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 CERN-EP-2023-208 LHCb-PAPER-2023-027

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LHCb collaboration

The production rate of ${{\Lambda}^{0}_{\mathrm{b}}}$ baryons relative to
${{\mathrm{B}}^{0}}$ mesons in $pp$ collisions at a center-of-mass energy
$\sqrt{s}=13\text{\,Te\kern-1.00006ptV}$ is measured by the LHCb experiment.
The ratio of ${{\Lambda}^{0}_{\mathrm{b}}}$ to ${{\mathrm{B}}^{0}}$ production
cross-sections shows a significant dependence on both the transverse momentum
and the measured charged-particle multiplicity. At low multiplicity, the ratio
measured at LHCb is consistent with the value measured in $e^{+}e^{-}$
collisions, and increases by a factor of $\sim 2$ with increasing
multiplicity. At relatively low transverse momentum, the ratio of
${{\Lambda}^{0}_{\mathrm{b}}}$ to ${{\mathrm{B}}^{0}}$ cross-sections is
higher than what is measured in $e^{+}e^{-}$ collisions, but converges with
the $e^{+}e^{-}$ ratio as the momentum increases. These results imply that the
evolution of heavy $b$ quarks into final-state hadrons is influenced by the
density of the hadronic environment produced in the collision. Comparisons
with a statistical hadronization model and implications for the mechanisms
enforcing quark confinement are discussed.

Submitted to Phys. Rev. Lett.

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

One of the defining features of Quantum Chromodynamics (QCD) is color
confinement, which prohibits isolated quarks and gluons from being observed.
Instead, the partons, which carry color charge, are found only as constituents
of color-neutral hadrons [Wilson:1974sk]. Quarks that are produced at
colliders such as the Large Hadron Collider (LHC), evolve into observable
hadrons through a process known as hadronization. Factorization theorems in
QCD typically assume that hadronization is a universal process, independent of
the colliding beam species [Collins:1989gx].

One mechanism of hadronization is fragmentation, where the potential between
outgoing partons grows until it is energetically favorable to produce other
partons from the vacuum that neutralize the initiating parton’s color charge.
This process is often modeled by cluster formation [Andersson:1983ia] or color
string breaking [Webber:1983if]. The resulting collections of particles are
known as jets [Field:1977fa], and have been studied extensively in
$e^{+}e^{-}$, $pp$, $p\bar{p}$, and heavy-ion collisions [Barber:1979yr,
JADE:1986kta, Mueller:1990gy, CDF:1996yow, D0:2008nou, Bhatti:2010bf,
Kogler:2018hem, Connors:2017ptx]. Fragmentation functions, which describe the
evolution of a parton into a jet, are constrained by data from $e^{+}e^{-}$
collisions [Kniehl:2000hk, Metz:2016swz, deFlorian:2007aj].

An alternative hadronization mechanism can arise when quarks that are produced
near each other combine to form color-neutral hadrons through a process called
coalescence. Models of coalescence generally require individual parton
wavefunctions to overlap in position and velocity space, and have successfully
described a range of collider and fixed-target data [Das:1977cp, Vogt:1994zf,
Braaten:2002yt, Rapp:2003wn, He:2019vgs]. In these models, the density of
partons produced in the underlying event has a significant effect on the
hadronization process, and is expected to be especially important in heavy-ion
collisions [Fries:2003kq, Rapp:2003wn]. Enhanced baryon production can be a
signature of coalescence, and models generally require coalescence in order to
reproduce the baryon/meson production cross-section ratios measured in heavy-
ion collisions [Hwa:2002tu, Fries:2003vb, Greco:2003xt]. This alternative
hadronization mechanism does not require fragmentation, and since charged-
particle multiplicity in the underlying event depends on the colliding beam
species, the emergence of coalescence in hadron collisions breaks the
universality of the hadronization process.

The family of hadrons containing bottom quarks is particularly sensitive to
hadronization. Due to their large mass, production of $b$ quarks via
fragmentation is suppressed, and the long wavelengths of heavy $b$ quarks at
low transverse momentum $p_{\mathrm{T}}$ can potentially overlap with other
particles produced in the event. Additionally, there is no $b$-quark content
in the valence quarks of beam particles, and $b$-quark production is dominated
by hard parton-parton interactions in the early stages of the collision,
before hadronization takes place [Norrbin:2000zc]. Total $b\bar{b}$ cross-
sections are consequently well described by perturbative QCD calculations
[LHCb-PAPER-2016-031, LHCb-PAPER-2017-037, ALICE:2021mgk]. Previous
measurements have shown that the fraction of $b$ quarks that hadronize into
baryons has a significant $p_{\mathrm{T}}$ dependence [LHCb-PAPER-2011-018,
LHCb-PAPER-2018-050], and that there is an asymmetry between
${{\Lambda}^{0}_{\mathrm{b}}}$ and ${{\kern 0.0pt\overline{\kern
0.0pt\Lambda}}{}^{0}_{\mathrm{b}}}$ production at the LHC [LHCb-
PAPER-2021-016]. There is also evidence for an increase in the rate of
${{\mathrm{B}}^{0}_{\mathrm{s}}}$ meson production relative to
${{\mathrm{B}}^{0}}$ production with increasing multiplicity at low
$p_{\mathrm{T}}$ [LHCb-PAPER-2022-001]. Additionally, the ALICE collaboration
has shown that the fragmentation fractions for charm quarks vary between
$e^{+}e^{-}$ and $pp$ collisions, with $pp$ data favoring higher
${{\Lambda}^{+}_{\mathrm{c}}}$ baryon production [ALICE:2021dhb], and that the
baryon production is affected by the multiplicity of the underlying event
[ALICE:2021npz]. None of these results are expected in a scenario where heavy
quarks hadronize only via fragmentation in the vacuum. If coalescence is
affecting $b$-quark hadronization, enhanced production of low-$p_{\mathrm{T}}$
${{\Lambda}^{0}_{\mathrm{b}}}$ baryons would be expected in collisions with
relatively high multiplicity. In contrast, $b$ quarks produced in low
multiplicity collisions and/or at high $p_{\mathrm{T}}$ would have little
interaction with other produced particles and fragment in the vacuum, as in
$e^{+}e^{-}$ collisions.

This Letter presents new measurements of the ratio of
${{\Lambda}^{0}_{\mathrm{b}}}$ baryon to ${{\mathrm{B}}^{0}}$ meson production
cross-sections, as a function of $p_{\mathrm{T}}$ and multiplicity, using a
sample of $pp$ collisions at $\sqrt{s}=13\text{\,Te\kern-1.00006ptV}$
corresponding to an integrated luminosity of about 5.4 fb-1. Candidates for
${{\Lambda}^{0}_{\mathrm{b}}}$ baryons and ${{\mathrm{B}}^{0}}$ mesons are
reconstructed through their decays to the
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}pK^{-}$ and
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}\pi^{-}K^{+}$ final states,
respectively (charge conjugation is assumed throughout this Letter), where the
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}$ meson subsequently decays to
the ${\upmu^{+}}\mu^{-}$ final state.

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] (known as the VELO detector), a large-area silicon-strip detector
located upstream of a dipole magnet with a bending power of about
$4{\mathrm{\,Tm}}$, 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 of charged particles with a
relative uncertainty that varies from 0.5% at low momentum to 1.0% at
200$\text{\,Ge\kern-1.00006ptV\\!/}c$. Different types of charged hadrons are
distinguished using information from two ring-imaging Cherenkov detectors
[LHCb-DP-2012-003]. Muons are identified by a system composed of alternating
layers of iron and multiwire proportional chambers [LHCb-DP-2012-002].

Simulation is required to model the effects of the detector acceptance and the
imposed selection requirements. In the simulation, $pp$ collisions are
generated using Pythia [Sjostrand:2007gs]. Decays of unstable particles are
described by EvtGen [Lange:2001uf], in which final-state radiation is
generated using Photos [davidson2015photos]. The interaction of the generated
particles with the detector, and its response, are implemented using the
Geant4 toolkit [Allison:2006ve] as described in Ref. [LHCb-PROC-2011-006].
Weights are applied to the simulation to ensure the invariant mass
distributions of product pairs from the ${{\Lambda}^{0}_{\mathrm{b}}}$ and
${{\mathrm{B}}^{0}}$ decays and the parent $p_{\mathrm{T}}$ match background-
subtracted distributions that are extracted from the data using the sPlot
method [splot].

Events considered here are identified by a series of hardware and software
triggers designed to select muons from the decay
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}\rightarrow{\upmu^{+}}\mu^{-}$,
and have exactly one reconstructed primary vertex. Each individual muon
candidate is required to have
$p_{\mathrm{T}}>500\text{\,Me\kern-1.00006ptV\\!/}c$ and to penetrate hadron
absorbers in the LHCb muon system. The reconstructed ${\upmu^{+}}\mu^{-}$ pair
must have a mass within $39\text{\,Me\kern-1.00006ptV\\!/}c^{2}$ of the known
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}$ mass (which corresponds to
three times the measured mass resolution of the
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}$ peak) [PDG2020], and must form
an origin vertex that is displaced from the primary vertex. Charged pion, kaon
and proton candidates are positively identified by the response of the LHCb
ring-imaging Cherenkov detectors, and are required to have a momentum above
$3\text{\,Ge\kern-1.00006ptV}/c$ and
$p_{\mathrm{T}}>750\text{\,Me\kern-1.00006ptV}/c$. Combinations of tracks that
meet these requirements are refit with kinematic constraints that fix the
${\upmu^{+}}\mu^{-}$ invariant mass to the known
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}$ mass, and require all four
tracks to share a common vertex.

The multiplicity metrics used are either the total number of charged tracks
reconstructed in the VELO detector, $\Nvelo$, or the subset of backwards VELO
tracks that point away from the LHCb spectrometer, $\Nback$, which covers the
pseudorapidity interval of approximately $-3.5\ <\eta<-1.5$. The backwards
VELO tracks provide a multiplicity estimate that is measured in a different
rapidity region than the signal. Events containing signal candidates are
characterized in terms of their relation to events that are selected by
triggering on the LHC beam clock alone, no bias (NB) events, which provide a
selection of $pp$ collisions that do not have biases resulting from trigger
decisions based on measured particles. The results are quoted in terms of
normalized multiplicity, defined as the number of tracks at the center of a
given multiplicity bin divided by the mean number of tracks in NB events,
which are $\langle\Nvelo\rangle$NB = 37.7 and $\langle\Nback\rangle$NB = 11.1,
with negligible statistical uncertainties of less than $0.1\%$ [LHCb-
PAPER-2022-001].

Extended maximum-likelihood fits are performed on the binned
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}pK^{-}$ and
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}\pi^{-}K^{+}$ invariant mass
spectra to determine the ${{\Lambda}^{0}_{\mathrm{b}}}$ and
${{\mathrm{B}}^{0}}$ yields, respectively, in intervals of $p_{\mathrm{T}}$
and multiplicity. The ${{\Lambda}^{0}_{\mathrm{b}}}$ and ${{\mathrm{B}}^{0}}$
signals are each described by a sum of two Crystal Ball functions
[Skwarnicki:1986xj], whose tail parameters and relative contributions are
fixed to values determined by fitting simulated decays. The background
contribution is described by an exponential function. Examples of the
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}pK^{-}$ and
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}\pi^{-}K^{+}$ invariant mass
distributions and fits are shown in Fig. 1. Variations of the fit functions
that converge change the extracted ${{\Lambda}^{0}_{\mathrm{b}}}$ and
${{\mathrm{B}}^{0}}$ yields by about $1\%$, which is taken as a systematic
uncertainty.

Figure 1: Invariant mass spectra in the transverse momentum interval
$10<p_{\mathrm{T}}<12\text{\,Ge\kern-1.00006ptV\\!/}c$ for the (a)
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}pK^{-}$ and (b)
${{\mathrm{J}\mskip-3.0mu/\mskip-2.0mu\uppsi}}\pi^{-}K^{+}$ final states,
integrated over multiplicity. Fit projections including signal and background
components are shown.

The ratio of production cross-sections
$\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$ is found
by calculating

$\frac{\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}}{\sigma_{{{\mathrm{B}}^{0}}}}=\frac{N_{{{\Lambda}^{0}_{\mathrm{b}}}}}{N_{{{\mathrm{B}}^{0}}}}\times\frac{{\mathcal{B}}_{{{\mathrm{B}}^{0}}}}{{\mathcal{B}}_{{{\Lambda}^{0}_{\mathrm{b}}}}}\times\frac{\epsilon^{\rm
acc}_{{{\mathrm{B}}^{0}}}}{\epsilon^{\rm
acc}_{{{\Lambda}^{0}_{\mathrm{b}}}}}\times\frac{\epsilon^{\rm
trig}_{{{\mathrm{B}}^{0}}}}{\epsilon^{\rm
trig}_{{{\Lambda}^{0}_{\mathrm{b}}}}}\times\frac{\epsilon^{\rm
rec}_{{{\mathrm{B}}^{0}}}}{\epsilon^{\rm
rec}_{{{\Lambda}^{0}_{\mathrm{b}}}}}\times\frac{\epsilon^{\rm
PID}_{{{\mathrm{B}}^{0}}}}{\epsilon^{\rm
PID}_{{{\Lambda}^{0}_{\mathrm{b}}}}},$ (1)

where $N_{{{\Lambda}^{0}_{\mathrm{b}}}}$ and $N_{{{\mathrm{B}}^{0}}}$ are the
${{\Lambda}^{0}_{\mathrm{b}}}$ and ${{\mathrm{B}}^{0}}$ yields extracted by
fitting the peaks in the invariant mass spectra,
${\mathcal{B}}_{{{\Lambda}^{0}_{\mathrm{b}}}}$ and
${\mathcal{B}}_{{{\mathrm{B}}^{0}}}$ are the branching fractions of
${{\Lambda}^{0}_{\mathrm{b}}}$ and ${{\mathrm{B}}^{0}}$ to the relevant final
states [PDG2020], $\epsilon^{\rm acc}$ is the acceptance of the LHCb
spectrometer for the given decay, $\epsilon^{\rm trig}$ is the efficiency for
triggering on the given decay, $\epsilon^{\rm rec}$ is the efficiency for
selecting and reconstructing the parent particle, and $\epsilon^{\rm PID}$ is
the total particle identification efficiency for the final-state charged
tracks from the decays.

The ratio leads to the partial cancellation of many of the correction factors
and their systematic uncertainties due to the similarities of the decays. The
ratio of acceptance corrections $\epsilon^{\rm
acc}_{{{\mathrm{B}}^{0}}}/\epsilon^{\rm acc}_{{{\Lambda}^{0}_{\mathrm{b}}}}$
is estimated via simulation to be $\sim 0.95$ at low $p_{\mathrm{T}}$ and
tends to unity with increasing $p_{\mathrm{T}}$. A systematic uncertainty of
$1\%$ is evaluated by varying the weights applied to the simulated events
within their uncertainties. The ratio of trigger efficiencies $\epsilon^{\rm
trig}_{{{\mathrm{B}}^{0}}}/\epsilon^{\rm trig}_{{{\Lambda}^{0}_{\mathrm{b}}}}$
is measured as described in Ref. [LHCb-PUB-2014-039], and found to be
consistent with unity. Uncertainties on this factor vary from 1$\%$ at low
$p_{\mathrm{T}}$ to $3\%$ at high $p_{\mathrm{T}}$, due to the finite size of
the data samples used to measure the trigger efficiencies. The ratio of
reconstruction efficiencies $\epsilon^{\rm
rec}_{{{\mathrm{B}}^{0}}}/\epsilon^{\rm rec}_{{{\Lambda}^{0}_{\mathrm{b}}}}$
varies from $\sim 0.8$ at the lowest $p_{\mathrm{T}}$ values and increases to
be consistent with unity where $p_{\mathrm{T}}$ is much greater than the
${{\Lambda}^{0}_{\mathrm{b}}}$ and ${{\mathrm{B}}^{0}}$ masses. The deviation
from unity is due to the differences in the reconstruction efficiencies of the
intermediate states in the products of the ${{\Lambda}^{0}_{\mathrm{b}}}$ and
${{\mathrm{B}}^{0}}$ decays [LHCb-PAPER-2015-029, LHCb-PAPER-2018-043, LHCb-
PAPER-2019-014]. A systematic uncertainty that varies with $p_{\mathrm{T}}$
from $2\%$ to $4\%$ is assigned to account for uncertainties on the weights
applied to the simulation, and an additional uncertainty that is negligible at
low $p_{\mathrm{T}}$ and increases to a maximum of $\sim 2\%$ at high
$p_{\mathrm{T}}$ is assigned to account for the finite size of the simulation
samples used to calculate this correction. The ratio of particle
identification efficiencies $\epsilon^{\rm
PID}_{{{\mathrm{B}}^{0}}}/\epsilon^{\rm PID}_{{{\Lambda}^{0}_{\mathrm{b}}}}$
is found using calibrated samples of identified particles taken from data.
This term deviates from unity by a maximum of 7$\%$ at low $p_{\mathrm{T}}$,
due to the difference in identification efficiencies for pions from
${{\mathrm{B}}^{0}}$ decays and protons from ${{\Lambda}^{0}_{\mathrm{b}}}$
decays. A systematic uncertainty of $2\%$ is assigned due to the finite size
of the calibration samples [LHCb-PUB-2016-021]. The total systematic
uncertainty is calculated by adding all contributions in quadrature.
Systematic uncertainties dominate for
$p_{\mathrm{T}}<18\text{\,Ge\kern-1.00006ptV\\!/}c$, with statistical
uncertainties becoming dominant at higher $p_{\mathrm{T}}$.

The resulting
$\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$ ratio is
shown in Fig. 2 as a function of $p_{\mathrm{T}}$. Numerical values are given
in the supplemental material [ref:SuppMat]. The blue points show the data
analyzed in this Letter, where the error bars are the quadrature sum of the
statistical and systematic uncertainties, and the error boxes indicate the
point-to-point fully correlated (global) uncertainty due to uncertainties on
the ${{\Lambda}^{0}_{\mathrm{b}}}$ and ${{\mathrm{B}}^{0}}$ branching
fractions. The gray points show a previous measurement of the ratio of the
${{\Lambda}^{0}_{\mathrm{b}}}$ cross-section to the sum of the
${{\mathrm{B}}^{0}}$ and ${{\mathrm{B}}^{+}}$ cross-sections measured using
semileptonic decays over the pseudorapidity interval $2<\eta<5$ [LHCb-
PAPER-2018-050]. For direct comparison here, that ratio is multiplied by a
factor of two under the assumption of equal production of ${{\mathrm{B}}^{0}}$
and ${{\mathrm{B}}^{+}}$ mesons, which is supported by data [LHCb-
PAPER-2013-004]. In the $p_{\mathrm{T}}$ range where the measurements overlap,
there is good agreement within uncertainties. Data from $p$Pb collisions
[LHCb-PAPER-2018-048] covering two different rapidity intervals are also shown
for comparison (purple points), and generally agree with the $pp$ data within
uncertainties.

The curves in Fig. 2 are from a recent model of statistical hadronization of
$b$ quarks [He:2022tod] that assumes relative chemical equilibrium between
different $b$-hadron yields, and considers two sets of $b$ hadrons as input.
The green solid curve uses the measured spectrum of baryons collected by the
Particle Data Group (PDG) in Ref. [PDG2020], while the black dashed curve uses
an expanded set of $b$ baryons that are expected by the Relativistic Quark
Model (RQM) [Ebert:2011kk]. The data generally favor the RQM calculation,
which may be interpreted as evidence that $b$-quark hadronization is
statistical in nature at the LHC, and that higher mass $b$-baryon states await
discovery. Feeddown contributions from these baryons would contribute to the
${{\Lambda}^{0}_{\mathrm{b}}}$ yields.

Figure 2: Ratio of ${{\Lambda}^{0}_{\mathrm{b}}}$ to ${{\mathrm{B}}^{0}}$
production cross-sections as a function of $p_{\mathrm{T}}$ (blue circles).
The error bars represent the quadrature sum of the statistical and systematic
uncertainties and the boxes depict the global uncertainties due to branching
fractions. The data are compared to previous $pp$ measurements using
semileptonic decays (gray circles) [LHCb-PAPER-2018-050], data from $p$Pb
collisions (squares) [LHCb-PAPER-2018-048], and a statistical hadronization
model (SHM, solid and dashed curves) [He:2022tod].

The $p_{\mathrm{T}}$-integrated
$\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$ ratio is
shown as a function of multiplicity in Fig. 3. Numerical values are given in
the supplemental material [ref:SuppMat]. The error bars represent the
quadrature sum of the statistical and systematic uncertainties, while the
global uncertainty of $\ {}^{+19\%}_{-16\%}$ due to the branching fractions is
indicated in text. In the lowest multiplicity bins, this $pp$ data approaches
the baryon fraction measured in $e^{+}e^{-}$ collisions at the Large Electron-
Position collider (LEP) [HFLAV18]. This is expected since $b$ quarks in low-
multiplicity events do not overlap with other particles and fragment in the
vacuum, as in $e^{+}e^{-}$ collisions. There is a distinct rise of the baryon
fraction with multiplicity, with a plateau at $\sim 0.5$ for collisions that
produce more than twice the average number of VELO tracks. This could indicate
that coalescence emerges as an additional production mechanism for baryons at
high multiplicity, where multiple quark wavefunctions overlap.

Figure 3: Ratio of ${{\Lambda}^{0}_{\mathrm{b}}}$ to ${{\mathrm{B}}^{0}}$
cross-sections as a function of the total track multiplicity measured in the
VELO detector (blue). The purple point indicates the value measured in
$e^{+}e^{-}$ collisions at LEP [HFLAV18].

The $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$ ratio
is shown in Fig. 4 as a function of $p_{\mathrm{T}}$ in different multiplicity
bins. Numerical values are given in the supplemental material [ref:SuppMat].
The left panel shows the data in the different bins of total track
multiplicity, where the multiplicity intervals correspond to less than
$\langle\Nvelo\rangle$NB, between one and two times $\langle\Nvelo\rangle$NB,
and greater than twice $\langle\Nvelo\rangle$NB. The right panel shows similar
data, but uses $\langle\Nback\rangle$NB to define multiplicity. The error bars
represent the quadrature sum of the statistical and systematic uncertainties,
while the global uncertainty on all data points due to the uncertainties on
the branching fractions is indicated in text. The purple point represents the
LEP measurement of the ratio of the $b$-baryon fraction to $b$-meson fraction
[HFLAV18].

A significant multiplicity dependence can be observed using both multiplicity
metrics, with higher multiplicity collisions displaying a larger
${{\Lambda}^{0}_{\mathrm{b}}}$ fraction. The dependence is more pronounced
when using the total number of VELO tracks (dominated by forward tracks),
where there is clear ordering at intermediate $p_{\mathrm{T}}$, however the
backwards VELO tracks metric also shows a clear difference between the lowest
and higher multiplicity bins. At low $p_{\mathrm{T}}$, the ratio
$\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$ is
significantly higher than the value measured in $e^{+}e^{-}$ collisions, but
as $p_{\mathrm{T}}$ increases the multiplicity dependence weakens and all data
converges to the value from LEP. This is expected in quark coalescence
scenarios, where low-$p_{\mathrm{T}}$ ${{\Lambda}^{0}_{\mathrm{b}}}$ baryons
can be produced when $b$ quarks combine with two light quarks. However, at
high-$p_{\mathrm{T}}$ ${{\Lambda}^{0}_{\mathrm{b}}}$ baryons have limited
overlap with the underlying event and are therefore produced by $b$-quark
fragmentation in the vacuum.

Figure 4: Ratio of ${{\Lambda}^{0}_{\mathrm{b}}}$ to ${{\mathrm{B}}^{0}}$
cross-sections as a function of $p_{\mathrm{T}}$, in bins of a) the total
multiplicity measured in the VELO detector and b) the backwards track
multiplicity. The purple point shows the value measured in
$e^{+}e^{-}\rightarrow{\mathrm{Z}}^{0}\rightarrow b\bar{b}$ reactions at LEP
[HFLAV18].

In summary, these new measurements from LHCb show clear variations of the
$\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$ ratio with
multiplicity and $p_{\mathrm{T}}$ in $pp$ collisions at
$\sqrt{s}=13\text{\,Te\kern-1.00006ptV}$. Production of the
${{\Lambda}^{0}_{\mathrm{b}}}$ baryon is enhanced relative to the
${{\mathrm{B}}^{0}}$ meson at high charged-particle multiplicity and
relatively low $p_{\mathrm{T}}$. The baryon fraction measured at LEP can be
reached in $pp$ collisions with very low multiplicity, and with $b$ hadrons at
high $p_{\mathrm{T}}$, regardless of multiplicity. These observations show
that $b$-quark hadronization is not universal between $e^{+}e^{-}$ and $pp$
collisions, and may indicate that quark coalescence plays an important role in
forming hadrons at the LHC. These results are qualitatively consistent with
the emergence of coalescence as an additional baryon production mechanism in
high-density hadronic environments.

## Appendix: Supplemental material

The ratio of ${{\Lambda}^{0}_{\mathrm{b}}}$ to ${{\mathrm{B}}^{0}}$ cross-
sections $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
as a function of $p_{\mathrm{T}}$ and normalized multiplicity
$\Nvelo/\langle\Nvelo\rangle$NB are given in Tables 1 and 2, respectively.
Tables 3, 4, and 5 give the ratio versus the total VELO multiplicity for low-,
intermediate-, and high-multiplicity ranges, respectively. Tables 6, 7, and 8
provide the ratio versus the backward multiplicity metric for low-,
intermediate-, and high-multiplicity ranges, respectively.

$p_{\mathrm{T}}$ range [GeV/$c$] | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0 – 2 | $0.45\pm 0.03$
2 – 4 | $0.44\pm 0.02$
4 – 6 | $0.46\pm 0.02$
6 – 8 | $0.41\pm 0.02$
8 – 10 | $0.39\pm 0.02$
10 – 12 | $0.33\pm 0.01$
12 – 14 | $0.29\pm 0.01$
14 – 16 | $0.27\pm 0.01$
16 – 18 | $0.23\pm 0.01$
18 – 20 | $0.21\pm 0.01$
20 – 22 | $0.21\pm 0.02$
22 – 24 | $0.23\pm 0.02$
24 – 26 | $0.19\pm 0.02$
26 – 28 | $0.18\pm 0.03$
28 – 30 | $0.16\pm 0.03$
Table 1: Ratio of cross-sections as a function of $p_{\mathrm{T}}$, as shown in Fig. 1. The additional ${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the branching fractions is not included. /$\langle\Nvelo\rangle$NB | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0.13 – 0.40 | $0.25\pm 0.05$
0.40 – 0.53 | $0.35\pm 0.03$
0.53 – 0.66 | $0.36\pm 0.03$
0.66 – 0.79 | $0.38\pm 0.02$
0.79 – 1.06 | $0.42\pm 0.02$
1.06 – 1.32 | $0.43\pm 0.02$
1.32 – 1.59 | $0.46\pm 0.03$
1.59 – 1.85 | $0.47\pm 0.03$
1.85 – 2.12 | $0.48\pm 0.03$
2.12 – 2.65 | $0.49\pm 0.03$
2.65 – 3.31 | $0.49\pm 0.03$
3.31 – 3.97 | $0.48\pm 0.03$
3.97 – 5.29 | $0.44\pm 0.03$
5.29 – 6.61 | $0.60\pm 0.08$
Table 2: Ratio of cross-sections as a function of multiplicity, as shown in Fig. 3. The additional ${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the branching fractions is not included. $p_{\mathrm{T}}$ range [GeV/$c$] | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0 – 2 | $0.35\pm 0.05$
2 – 4 | $0.41\pm 0.03$
4 – 6 | $0.38\pm 0.02$
6 – 8 | $0.35\pm 0.02$
8 – 10 | $0.29\pm 0.02$
10 – 12 | $0.23\pm 0.02$
12 – 14 | $0.21\pm 0.02$
14 – 16 | $0.18\pm 0.02$
16 – 18 | $0.12\pm 0.02$
18 – 20 | $0.18\pm 0.05$
Table 3: Ratio of cross-sections for low multiplicity data, as measured using VELO tracks, shown in blue in the left panel of Fig. 4. The additional ${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the branching fractions is not included. $p_{\mathrm{T}}$ range [GeV/$c$] | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0 – 2 | $0.51\pm 0.04$
2 – 4 | $0.45\pm 0.02$
4 – 6 | $0.46\pm 0.02$
6 – 8 | $0.42\pm 0.02$
8 – 10 | $0.38\pm 0.02$
10 – 12 | $0.33\pm 0.02$
12 – 14 | $0.28\pm 0.02$
14 – 16 | $0.25\pm 0.02$
16 – 18 | $0.23\pm 0.02$
18 – 20 | $0.17\pm 0.02$
20 – 22 | $0.20\pm 0.02$
22 – 24 | $0.19\pm 0.02$
Table 4: Ratio of cross-sections for intermediate multiplicity data, as measured using VELO tracks, shown in black in the left panel of Fig. 4. The additional ${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the branching fractions is not included. $p_{\mathrm{T}}$ range [GeV/$c$] | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0 – 2 | $0.49\pm 0.05$
2 – 4 | $0.45\pm 0.02$
4 – 6 | $0.51\pm 0.02$
6 – 8 | $0.45\pm 0.02$
8 – 10 | $0.44\pm 0.02$
10 – 12 | $0.35\pm 0.02$
12 – 14 | $0.32\pm 0.02$
14 – 16 | $0.30\pm 0.02$
16 – 18 | $0.25\pm 0.02$
18 – 20 | $0.25\pm 0.02$
20 – 22 | $0.24\pm 0.02$
22 – 24 | $0.22\pm 0.02$
Table 5: Ratio of cross-sections for high multiplicity data, as measured using VELO tracks, shown in red in the left panel of Fig. 4. The additional ${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the branching fractions is not included. $p_{\mathrm{T}}$ range [GeV/$c$] | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0 – 2 | $0.39\pm 0.04$
2 – 4 | $0.42\pm 0.02$
4 – 6 | $0.42\pm 0.02$
6 – 8 | $0.39\pm 0.02$
8 – 10 | $0.37\pm 0.01$
10 – 12 | $0.29\pm 0.02$
12 – 14 | $0.31\pm 0.02$
14 – 16 | $0.23\pm 0.02$
16 – 18 | $0.19\pm 0.02$
18 – 20 | $0.19\pm 0.02$
20 – 22 | $0.21\pm 0.03$
22 – 24 | $0.24\pm 0.03$
Table 6: Ratio of cross-sections for low multiplicity data, as measured using backward tracks, shown in blue in the right panel of Fig. 4. The additional ${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the branching fractions is not included. $p_{\mathrm{T}}$ range [GeV/$c$] | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0 – 2 | $0.41\pm 0.05$
2 – 4 | $0.49\pm 0.03$
4 – 6 | $0.50\pm 0.02$
6 – 8 | $0.44\pm 0.02$
8 – 10 | $0.43\pm 0.02$
10 – 12 | $0.33\pm 0.02$
12 – 14 | $0.29\pm 0.02$
14 – 16 | $0.27\pm 0.02$
16 – 18 | $0.26\pm 0.02$
18 – 20 | $0.23\pm 0.02$
20 – 22 | $0.21\pm 0.02$
22 – 24 | $0.18\pm 0.02$
Table 7: Ratio of cross-sections for intermediate multiplicity data, as measured using backward tracks, shown in black in the right panel of Fig. 4. The additional ${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the branching fractions is not included. $p_{\mathrm{T}}$ range [GeV/$c$] | $\sigma_{{{\Lambda}^{0}_{\mathrm{b}}}}/\sigma_{{{\mathrm{B}}^{0}}}$
---|---
0 – 2 | $0.55\pm 0.07$
2 – 4 | $0.45\pm 0.03$
4 – 6 | $0.51\pm 0.02$
6 – 8 | $0.45\pm 0.02$
8 – 10 | $0.43\pm 0.02$
10 – 12 | $0.38\pm 0.02$
12 – 14 | $0.32\pm 0.02$
14 – 16 | $0.31\pm 0.02$
16 – 18 | $0.24\pm 0.02$
18 – 20 | $0.22\pm 0.02$
20 – 22 | $0.22\pm 0.02$
22 – 24 | $0.22\pm 0.02$
Table 8: Ratio of cross-sections for high multiplicity data, as measured using
back tracks, shown in red in the right panel of Fig. 4. The additional
${}^{+19\%}_{-16\%}$ global uncertainty due to the uncertainty in the
branching fractions is not included.

## 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 9: 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 Plot111Dalitz 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 |  [davidson2015photos] davidson2015photos
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
TMVA222Do 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
GammaCombo333Always 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 function444A 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 10: LHCb detector performance papers. LHCb-DP number | Title
---|---
LHCb-DP-2020-003 [LHCb-DP-2020-003] | TBD
LHCb-DP-2020-002 [LHCb-DP-2020-002] | TBD
LHCb-DP-2020-001 [LHCb-DP-2020-001] | TBD
LHCb-DP-2019-006 [LHCb-DP-2019-006] | TBD
LHCb-DP-2019-005 [LHCb-DP-2019-005] | TBD
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 11: 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 12: LHCb-PAPERs (which have their identifier as their cite code). DNE: Does not exist.  LHCb-PAPER-2021-020 [LHCb-PAPER-2021-020] |  LHCb-PAPER-2021-019 [LHCb-PAPER-2021-019] |  LHCb-PAPER-2021-018 [LHCb-PAPER-2021-018] |  LHCb-PAPER-2021-017 [LHCb-PAPER-2021-017] |  LHCb-PAPER-2021-016 [LHCb-PAPER-2021-016]
---|---|---|---|---
LHCb-PAPER-2021-015 [LHCb-PAPER-2021-015] |  LHCb-PAPER-2021-014 [LHCb-PAPER-2021-014] |  LHCb-PAPER-2021-013 [LHCb-PAPER-2021-013] |  LHCb-PAPER-2021-012 [LHCb-PAPER-2021-012] |  LHCb-PAPER-2021-011 [LHCb-PAPER-2021-011]
LHCb-PAPER-2021-010 [LHCb-PAPER-2021-010] |  LHCb-PAPER-2021-009 [LHCb-PAPER-2021-009] |  LHCb-PAPER-2021-008 [LHCb-PAPER-2021-008] |  LHCb-PAPER-2021-007 [LHCb-PAPER-2021-007] |  LHCb-PAPER-2021-006 [LHCb-PAPER-2021-006]
LHCb-PAPER-2021-005 [LHCb-PAPER-2021-005] |  LHCb-PAPER-2021-004 [LHCb-PAPER-2021-004] |  LHCb-PAPER-2021-003 [LHCb-PAPER-2021-003] |  LHCb-PAPER-2021-002 [LHCb-PAPER-2021-002] |  LHCb-PAPER-2021-001 [LHCb-PAPER-2021-001]
LHCb-PAPER-2020-048 [LHCb-PAPER-2020-048] |  LHCb-PAPER-2020-047 [LHCb-PAPER-2020-047] |  LHCb-PAPER-2020-046 [LHCb-PAPER-2020-046] |  |
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-2011-039555LHCb-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 13: 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]666If 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 $\,\upmu\text{m}$ 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 | ${\mathrm{D}}^{*\mp}_{\mathrm{s}}$ | \DporDsp | ${\mathrm{D}}_{({\mathrm{s}})}^{+}$
\DmorDsm | ${\mathrm{D}}{}_{({\mathrm{s}})}^{-}$ | \DpmorDspm | ${\mathrm{D}}{}_{({\mathrm{s}})}^{\pm}$ |  |

####  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 | $\,\upmu\text{m}$ | \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 |
---|---

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.