm{D}}^{*\mp}$
\theDstarp | ${\mathrm{D}}^{*}(2010)^{+}$ | \theDstarm | ${\mathrm{D}}^{*}(2010)^{-}$ | \theDstarpm | ${\mathrm{D}}^{*}(2010)^{\pm}$
\theDstarmp | ${\mathrm{D}}^{*}(2010)^{\mp}$ | \Ds | ${\mathrm{D}}^{+}_{\mathrm{s}}$ | \Dsp | ${\mathrm{D}}^{+}_{\mathrm{s}}$
\Dsm | ${\mathrm{D}}^{-}_{\mathrm{s}}$ | \Dspm | ${\mathrm{D}}^{\pm}_{\mathrm{s}}$ | \Dsmp | ${\mathrm{D}}^{\mp}_{\mathrm{s}}$
\Dss | ${\mathrm{D}}^{*+}_{\mathrm{s}}$ | \Dssp | ${\mathrm{D}}^{*+}_{\mathrm{s}}$ | \Dssm | ${\mathrm{D}}^{*-}_{\mathrm{s}}$
\Dsspm | ${\mathrm{D}}^{*\pm}_{\mathrm{s}}$ | \Dssmp | ${\mathrm{D}}^{*\mp}_{\mathrm{s}}$ |  |

####  C.2.6 Beauty mesons

\B | $\mathrm{B}$ | \Bbar | $\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}$ | \Bb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}$
---|---|---|---|---|---
\BorBbar |  ( ) [-.7ex] $\kern 0.0pt\mathrm{B}$ | \Bz | ${\mathrm{B}}^{0}$ | \Bzb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}$
\Bd | ${\mathrm{B}}^{0}$ | \Bdb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}$ | \BdorBdbar |  ( ) [-.7ex] $\kern 0.0pt{{\mathrm{B}}^{0}}$
\Bu | ${\mathrm{B}}^{+}$ | \Bub | ${\mathrm{B}}^{-}$ | \Bp | ${{\mathrm{B}}^{+}}$
\Bm | ${{\mathrm{B}}^{-}}$ | \Bpm | ${\mathrm{B}}^{\pm}$ | \Bmp | ${\mathrm{B}}^{\mp}$
\Bs | ${\mathrm{B}}^{0}_{\mathrm{s}}$ | \Bsb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}_{\mathrm{s}}$ | \BsorBsbar |  ( ) [-.7ex] $\kern 0.0pt{{\mathrm{B}}^{0}_{\mathrm{s}}}$
\Bc | ${\mathrm{B}}_{\mathrm{c}}^{+}$ | \Bcp | ${\mathrm{B}}_{\mathrm{c}}^{+}$ | \Bcm | ${\mathrm{B}}_{\mathrm{c}}^{-}$
\Bcpm | ${\mathrm{B}}_{\mathrm{c}}^{\pm}$ | \Bds | ${\mathrm{B}}_{({\mathrm{s}})}^{0}$ | \Bdsb | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}_{({\mathrm{s}})}^{0}$
\BdorBs | ${\mathrm{B}}_{({\mathrm{s}})}^{0}$ | \BdorBsbar | ${\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}_{({\mathrm{s}})}^{0}$ |  |

####  C.2.7 Onia

\jpsi | ${\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}$ | \psitwos | $\uppsi{(2S)}$ | \psiprpr | $\uppsi(3770)$
---|---|---|---|---|---
\etac | $\upeta_{\mathrm{c}}$ | \psires | $\uppsi$ | \chic | $\upchi_{\mathrm{c}}$
\chiczero | $\upchi_{{\mathrm{c}}0}$ | \chicone | $\upchi_{{\mathrm{c}}1}$ | \chictwo | $\upchi_{{\mathrm{c}}2}$
\chicJ | $\upchi_{{\mathrm{c}}J}$ | \Upsilonres | $\Upsilon$ | \OneS | $\Upsilon{(1S)}$
\TwoS | $\Upsilon{(2S)}$ | \ThreeS | $\Upsilon{(3S)}$ | \FourS | $\Upsilon{(4S)}$
\FiveS | $\Upsilon{(5S)}$ | \chib | $\upchi_{b}$ | \chibzero | $\upchi_{{\mathrm{b}}0}$
\chibone | $\upchi_{{\mathrm{b}}1}$ | \chibtwo | $\upchi_{{\mathrm{b}}2}$ | \chibJ | $\upchi_{{\mathrm{b}}J}$
\theX | $\upchi_{c1}(3872)$ |  |  |  |

####  C.2.8 Light Baryons

\proton | $\mathrm{p}$ | \antiproton | $\overline{\mathrm{p}}$ | \neutron | $\mathrm{n}$
---|---|---|---|---|---
\antineutron | $\overline{\mathrm{n}}$ | \Deltares | $\Delta$ | \Deltaresbar | $\overline{\Delta}$
\Lz | $\Lambda$ | \Lbar | $\kern 0.0pt\overline{\kern 0.0pt\Lambda}$ | \LorLbar |  ( ) [-.7ex] $\kern 0.0pt\Lambda$
\Lambdares | $\Lambda$ | \Lambdaresbar | ${\kern 0.0pt\overline{\kern 0.0pt\Lambda}}$ | \Sigmares | $\Sigma$
\Sigmaz | ${\Sigma}{}^{0}$ | \Sigmap | ${\Sigma}{}^{+}$ | \Sigmam | ${\Sigma}{}^{-}$
\Sigmaresbar | $\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}$ | \Sigmabarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}{}^{0}$ | \Sigmabarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}{}^{+}$
\Sigmabarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}{}^{-}$ | \Xires | $\Xi$ | \Xiz | ${\Xi}^{0}$
\Xim | ${\Xi}^{-}$ | \Xiresbar | $\kern 0.0pt\overline{\kern 0.0pt{\Xi}}$ | \Xibarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}^{0}$
\Xibarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}^{+}$ | \Omegares | $\Omega$ | \Omegaresbar | $\kern 0.0pt\overline{\kern 0.0pt\Omega}$
\Omegam | ${\Omega}^{-}$ | \Omegabarp | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}^{+}$ |  |

####  C.2.9 Charmed Baryons

\Lc | ${\Lambda}^{+}_{\mathrm{c}}$ | \Lcbar | ${\kern 0.0pt\overline{\kern 0.0pt\Lambda}}{}^{-}_{\mathrm{c}}$ | \Xic | ${\Xi}_{\mathrm{c}}$
---|---|---|---|---|---
\Xicz | ${\Xi}^{0}_{\mathrm{c}}$ | \Xicp | ${\Xi}^{+}_{\mathrm{c}}$ | \Xicbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{c}}$
\Xicbarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{c}}^{0}$ | \Xicbarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{c}}^{-}$ | \Omegac | ${\Omega}^{0}_{\mathrm{c}}$
\Omegacbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{\mathrm{c}}^{0}$ | \Xicc | ${\Xi}_{{\mathrm{c}}{\mathrm{c}}}$ | \Xiccbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{{\mathrm{c}}{\mathrm{c}}}$
\Xiccp | ${\Xi}^{+}_{{\mathrm{c}}{\mathrm{c}}}$ | \Xiccpp | ${\Xi}^{++}_{{\mathrm{c}}{\mathrm{c}}}$ | \Xiccbarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{{\mathrm{c}}{\mathrm{c}}}^{-}$
\Xiccbarmm | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{{\mathrm{c}}{\mathrm{c}}}^{--}$ | \Omegacc | ${\Omega}^{+}_{{\mathrm{c}}{\mathrm{c}}}$ | \Omegaccbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{{\mathrm{c}}{\mathrm{c}}}^{-}$
\Omegaccc | ${\Omega}^{++}_{{\mathrm{c}}{\mathrm{c}}{\mathrm{c}}}$ | \Omegacccbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{{\mathrm{c}}{\mathrm{c}}{\mathrm{c}}}^{--}$ |  |

####  C.2.10 Beauty Baryons

\Lb | ${\Lambda}^{0}_{\mathrm{b}}$ | \Lbbar | ${\kern 0.0pt\overline{\kern 0.0pt\Lambda}}{}^{0}_{\mathrm{b}}$ | \Sigmab | ${\Sigma}_{\mathrm{b}}$
---|---|---|---|---|---
\Sigmabp | ${\Sigma}_{\mathrm{b}}^{+}$ | \Sigmabz | ${\Sigma}_{\mathrm{b}}^{0}$ | \Sigmabm | ${\Sigma}_{\mathrm{b}}^{-}$
\Sigmabpm | ${\Sigma}_{\mathrm{b}}^{\pm}$ | \Sigmabbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}$ | \Sigmabbarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{+}$
\Sigmabbarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{0}$ | \Sigmabbarm | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{-}$ | \Sigmabbarpm | ${\kern 0.0pt\overline{\kern 0.0pt{\Sigma}}}_{\mathrm{b}}^{-}$
\Xib | ${\Xi}_{\mathrm{b}}$ | \Xibz | ${\Xi}^{0}_{\mathrm{b}}$ | \Xibm | ${\Xi}^{-}_{\mathrm{b}}$
\Xibbar | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{b}}$ | \Xibbarz | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{b}}^{0}$ | \Xibbarp | ${\kern 0.0pt\overline{\kern 0.0pt{\Xi}}}{}_{\mathrm{b}}^{+}$
\Omegab | ${\Omega}^{-}_{\mathrm{b}}$ | \Omegabbar | ${\kern 0.0pt\overline{\kern 0.0pt\Omega}}{}_{\mathrm{b}}^{+}$ |  |

###  C.3 Physics symbols

####  C.3.1 Decays

\BF | $\mathcal{B}$ | \BR | $\mathcal{B}$ | \BRvis | ${\mathcal{B}}_{\mathrm{{vis}}}$
---|---|---|---|---|---
\ra | $\rightarrow$ | \to | $\rightarrow$ |  |

####  C.3.2 Lifetimes

\tauBs | $\tau_{{{\mathrm{B}}^{0}_{\mathrm{s}}}}$ | \tauBd | $\tau_{{{\mathrm{B}}^{0}}}$ | \tauBz | $\tau_{{{\mathrm{B}}^{0}}}$
---|---|---|---|---|---
\tauBu | $\tau_{{{{\mathrm{B}}^{+}}}}$ | \tauDp | $\tau_{{{\mathrm{D}}^{+}}}$ | \tauDz | $\tau_{{{\mathrm{D}}^{0}}}$
\tauL | $\tau_{\mathrm{L}}$ | \tauH | $\tau_{\mathrm{H}}$ |  |

####  C.3.3 Masses

\mBd | $m_{{{\mathrm{B}}^{0}}}$ | \mBp | $m_{{{{\mathrm{B}}^{+}}}}$ | \mBs | $m_{{{\mathrm{B}}^{0}_{\mathrm{s}}}}$
---|---|---|---|---|---
\mBc | $m_{{{\mathrm{B}}_{\mathrm{c}}^{+}}}$ | \mLb | $m_{{{\Lambda}^{0}_{\mathrm{b}}}}$ |  |

####  C.3.4 EW theory, groups

\grpsuthree | $\mathrm{SU}(3)$ | \grpsutw | $\mathrm{SU}(2)$ | \grpuone | $\mathrm{U}(1)$
---|---|---|---|---|---
\ssqtw | $\sin^{2}\\!\theta_{\mathrm{W}}$ | \csqtw | $\cos^{2}\\!\theta_{\mathrm{W}}$ | \stw | $\sin\theta_{\mathrm{W}}$
\ctw | $\cos\theta_{\mathrm{W}}$ | \ssqtwef | ${\sin}^{2}\theta_{\mathrm{W}}^{\mathrm{eff}}$ | \csqtwef | ${\cos}^{2}\theta_{\mathrm{W}}^{\mathrm{eff}}$
\stwef | $\sin\theta_{\mathrm{W}}^{\mathrm{eff}}$ | \ctwef | $\cos\theta_{\mathrm{W}}^{\mathrm{eff}}$ | \gv | $g_{\mbox{\tiny V}}$
\ga | $g_{\mbox{\tiny A}}$ | \order | $\mathcal{O}$ | \ordalph | $\mathcal{O}(\alpha)$
\ordalsq | $\mathcal{O}(\alpha^{2})$ | \ordalcb | $\mathcal{O}(\alpha^{3})$ |  |

####  C.3.5 QCD parameters

\as | $\alpha_{s}$ | \MSb | $\overline{\mathrm{MS}}$ | \lqcd | $\Lambda_{\mathrm{QCD}}$
---|---|---|---|---|---
\qsq | $q^{2}$ |  |  |  |

####  C.3.6 CKM, $C\\!P$ violation

\eps | $\varepsilon$ | \epsK | $\varepsilon_{K}$ | \epsB | $\varepsilon_{B}$
---|---|---|---|---|---
\epsp | $\varepsilon^{\prime}_{K}$ | \CP | $C\\!P$ | \CPT | $C\\!PT$
\T | $T$ | \rhobar | $\overline{\rho}$ | \etabar | $\overline{\eta}$
\Vud | $V_{{\mathrm{u}}{\mathrm{d}}}^{\phantom{\ast}}$ | \Vcd | $V_{{\mathrm{c}}{\mathrm{d}}}^{\phantom{\ast}}$ | \Vtd | $V_{{\mathrm{t}}{\mathrm{d}}}^{\phantom{\ast}}$
\Vus | $V_{{\mathrm{u}}{\mathrm{s}}}^{\phantom{\ast}}$ | \Vcs | $V_{{\mathrm{c}}{\mathrm{s}}}^{\phantom{\ast}}$ | \Vts | $V_{{\mathrm{t}}{\mathrm{s}}}^{\phantom{\ast}}$
\Vub | $V_{{\mathrm{u}}{\mathrm{b}}}^{\phantom{\ast}}$ | \Vcb | $V_{{\mathrm{c}}{\mathrm{b}}}^{\phantom{\ast}}$ | \Vtb | $V_{{\mathrm{t}}{\mathrm{b}}}^{\phantom{\ast}}$
\Vuds | $V_{{\mathrm{u}}{\mathrm{d}}}^{\ast}$ | \Vcds | $V_{{\mathrm{c}}{\mathrm{d}}}^{\ast}$ | \Vtds | $V_{{\mathrm{t}}{\mathrm{d}}}^{\ast}$
\Vuss | $V_{{\mathrm{u}}{\mathrm{s}}}^{\ast}$ | \Vcss | $V_{{\mathrm{c}}{\mathrm{s}}}^{\ast}$ | \Vtss | $V_{{\mathrm{t}}{\mathrm{s}}}^{\ast}$
\Vubs | $V_{{\mathrm{u}}{\mathrm{b}}}^{\ast}$ | \Vcbs | $V_{{\mathrm{c}}{\mathrm{b}}}^{\ast}$ | \Vtbs | $V_{{\mathrm{t}}{\mathrm{b}}}^{\ast}$

####  C.3.7 Oscillations

\dm | $\Delta m$ | \dms | $\Delta m_{{\mathrm{s}}}$ | \dmd | $\Delta m_{{\mathrm{d}}}$
---|---|---|---|---|---
\DG | $\Delta\Gamma$ | \DGs | $\Delta\Gamma_{{\mathrm{s}}}$ | \DGd | $\Delta\Gamma_{{\mathrm{d}}}$
\Gs | $\Gamma_{{\mathrm{s}}}$ | \Gd | $\Gamma_{{\mathrm{d}}}$ | \MBq | $M_{{\mathrm{B}}_{\mathrm{q}}}$
\DGq | $\Delta\Gamma_{{\mathrm{q}}}$ | \Gq | $\Gamma_{{\mathrm{q}}}$ | \dmq | $\Delta m_{{\mathrm{q}}}$
\GL | $\Gamma_{\mathrm{L}}$ | \GH | $\Gamma_{\mathrm{H}}$ | \DGsGs | $\Delta\Gamma_{{\mathrm{s}}}/\Gamma_{{\mathrm{s}}}$
\Delm | $\Delta m$ | \ACP | ${\mathcal{A}}^{{C\\!P}}$ | \Adir | ${\mathcal{A}}^{\mathrm{dir}}$
\Amix | ${\mathcal{A}}^{\mathrm{mix}}$ | \ADelta | ${\mathcal{A}}^{\Delta}$ | \phid | $\phi_{{\mathrm{d}}}$
\sinphid | $\sin\\!{\phi_{{\mathrm{d}}}}$ | \phis | $\phi_{{\mathrm{s}}}$ | \betas | $\beta_{{\mathrm{s}}}$
\sbetas | $\sigma(\beta_{{\mathrm{s}}})$ | \stbetas | $\sigma(2\beta_{{\mathrm{s}}})$ | \stphis | $\sigma(\phi_{{\mathrm{s}}})$
\sinphis | $\sin\\!{\phi_{{\mathrm{s}}}}$ |  |  |  |

####  C.3.8 Tagging

\edet | $\varepsilon_{\mathrm{det}}$ | \erec | $\varepsilon_{\mathrm{rec/det}}$ | \esel | $\varepsilon_{\mathrm{sel/rec}}$
---|---|---|---|---|---
\etrg | $\varepsilon_{\mathrm{trg/sel}}$ | \etot | $\varepsilon_{\mathrm{tot}}$ | \mistag | $\omega$
\wcomb | $\omega^{\mathrm{comb}}$ | \etag | $\varepsilon_{\mathrm{tag}}$ | \etagcomb | $\varepsilon_{\mathrm{tag}}^{\mathrm{comb}}$
\effeff | $\varepsilon_{\mathrm{eff}}$ | \effeffcomb | $\varepsilon_{\mathrm{eff}}^{\mathrm{comb}}$ | \efftag | ${\varepsilon_{\mathrm{tag}}}(1-2\omega)^{2}$
\effD | ${\varepsilon_{\mathrm{tag}}}D^{2}$ | \etagprompt | $\varepsilon_{\mathrm{tag}}^{\mathrm{Pr}}$ | \etagLL | $\varepsilon_{\mathrm{tag}}^{\mathrm{LL}}$

####  C.3.9 Key decay channels

\BdToKstmm | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{*0}}{\upmu^{+}}{\upmu^{-}}$ | \BdbToKstmm | ${{\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}}\\!\rightarrow{{\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}}{\upmu^{+}}{\upmu^{-}}$ | \BsToJPsiPhi | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}\phi$
---|---|---|---|---|---
\BdToJPsiKst | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}{{\mathrm{K}}^{*0}}$ | \BdbToJPsiKst | ${{\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}}\\!\rightarrow{{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}{{\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}}$ | \BsPhiGam | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow\phi{\upgamma}$
\BdKstGam | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{*0}}{\upgamma}$ | \BTohh | ${\mathrm{B}}\\!\rightarrow\mathrm{h}^{+}\mathrm{h}^{\prime-}$ | \BdTopipi | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\uppi}^{+}}{{\uppi}^{-}}$
\BdToKpi | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{+}}{{\uppi}^{-}}$ | \BsToKK | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}$ | \BsTopiK | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{{\uppi}^{+}}{{\mathrm{K}}^{-}}$
\Cpipi | $C_{{{\uppi}^{+}}{{\uppi}^{-}}}$ | \Spipi | $S_{{{\uppi}^{+}}{{\uppi}^{-}}}$ | \CKK | $C_{{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}}$
\SKK | $S_{{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}}$ | \ADGKK | $A^{{\Delta\Gamma}}_{{{\mathrm{K}}^{+}}{{\mathrm{K}}^{-}}}$ |  |

####  C.3.10 Rare decays

\BdKstee | ${{\mathrm{B}}^{0}}\\!\rightarrow{{\mathrm{K}}^{*0}}{\mathrm{e}^{+}\mathrm{e}^{-}}$ | \BdbKstee | ${{\kern 0.0pt\overline{\kern 0.0pt\mathrm{B}}}{}^{0}}\\!\rightarrow{{\kern 0.0pt\overline{\kern 0.0pt\mathrm{K}}}{}^{*0}}{\mathrm{e}^{+}\mathrm{e}^{-}}$ | \bsll | ${\mathrm{b}}\\!\rightarrow{\mathrm{s}}\ell^{+}\ell^{-}$
---|---|---|---|---|---
\AFB | $A_{\mathrm{FB}}$ | \FL | $F_{\mathrm{L}}$ | \AT#1 \AT2 | $A_{\mathrm{T}}^{2}$
\btosgam | ${\mathrm{b}}\\!\rightarrow{\mathrm{s}}{\upgamma}$ | \btodgam | ${\mathrm{b}}\\!\rightarrow{\mathrm{d}}{\upgamma}$ | \Bsmm | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{\upmu^{+}}{\upmu^{-}}$
\Bdmm | ${{\mathrm{B}}^{0}}\\!\rightarrow{\upmu^{+}}{\upmu^{-}}$ | \Bsee | ${{\mathrm{B}}^{0}_{\mathrm{s}}}\\!\rightarrow{\mathrm{e}^{+}\mathrm{e}^{-}}$ | \Bdee | ${{\mathrm{B}}^{0}}\\!\rightarrow{\mathrm{e}^{+}\mathrm{e}^{-}}$
\ctl | $\cos{\theta_{\ell}}$ | \ctk | $\cos{\theta_{K}}$ |  |

####  C.3.11 Wilson coefficients and operators

\C#1 \C9 | $\mathcal{C}_{9}$ | \Cp#1 \Cp7 | $\mathcal{C}_{7}^{{}^{\prime}}$ | \Ceff#1 \Ceff9 | $\mathcal{C}_{9}^{\mathrm{(eff)}}$
---|---|---|---|---|---
\Cpeff#1 \Cpeff7 | $\mathcal{C}_{7}^{{}^{\prime}\mathrm{(eff)}}$ | \Ope#1 \Ope2 | $\mathcal{O}_{2}$ | \Opep#1 \Opep7 | $\mathcal{O}_{7}^{{}^{\prime}}$

####  C.3.12 Charm

\xprime | $x^{\prime}$ | \yprime | $y^{\prime}$ | \ycp | $y_{{C\\!P}}$
---|---|---|---|---|---
\agamma | $A_{\Gamma}$ | \dkpicf | ${{\mathrm{D}}^{0}}\\!\rightarrow{{\mathrm{K}}^{-}}{{\uppi}^{+}}$ |  |

####  C.3.13 QM

\bra[1] \bra{a} | $\langle a|$ | \ket[1] \ket{b} | $|b\rangle$ | \braket[2] \braket{a}{b} | $\langle a|b\rangle$
---|---|---|---|---|---

###  C.4 Units (these macros add a small space in front)

\unit[1] \unit{kg} |  kg
---|---

####  C.4.1 Energy and momentum

\tev |  TeV | \gev |  GeV | \mev |  MeV
---|---|---|---|---|---
\kev |  keV | \ev |  eV | \gevgev | $\text{\,Ge\kern-1.00006ptV}^{2}$
\mevc | $\text{\,Me\kern-1.00006ptV\\!/}c$ | \gevc | $\text{\,Ge\kern-1.00006ptV\\!/}c$ | \mevcc | $\text{\,Me\kern-1.00006ptV\\!/}c^{2}$
\gevcc | $\text{\,Ge\kern-1.00006ptV\\!/}c^{2}$ | \gevgevcc | $\text{\,Ge\kern-1.00006ptV}^{2}\\!/c^{2}$ | \gevgevcccc | $\text{\,Ge\kern-1.00006ptV}^{2}\\!/c^{4}$

####  C.4.2 Distance and area (these macros add a small space)

\km |  km | \m |  m | \ma | $\text{\,m}^{2}$
---|---|---|---|---|---
\cm |  cm | \cma | $\text{\,cm}^{2}$ | \mm |  mm
\mma | $\text{\,mm}^{2}$ | \mum | $\,\mu\text{m}$ | \muma | $\,\upmu\text{m}^{2}$
\nm |  nm | \fm |  fm | \barn |  b
\mbarn |  mb | \mub | $\,\upmu\text{b}$ | \nb |  nb
\invnb | $\text{\,nb}^{-1}$ | \pb |  pb | \invpb | $\text{\,pb}^{-1}$
\fb |  fb | \invfb | $\text{\,fb}^{-1}$ | \ab |  ab
\invab | $\text{\,ab}^{-1}$ |  |  |  |

####  C.4.3 Time

\sec |  s | \ms |  ms | \mus | $\,\upmu\text{s}$
---|---|---|---|---|---
\ns |  ns | \ps |  ps | \fs |  fs
\mhz |  MHz | \khz |  kHz | \hz |  Hz
\invps | $\text{\,ps}^{-1}$ | \invns | $\text{\,ns}^{-1}$ | \yr |  yr
\hr |  hr |  |  |  |

####  C.4.4 Temperature

\degc |  ∘C | \degk |  K
---|---|---|---

####  C.4.5 Material lengths, radiation

\Xrad | $X_{0}$ | \NIL | $\lambda_{\rm int}$ | \mip | MIP
---|---|---|---|---|---
\neutroneq | $n_{\text{eq}}$ | \neqcmcm | $n_{\text{eq}}/\text{cm}^{2}$ | \kRad |  kRad
\MRad |  MRad | \ci |  Ci | \mci |  mCi

####  C.4.6 Uncertainties

\sx | $\sigma_{x}$ | \sy | $\sigma_{y}$ | \sz | $\sigma_{z}$
---|---|---|---|---|---
\stat |  (stat) | \syst |  (syst) | \lumi |  (lumi)

####  C.4.7 Maths

\order | $\mathcal{O}$ | \chisq | $\chi^{2}$ | \chisqndf | $\chi^{2}/\mathrm{ndf}$
---|---|---|---|---|---
\chisqip | $\chi^{2}_{\text{IP}}$ | \chisqvs | $\chi^{2}_{\text{VS}}$ | \chisqvtx | $\chi^{2}_{\text{vtx}}$
\chisqvtxndf | $\chi^{2}_{\text{vtx}}/\mathrm{ndf}$ | \deriv | $\mathrm{d}$ | \gsim |  $>$$\sim$
\lsim |  $<$$\sim$ | \mean[1] \mean{x} | $\left\langle x\right\rangle$ | \abs[1] \abs{x} | $\left\|x\right\|$
\Real | $\mathcal{R}e$ | \Imag | $\mathcal{I}m$ | \PDF | PDF
\sPlot | sPlot | \sFit | sFit |  |

###  C.5 Kinematics

####  C.5.1 Energy, Momenta

\Ebeam | $E_{\mbox{\tiny BEAM}}$ | \sqs | $\sqrt{s}$ | \sqsnn | $\sqrt{s_{\scriptscriptstyle\text{NN}}}$
---|---|---|---|---|---
\pt | $p_{\mathrm{T}}$ | \ptsq | $p_{\mathrm{T}}^{2}$ | \ptot | $p$
\et | $E_{\mathrm{T}}$ | \mt | $M_{\mathrm{T}}$ | \dpp | $\Delta p/p$
\msq | $m^{2}$ | \dedx | $\mathrm{d}E/\mathrm{d}x$ |  |

####  C.5.2 PID

\dllkpi | $\mathrm{DLL}_{{\mathrm{K}}{\uppi}}$ | \dllppi | $\mathrm{DLL}_{{\mathrm{p}}{\uppi}}$ | \dllepi | $\mathrm{DLL}_{{\mathrm{e}}{\uppi}}$
---|---|---|---|---|---
\dllmupi | $\mathrm{DLL}_{{\upmu}\pi}$ |  |  |  |

####  C.5.3 Geometry

\degrees | ∘ | \murad | $\,\upmu\text{rad}$ | \mrad |  mrad
---|---|---|---|---|---
\rad |  rad |  |  |  |

####  C.5.4 Accelerator

\betastar | $\beta^{*}$ | \lum | $\mathcal{L}$ | \intlum[1] \intlum{2 $\text{\,fb}^{-1}$ } | $\int\mathcal{L}=2\,\text{\,fb}^{-1}$
---|---|---|---|---|---

###  C.6 Software

####  C.6.1 Programs

\bcvegpy | Bcvegpy | \boole | Boole | \brunel | Brunel
---|---|---|---|---|---
\davinci | DaVinci | \dirac | Dirac | \evtgen | EvtGen
\fewz | Fewz | \fluka | Fluka | \ganga | Ganga
\gaudi | Gaudi | \gauss | Gauss | \geant | Geant4
\hepmc | HepMC | \herwig | Herwig | \moore | Moore
\neurobayes | NeuroBayes | \photos | Photos | \powheg | Powheg
\pythia | Pythia | \resbos | ResBos | \roofit | RooFit
\root | Root | \spice | Spice | \urania | Urania

####  C.6.2 Languages

\cpp | C++ | \ruby | Ruby | \fortran | Fortran
---|---|---|---|---|---
\svn | svn | \git | git | \latex | LaTeX

####  C.6.3 Data processing

\kbit |  kbit | \kbps |  kbit/s | \kbytes |  kB
---|---|---|---|---|---
\kbyps |  kB/s | \mbit |  Mbit | \mbps |  Mbit/s
\mbytes |  MB | \mbyps |  MB/s | \gbit |  Gbit
\gbps |  Gbit/s | \gbytes |  GB | \gbyps |  GB/s
\tbit |  Tbit | \tbps |  Tbit/s | \tbytes |  TB
\tbyps |  TB/s | \dst | DST |  |

###  C.7 Detector related

####  C.7.1 Detector technologies

\nonn | $\mathrm{{\mathit{n^{+}}}\mbox{-}on\mbox{-}{\mathit{n}}}$ | \ponn | $\mathrm{{\mathit{p^{+}}}\mbox{-}on\mbox{-}{\mathit{n}}}$ | \nonp | $\mathrm{{\mathit{n^{+}}}\mbox{-}on\mbox{-}{\mathit{p}}}$
---|---|---|---|---|---
\cvd | CVD | \mwpc | MWPC | \gem | GEM

####  C.7.2 Detector components, electronics

\tell1 | TELL1 | \ukl1 | UKL1 | \beetle | Beetle
---|---|---|---|---|---
\otis | OTIS | \croc | CROC | \carioca | CARIOCA
\dialog | DIALOG | \sync | SYNC | \cardiac | CARDIAC
\gol | GOL | \vcsel | VCSEL | \ttc | TTC
\ttcrx | TTCrx | \hpd | HPD | \pmt | PMT
\specs | SPECS | \elmb | ELMB | \fpga | FPGA
\plc | PLC | \rasnik | RASNIK | \elmb | ELMB
\can | CAN | \lvds | LVDS | \ntc | NTC
\adc | ADC | \led | LED | \ccd | CCD
\hv | HV | \lv | LV | \pvss | PVSS
\cmos | CMOS | \fifo | FIFO | \ccpc | CCPC

####  C.7.3 Chemical symbols

\cfourften | $\mathrm{C_{4}F_{10}}$ | \cffour | $\mathrm{CF_{4}}$ | \cotwo | $\mathrm{CO_{2}}$
---|---|---|---|---|---
\csixffouteen | $\mathrm{C_{6}F_{14}}$ | \mgftwo | $\mathrm{MgF_{2}}$ | \siotwo | $\mathrm{SiO_{2}}$

###  C.8 Special Text

\eg | e.g. | \ie | i.e. | \etal | et al.
---|---|---|---|---|---
\etc | etc. | \cf | cf. | \ffp | ff.
\vs | vs. |  |  |  |

####  C.8.1 Helpful to align numbers in tables

\phz |
---|---

##  Appendix D Supplementary material for LHCb-PAPER-20XX-YYY

This appendix contains supplementary material that will posted on the public
CDS record but will not appear in the paper.

Please leave the above sentence in your draft for first and second circulation
and replace what follows by your actual supplementary material. For more
information about other types of supplementary material, see Section 9. Plots
and tables that follow should be well described, either with captions or with
additional explanatory text.

Figure 5:  Comparison of our result to those from other experiments. Note that
the style of this figure differs slightly from that of Figure
LABEL:fig:example

LHCb collaboration

A. N. Other1.

1University of nowhere

The author list for journal publications is generated from the Membership
Database shortly after ’approval to go to paper’ has been given. It will be
sent to you by email shortly after a paper number has been assigned. The
author list should be included in the draft used for first and second
circulation, to allow new members of the collaboration to verify that they
have been included correctly. Occasionally a misspelled name is corrected, or
associated institutions become full members. Therefore an updated author list
will be sent to you after the final EB review of the paper. In case line
numbering doesn’t work well after including the authorlist, try moving the
`\bigskip` after the last author to a separate line.

The authorship for Conference Reports should be “The LHCb collaboration”, with
a footnote giving the name(s) of the contact author(s), but without the full
list of collaboration names.

The authorship for Figure Reports should be “The LHCb collaboration”, with no
contact author and without the full list of collaboration names.