* Barreiro et al. (2000) T. Barreiro, E.J. Copeland, and N.J. Nunes.  Quintessence arising from exponential potentials.  _Phys. Rev. D_ , 61:127301, 2000.
  * Billyard et al. (1999) A.P. Billyard, A.A. Coley, R.J. van den Hoogen, J. Ibanez, and I. Olasagasti.  Scalar field cosmologies with barotropic matter: Models of Bianchi class B.  _Class. Quant. Grav._ , 16:4035–4056, 1999.
  * Macorra and Piccinelli (2000) A.d.l. Macorra and G. Piccinelli.  Cosmological evolution of general scalar fields and quintessence.  _Phys. Rev. D_ , 61:123503, May 2000.
  * Nunes and Mimoso (2000) A. Nunes and J.P. Mimoso.  On the potentials yielding cosmological scaling solutions.  _Phys. Lett. B_ , 488:423–427, 2000.
  * Ng et al. (2001) S.C.C. Ng, N.J. Nunes, and F. Rosati.  Applications of scalar attractor solutions to cosmology.  _Phys. Rev._ , D64:083510, 2001.
  * Rubano and Barrow (2001) C. Rubano and J.D. Barrow.  Scaling solutions and reconstruction of scalar field potentials.  _Phys. Rev. D_ , 64:127301, Nov 2001.
  * Uzan (1999) J.P. Uzan.  Cosmological scaling solutions of nonminimally coupled scalar fields.  _Phys. Rev. D_ , 59:123510, 1999.
  * Jarv et al. (2004) L. Jarv, T. Mohaupt, and F. Saueressig.  Quintessence cosmologies with a double exponential potential.  _JCAP_ , 0408:016, 2004.
  * Li et al. (2005) X.Z. Li, Y.B. Zhao, and C.B. Sun.  Heteroclinic orbit and tracking attractor in cosmological model with a double exponential potential.  _Class. Quant. Grav._ , 22:3759–3766, 2005.
  * Ng and Wiltshire (2001) S.C.C. Ng and D.L. Wiltshire.  Properties of cosmologies with dynamical pseudo Nambu-Goldstone bosons.  _Phys. Rev._ , D63:023503, 2001.
  * Gong (2014) Y. Gong.  The general property of dynamical quintessence field.  _Phys. Lett._ , B731:342–349, 2014.
  * Fang et al. (2009) W. Fang, Y. Li, K. Zhang, and H.Q. Lu.  Exact Analysis of Scaling and Dominant Attractors Beyond the Exponential Potential.  _Class. Quant. Grav._ , 26:155005, 2009.
  * Roy and Banerjee (2014) N. Roy and N. Banerjee.  Tracking quintessence: a dynamical systems study.  _Gen. Rel. Grav._ , 46:1651, 2014.
  * García-Salcedo et al. (2015) R. García-Salcedo, T. Gonzalez, F.A. Horta-Rangel, I. Quiros, and D. Sanchez-Guzmán.  Introduction to the application of dynamical systems theory in the study of the dynamics of cosmological models of dark energy.  _Eur. J. Phys._ , 36(2):025008, 2015.
  * Paliathanasis et al. (2015) A. Paliathanasis, M. Tsamparlis, S. Basilakos, and J.D. Barrow.  Dynamical analysis in scalar field cosmology.  _Phys. Rev._ , D91(12):123535, 2015.
  * Zhou (2008) S.Y. Zhou.  A New Approach to Quintessence and Solution of Multiple Attractors.  _Phys. Lett._ , B660:7–12, 2008.
  * Matos et al. (2009) T. Matos, J.R. Luevano, I. Quiros, L.A. Urena-Lopez, and J.A. Vazquez.  Dynamics of Scalar Field Dark Matter With a Cosh-like Potential.  _Phys. Rev._ , D80:123521, 2009.
  * Clemson and Liddle (2009) T.G. Clemson and A.R. Liddle.  Observational constraints on thawing quintessence models.  _Mon. Not. Roy. Astron. Soc._ , 395:1585–1590, 2009.
  * Faraoni et al. (1999) V. Faraoni, E. Gunzig, and P. Nardone.  Conformal transformations in classical gravitational theories and in cosmology.  _Fund. Cosmic Phys._ , 20:121, 1999.
  * Chiba et al. (2000) T. Chiba, T. Okabe, and M. Yamaguchi.  Kinetically driven quintessence.  _Phys. Rev. D_ , 62:023511, Jun 2000.
  * Armendariz-Picon et al. (2000) C. Armendariz-Picon, V.F. Mukhanov, and P.J. Steinhardt.  A Dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration.  _Phys. Rev. Lett._ , 85:4438–4441, Nov 2000.
  * Armendariz-Picon et al. (2001) C. Armendariz-Picon, V.F. Mukhanov, and P.J. Steinhardt.  Essentials of k-essence.  _Phys. Rev. D_ , 63:103510, Apr 2001.
  * Sbisà (2015) F. Sbisà.  Classical and quantum ghosts.  _Eur. J. Phys._ , 36:015009, 2015.
  * Armendariz-Picon et al. (1999) C. Armendariz-Picon, T. Damour, and V.F. Mukhanov.  k - inflation.  _Phys. Lett. B_ , 458:209–218, 1999.
  * Barros (2019) B.J. Barros.  Kinetically coupled dark energy.  _Phys. Rev. D_ , 99(6):064051, 2019.
  * Mach (2013) E. Mach.  _The Science of Mechanics: A Critical and Historical Exposition of its Principles_.  Cambridge Library Collection - Physical Sciences. Cambridge University Press, 2013.
  * Einstein and Greene (2014) A. Einstein and B. Greene.  _The Meaning of Relativity: Including the Relativistic Theory of the Non-Symmetric Field - Fifth Edition_.  Princeton University Press, 2014.
  * Faraoni and Capozziello (2011) V. Faraoni and S. Capozziello.  _Beyond Einstein Gravity_ , volume 170.  Springer, 2011.
  * Faraoni and Nadeau (2007) V. Faraoni and S. Nadeau.  The (pseudo)issue of the conformal frame revisited.  _Phys. Rev. D_ , 75:023501, 2007.
  * Bekenstein (1993) J.D. Bekenstein.  The Relation between physical and gravitational geometry.  _Phys. Rev. D_ , 48:3641–3647, 1993.
  * Asanov (1985) G.S. Asanov.  _Finsler geometry, relativity and gauge theories_.  D. Reidel Publishing, 1985.
  * Horndeski (1974) G.W. Horndeski.  Second-order scalar-tensor field equations in a four-dimensional space.  _Int. J. Theor. Phys._ , 10:363–384, 1974.
  * Deffayet and Steer (2013) C. Deffayet and D.A. Steer.  A formal introduction to Horndeski and Galileon theories and their generalizations.  _Class. Quant. Grav._ , 30:214006, 2013.
  * Bettoni and Liberati (2013) D. Bettoni and S. Liberati.  Disformal invariance of second order scalar-tensor theories: Framing the Horndeski action.  _Phys. Rev. D_ , 88:084020, 2013.
  * Lin et al. (2014) C. Lin, S. Mukohyama, R. Namba, and R. Saitou.  Hamiltonian structure of scalar-tensor theories beyond Horndeski.  _JCAP_ , 1410(10):071, 2014.
  * Gleyzes et al. (2015) J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi.  New class of consistent scalar-tensor theories.  _Phys. Rev. Lett._ , 114(21):211101, 2015.
  * Zumalacárregui and García-Bellido (2014) M. Zumalacárregui and J. García-Bellido.  Transforming gravity: from derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian.  _Phys. Rev. D_ , 89:064046, 2014.
  * Woodard (2015) R.P. Woodard.  Ostrogradsky’s theorem on Hamiltonian instability.  _Scholarpedia_ , 10(8):32243, 2015.
  * Ostrogradsky (1850) M. Ostrogradsky.  Mémoires sur les équations différentielles, relatives au problème des isopérimètres.  _Mem. Acad. St. Petersbourg_ , 6(4):385–517, 1850\.
  * De Felice and Tsujikawa (2012) A. De Felice and S. Tsujikawa.  Conditions for the cosmological viability of the most general scalar-tensor theories and their applications to extended Galileon dark energy models.  _JCAP_ , 1202:007, 2012.
  * Ellis et al. (1989) J. Ellis, S. Kalara, K. Olive, and C. Wetterich.  Density-dependent couplings and astrophysical bounds on light scalar particles.  _Physics Letters B_ , 228(2):264 – 272, 1989\.
  * Wetterich (1995) C. Wetterich.  The Cosmon model for an asymptotically vanishing time dependent cosmological ’constant’.  _Astron. Astrophys._ , 301:321–328, 1995.
  * Damour and Nordtvedt (1993) T. Damour and K. Nordtvedt.  Tensor-scalar cosmological models and their relaxation toward general relativity.  _Phys. Rev. D_ , 48:3436–3450, 1993.
  * Damour and Polyakov (1994) T. Damour and A. Polyakov.  The string dilation and a least coupling principle.  _Nuclear Physics B_ , 423(2):532 – 558, 1994\.
  * Szydlowski (2006) M. Szydlowski.  Cosmological model with energy transfer.  _Physics Letters B_ , 632(1):1 – 5, 2006.
  * Szydłowski et al. (2006) M. Szydłowski, T. Stachowiak, and R. Wojtak.  Towards testing interacting cosmology by distant supernovae.  _Phys. Rev. D_ , 73:063516, 2006.
  * Nunes et al. (2001) A. Nunes, J.P. Mimoso, and T.C. Charters.  Scaling solutions from interacting fluids.  _Phys. Rev._ , D63:083506, 2001.
  * Chimento et al. (2003) L.P. Chimento, A.S. Jakubi, D. Pavon, and W. Zimdahl.  Interacting quintessence solution to the coincidence problem.  _Phys. Rev. D_ , 67:083513, 2003.
  * Olivares et al. (2008) G. Olivares, F. Atrio-Barandela, and D. Pavon.  Dynamics of Interacting Quintessence Models: Observational Constraints.  _Phys. Rev._ , D77:063513, 2008.
  * Quartin et al. (2008) M. Quartin, M.O. Calvao, S.E. Joras, R.R.R. Reis, and I. Waga.  Dark Interactions and Cosmological Fine-Tuning.  _JCAP_ , 0805:007, 2008.
  * Chen et al. (2008) S. Chen, B. Wang, and J. Jing.  Dynamics of interacting dark energy model in Einstein and Loop Quantum Cosmology.  _Phys. Rev._ , D78:123503, 2008.
  * Quercellini et al. (2008) C. Quercellini, M. Bruni, A. Balbi, and D. Pietrobon.  Late universe dynamics with scale-independent linear couplings in the dark sector.  _Phys. Rev._ , D78:063527, 2008.
  * Caldera-Cabral et al. (2009) G. Caldera-Cabral, R. Maartens, and L.A. Urena-Lopez.  Dynamics of interacting dark energy.  _Phys. Rev._ , D79:063518, 2009.
  * Li and Ma (2010) S. Li and Y. Ma.  Dark Energy Interacting with Dark Matter in Classical Einstein and Loop Quantum Cosmology.  _Eur. Phys. J._ , C68:227–239, 2010.
  * Arevalo et al. (2012) F. Arevalo, A.P.R. Bacalhau, and W. Zimdahl.  Cosmological dynamics with non-linear interactions.  _Class. Quant. Grav._ , 29:235001, 2012.
  * Perez et al. (2014) J. Perez, A. Füzfa, T. Carletti, L. Mélot, and L. Guedezounme.  The Jungle Universe: coupled cosmological models in a Lotka-Volterra framework.  _Gen. Rel. Grav._ , 46:1753, 2014.
  * Szydłowski and Stachowski (2016) M. Szydłowski and A. Stachowski.  Does the diffusion dark matter-dark energy interaction model solve cosmological puzzles?  _Phys. Rev._ , D94(4):043521, 2016.
  * Haba et al. (2016) Z. Haba, A. Stachowski, and M. Szydłowski.  Dynamics of the diffusive DM-DE interaction – Dynamical system approach.  _JCAP_ , 1607(07):024, 2016.
  * Amendola (2000) L. Amendola.  Coupled quintessence.  _Phys. Rev. D_ , 62:043511, 2000.
  * Zimdahl and Pavon (2001) W. Zimdahl and D. Pavon.  Interacting quintessence.  _Phys. Lett._ , B521:133–138, 2001.
  * Amendola (1999) L. Amendola.  Scaling solutions in general nonminimal coupling theories.  _Phys. Rev. D_ , 60:043501, 1999.
  * Billyard and Coley (2000) A.P. Billyard and A.A. Coley.  Interactions in scalar field cosmology.  _Phys. Rev._ , D61:083503, 2000.
  * Holden and Wands (2000) D.J. Holden and D. Wands.  Selfsimilar cosmological solutions with a nonminimally coupled scalar field.  _Phys. Rev. D_ , 61:043506, 2000.
  * Amendola and Tocchini-Valentini (2001) L. Amendola and D. Tocchini-Valentini.  Stationary dark energy: The Present universe as a global attractor.  _Phys. Rev._ , D64:043509, 2001.
  * Tocchini-Valentini and Amendola (2002) D. Tocchini-Valentini and L. Amendola.  Stationary dark energy with a baryon dominated era: Solving the coincidence problem with a linear coupling.  _Phys. Rev._ , D65:063508, 2002.
  * Gumjudpai et al. (2005) B. Gumjudpai, T. Naskar, M. Sami, and S. Tsujikawa.  Coupled dark energy: Towards a general description of the dynamics.  _JCAP_ , 06:007, 2005.
  * Liu and Li (2005) D.J. Liu and X.Z. Li.  Dynamics of quintessence with thermal interactions.  _Phys. Lett._ , B611:8–14, 2005.
  * Gonzalez et al. (2006) T. Gonzalez, G. Leon, and I. Quiros.  Dynamics of quintessence models of dark energy with exponential coupling to dark matter.  _Class. Quant. Grav._ , 23:3165–3179, 2006.
  * Mimoso et al. (2006) J.P. Mimoso, A. Nunes, and D. Pavón.  Asymptotic behavior of the warm inflation scenario with viscous pressure.  _Phys. Rev. D_ , 73:023502, 2006.
  * Chen and Gong (2009) X.m. Chen and Y. Gong.  Fixed points in interacting dark energy models.  _Phys. Lett._ , B675:9–13, 2009.
  * Boehmer et al. (2010) C.G. Boehmer, G. Caldera-Cabral, N. Chan, R. Lazkoz, and R. Maartens.  Quintessence with quadratic coupling to dark matter.  _Phys. Rev._ , D81:083003, 2010.
  * Lopez Honorez et al. (2010) L. Lopez Honorez, O. Mena, and G. Panotopoulos.  Higher-order coupled quintessence.  _Phys. Rev._ , D82:123525, 2010.
  * Wei (2011) H. Wei.  Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector.  _Nucl. Phys._ , B845:381–392, 2011.
  * Cicoli et al. (2012) M. Cicoli, F.G. Pedro, and G. Tasinato.  Natural Quintessence in String Theory.  _JCAP_ , 1207:044, 2012.
  * Xu et al. (2012) C. Xu, E.N. Saridakis, and G. Leon.  Phase-Space analysis of Teleparallel Dark Energy.  _JCAP_ , 1207:005, 2012.
  * Morris et al. (2013) S.C.F. Morris, A.M. Green, A. Padilla, and E.R.M. Tarrant.  Cosmological effects of coupled dark matter.  _Phys. Rev._ , D88(8):083522, 2013.
  * Tzanni and Miritzis (2014) K. Tzanni and J. Miritzis.  Coupled quintessence with double exponential potentials.  _Phys. Rev._ , D89(10):103540, 2014.  [Addendum: Phys. Rev.D89,no.12,129902(2014)].
  * Hossain et al. (2014) M.W. Hossain, R. Myrzakulov, M. Sami, and E.N. Saridakis.  Variable gravity: A suitable framework for quintessential inflation.  _Phys. Rev._ , D90(2):023512, 2014.
  * Zhang et al. (2014) M. Zhang, C. Sun, Z. Yang, and R. Yue.  Cosmological evolution of quintessence with a sign-changing interaction in dark sector.  _Sci. China Phys. Mech. Astron._ , 57:1805–1808, 2014.
  * Roy and Banerjee (2015) N. Roy and N. Banerjee.  Dynamical systems study of Chameleon scalar field.  _Annals Phys._ , 356:452–466, 2015.
  * Shahalam et al. (2015) M. Shahalam, S.D. Pathak, M.M. Verma, M.Yu. Khlopov, and R. Myrzakulov.  Dynamics of interacting quintessence.  _Eur. Phys. J._ , C75(8):395, 2015.
  * Singh and Singh (2016) S. Singh and P. Singh.  It’s a dark, dark world: Background evolution of interacting $\phi$CDM models beyond simple exponential potentials.  _JCAP_ , 1605(05):017, 2016.
  * Bernardi and Landim (2017) F.F. Bernardi and R.G. Landim.  Coupled quintessence and the impossibility of an interaction: a dynamical analysis study.  _Eur. Phys. J._ , C77(5):290, 2017.
  * Barros et al. (2019) B.J. Barros, L. Amendola, T. Barreiro, and N.J. Nunes.  Coupled quintessence with a $\Lambda$CDM background: removing the $\sigma_{8}$ tension.  _JCAP_ , 01:007, 2019.
  * ter Haar et al. (2021) L. ter Haar, M. Bezares, M. Crisostomi, E. Barausse, and C. Palenzuela.  Dynamics of screening in modified gravity.  _Phys. Rev. Lett._ , 126:091102, Mar 2021.
  * Koyama (2016) K. Koyama.  Cosmological Tests of Modified Gravity.  _Rept. Prog. Phys._ , 79(4):046902, 2016.
  * Joyce et al. (2015) A. Joyce, B. Jain, J. Khoury, and M. Trodden.  Beyond the Cosmological Standard Model.  _Phys. Rept._ , 568:1–98, 2015.
  * Khoury (2013) J. Khoury.  Chameleon Field Theories.  _Class. Quant. Grav._ , 30:214004, 2013.
  * Babichev and Deffayet (2013) E. Babichev and C. Deffayet.  An introduction to the Vainshtein mechanism.  _Class. Quant. Grav._ , 30:184001, 2013.
  * Brax et al. (2021) P. Brax, S. Casas, H. Desmond, and B. Elder.  Testing Screened Modified Gravity.  _Universe_ , 8(1):11, 2021.
  * Brax (2013) P. Brax.  Screening mechanisms in modified gravity.  _Class. Quant. Grav._ , 30:214005, 2013.
  * Brax et al. (2004) P. Brax, C. van de Bruck, A.C. Davis, J. Khoury, and A. Weltman.  Detecting dark energy in orbit: The cosmological chameleon.  _Phys. Rev. D_ , 70:123518, 2004.
  * van de Bruck et al. (2013) C. van de Bruck, J. Morrice, and S. Vu.  Constraints on Nonconformal Couplings from the Properties of the Cosmic Microwave Background Radiation.  _Phys. Rev. Lett._ , 111:161302, 2013.
  * van de Bruck et al. (2017) C. van de Bruck, J. Mifsud, and J. Morrice.  Testing coupled dark energy models with their cosmological background evolution.  _Phys. Rev. D_ , 95(4):043513, 2017.
  * van de Bruck et al. (2016a) C. van de Bruck, J. Mifsud, J.P. Mimoso, and N.J. Nunes.  Generalized dark energy interactions with multiple fluids.  _JCAP_ , 11(11):031, 2016a.
  * Van De Bruck and Mifsud (2018) C. Van De Bruck and J. Mifsud.  Searching for dark matter - dark energy interactions: going beyond the conformal case.  _Phys. Rev. D_ , 97(2):023506, 2018.
  * Mifsud and Van De Bruck (2017) J. Mifsud and C. Van De Bruck.  Probing the imprints of generalized interacting dark energy on the growth of perturbations.  _JCAP_ , 11:001, 2017.
  * Gómez-Valent et al. (2020) A. Gómez-Valent, V. Pettorino, and L. Amendola.  Update on coupled dark energy and the $H_{0}$ tension.  _Phys. Rev. D_ , 101(12):123513, 2020.
  * Pettorino et al. (2012) V. Pettorino, L. Amendola, C. Baccigalupi, and C. Quercellini.  Constraints on coupled dark energy using CMB data from WMAP and SPT.  _Phys. Rev. D_ , 86:103507, 2012.
  * Amendola et al. (2012) L. Amendola, V. Pettorino, C. Quercellini, and A. Vollmer.  Testing coupled dark energy with next-generation large-scale observations.  _Phys. Rev. D_ , 85:103008, 2012.
  * Amendola et al. (2014) L. Amendola, T. Barreiro, and N.J. Nunes.  Multifield coupled quintessence.  _Phys. Rev. D_ , 90(8):083508, 2014.
  * Pourtsidou et al. (2013) A. Pourtsidou, C. Skordis, and E.J. Copeland.  Models of dark matter coupled to dark energy.  _Phys. Rev. D_ , 88(8):083505, 2013.
  * Pace et al. (2014) F. Pace, L. Moscardini, R. Crittenden, M. Bartelmann, and V. Pettorino.  A comparison of structure formation in minimally and non-minimally coupled quintessence models.  _Mon. Not. Roy. Astron. Soc._ , 437(1):547–561, 2014.
  * Tarrant et al. (2012) E.R.M. Tarrant, C. van de Bruck, E.J. Copeland, and A.M. Green.  Coupled quintessence and the halo mass function.  _Phys. Rev. D_ , 85:023503, 2012.
  * Teixeira et al. (2020) E.M. Teixeira, A. Nunes, and N.J. Nunes.  Disformally Coupled Quintessence.  _Phys. Rev. D_ , 101(8):083506, 2020.
  * Di Valentino et al. (2020) E. Di Valentino, A. Melchiorri, and J. Silk.  Cosmological constraints in extended parameter space from the Planck 2018 Legacy release.  _JCAP_ , 01:013, 2020.
  * Efstathiou (2003) G. Efstathiou.  Is the low cosmic microwave background quadrupole a signature of spatial curvature?  _Monthly Notices of the Royal Astronomical Society_ , 343(4):L95–L98, 08 2003.
  * Riess et al. (2022b) A.G. Riess, L. Breuval, W. Yuan, S. Casertano, L.M. Macri, J.B. Bowers, D. Scolnic, T. Cantat-Gaudin, R.I. Anderson, and M.C. Reyes.  Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero-point Uncertainties, and Hubble Space Telescope Photometry.  _Astrophys. J._ , 938(1):36, 2022b.
  * Forconi et al. (2021) M. Forconi, W. Giarè, E. Di Valentino, and A. Melchiorri.  Cosmological constraints on slow roll inflation: An update.  _Phys. Rev. D_ , 104(10):103528, 2021.
  * Linde (1995) A.D. Linde.  Inflation with variable Omega.  _Phys. Lett. B_ , 351:99–104, 1995.
  * Linde (2003) A.D. Linde.  Can we have inflation with Omega $>$ 1?  _JCAP_ , 05:002, 2003.
  * Ratra (2017) B. Ratra.  Inflation in a closed universe.  _Phys. Rev. D_ , 96(10):103534, 2017.
  * Bonga et al. (2016) B. Bonga, B. Gupt, and N. Yokomizo.  Inflation in the closed FLRW model and the CMB.  _JCAP_ , 10:031, 2016.
  * Handley (2019) W. Handley.  Primordial power spectra for curved inflating universes.  _Phys. Rev. D_ , 100(12):123517, 2019.
  * Bonga et al. (2017) B. Bonga, B. Gupt, and N. Yokomizo.  Tensor perturbations during inflation in a spatially closed Universe.  _JCAP_ , 05:021, 2017.
  * Ooba et al. (2018) J. Ooba, B. Ratra, and N. Sugiyama.  Planck 2015 Constraints on the Non-flat $\Lambda$CDM Inflation Model.  _Astrophys. J._ , 864(1):80, 2018.
  * Ellis et al. (2002) G.F.R. Ellis, W.R. Stoeger, S. J., P. McEwan, and P. Dunsby.  Dynamics of inflationary universes with positive spatial curvature.  _Gen. Rel. Grav._ , 34:1445–1459, 2002.
  * Uzan et al. (2003) J.P. Uzan, U. Kirchner, and G.F.R. Ellis.  WMAP data and the curvature of space.  _Mon. Not. Roy. Astron. Soc._ , 344:L65, 2003.
  * Gordon et al. (2021) L. Gordon, B.F. Li, and P. Singh.  Quantum gravitational onset of Starobinsky inflation in a closed universe.  _Phys. Rev. D_ , 103(4):046016, 2021.
  * Sloan et al. (2020) D. Sloan, K. Dimopoulos, and S. Karamitsos.  T-Model Inflation and Bouncing Cosmology.  _Phys. Rev. D_ , 101(4):043521, 2020.
  * Di Valentino et al. (2021d) E. Di Valentino, A. Melchiorri, O. Mena, S. Pan, and W. Yang.  Interacting Dark Energy in a closed universe.  _Mon. Not. Roy. Astron. Soc._ , 502(1):L23–L28, 2021d.
  * Knox and Millea (2020) L. Knox and M. Millea.  Hubble constant hunter’s guide.  _Phys. Rev. D_ , 101(4):043533, 2020.
  * Keeley and Shafieloo (2022) R.E. Keeley and A. Shafieloo.  Ruling Out New Physics at Low Redshift as a solution to the $H_{0}$ Tension.  6 2022.
  * Arendse et al. (2020) N. Arendse et al.  Cosmic dissonance: are new physics or systematics behind a short sound horizon?  _Astron. Astrophys._ , 639:A57, 2020.
  * Di Valentino et al. (2021e) E. Di Valentino, A. Mukherjee, and A.A. Sen.  Dark Energy with Phantom Crossing and the $H_{0}$ Tension.  _Entropy_ , 23(4):404, 2021e.
  * Chudaykin et al. (2022) A. Chudaykin, D. Gorbunov, and N. Nedelko.  Exploring $\Lambda$CDM extensions with SPT-3G and Planck data: 4$\sigma$ evidence for neutrino masses, full resolution of the Hubble crisis by dark energy with phantom crossing, and all that.  3 2022.
  * Koivisto (2005) T. Koivisto.  Growth of perturbations in dark matter coupled with quintessence.  _Phys. Rev. D_ , 72:043516, 2005.
  * Kase and Tsujikawa (2020) R. Kase and S. Tsujikawa.  Scalar-Field Dark Energy Nonminimally and Kinetically Coupled to Dark Matter.  _Phys. Rev. D_ , 101(6):063511, 2020.
  * Avelino and Sousa (2018) P.P. Avelino and L. Sousa.  Matter Lagrangian of particles and fluids.  _Phys. Rev. D_ , 97(6):064019, 2018.
  * Faraoni (2012) V. Faraoni.  The correspondence between a scalar field and an effective perfect fluid.  _Phys. Rev. D_ , 85:024040, 2012.
  * Frusciante et al. (2020) N. Frusciante, S. Peirone, L. Atayde, and A. De Felice.  Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds.  _Phys. Rev. D_ , 101(6):064001, 2020.
  * Carter et al. (2020) P. Carter, F. Beutler, W.J. Percival, J. DeRose, R.H. Wechsler, and C. Zhao.  The impact of the fiducial cosmology assumption on BAO distance scale measurements.  _Mon. Not. Roy. Astron. Soc._ , 494(2):2076–2089, 2020.
  * Adam et al. (2016) R. Adam et al.  Planck 2015 results. I. Overview of products and scientific results.  _Astron. Astrophys._ , 594:A1, 2016.
  * Creminelli and Vernizzi (2017) P. Creminelli and F. Vernizzi.  Dark Energy after GW170817 and GRB170817A.  _Phys. Rev. Lett._ , 119(25):251302, 2017.
  * Baker et al. (2017) T. Baker, E. Bellini, P.G. Ferreira, M. Lagos, J. Noller, and I. Sawicki.  Strong constraints on cosmological gravity from GW170817 and GRB 170817A.  _Phys. Rev. Lett._ , 119(25):251301, 2017.
  * Ezquiaga and Zumalacárregui (2017) J.M. Ezquiaga and M. Zumalacárregui.  Dark Energy After GW170817: Dead Ends and the Road Ahead.  _Phys. Rev. Lett._ , 119(25):251304, 2017.
  * Creminelli et al. (2018) P. Creminelli, M. Lewandowski, G. Tambalo, and F. Vernizzi.  Gravitational Wave Decay into Dark Energy.  _JCAP_ , 12:025, 2018.
  * Amendola et al. (2018) L. Amendola, M. Kunz, I.D. Saltas, and I. Sawicki.  Fate of Large-Scale Structure in Modified Gravity After GW170817 and GRB170817A.  _Phys. Rev. Lett._ , 120(13):131101, 2018.
  * Belgacem et al. (2018) E. Belgacem, Y. Dirian, S. Foffa, and M. Maggiore.  Modified gravitational-wave propagation and standard sirens.  _Phys. Rev. D_ , 98(2):023510, 2018.
  * Allahyari et al. (2022) A. Allahyari, R.C. Nunes, and D.F. Mota.  No slip gravity in light of LISA standard sirens.  _Mon. Not. Roy. Astron. Soc._ , 514(1):1274–1281, 2022.
  * Califano et al. (2023) M. Califano, I. de Martino, D. Vernieri, and S. Capozziello.  Exploiting the Einstein Telescope to solve the Hubble tension.  _Phys. Rev. D_ , 107(12):123519, 2023.
  * Ferreira et al. (2022) J. Ferreira, T. Barreiro, J. Mimoso, and N.J. Nunes.  Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens.  _Phys. Rev. D_ , 105(12):123531, 2022.
  * Abbott et al. (2017c) B.P. Abbott et al.  A gravitational-wave standard siren measurement of the Hubble constant.  _Nature_ , 551(7678):85–88, 2017c.
  * Chen et al. (2018) H.Y. Chen, M. Fishbach, and D.E. Holz.  A two per cent Hubble constant measurement from standard sirens within five years.  _Nature_ , 562(7728):545–547, 2018.
  * Hild et al. (2011) S. Hild et al.  Sensitivity Studies for Third-Generation Gravitational Wave Observatories.  _Class. Quant. Grav._ , 28:094013, 2011.
  * Feroz et al. (2009) F. Feroz, M.P. Hobson, and M. Bridges.  MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics.  _Mon. Not. Roy. Astron. Soc._ , 398:1601–1614, 2009.
  * Feroz et al. (2019) F. Feroz, M.P. Hobson, E. Cameron, and A.N. Pettitt.  Importance Nested Sampling and the MultiNest Algorithm.  _Open J. Astrophys._ , 2(1):10, 2019.
  * Buchner et al. (2014) J. Buchner, A. Georgakakis, K. Nandra, L. Hsu, C. Rangel, M. Brightman, A. Merloni, M. Salvato, J. Donley, and D. Kocevski.  X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue.  _Astron. Astrophys._ , 564:A125, 2014.
  * van de Bruck and Morrice (2015) C. van de Bruck and J. Morrice.  Disformal couplings and the dark sector of the universe.  _JCAP_ , 04:036, 2015.
  * Farrar and Peebles (2004) G.R. Farrar and P.J.E. Peebles.  Interacting dark matter and dark energy.  _Astrophys. J._ , 604:1–11, 2004.
  * Amendola (2004) L. Amendola.  Linear and non-linear perturbations in dark energy models.  _Phys. Rev. D_ , 69:103524, 2004.
  * Rugh and Zinkernagel (2002) S. Rugh and H. Zinkernagel.  The Quantum vacuum and the cosmological constant problem.  _Stud. Hist. Phil. Sci. B_ , 33:663–705, 2002.
  * Gao et al. (2010) C. Gao, M. Kunz, A.R. Liddle, and D. Parkinson.  Unified dark energy and dark matter from a scalar field different from quintessence.  _Phys. Rev. D_ , 81:043520, 2010.
  * Ansoldi and Guendelman (2013) S. Ansoldi and E.I. Guendelman.  Unified Dark Energy-Dark Matter model with Inverse Quintessence.  _JCAP_ , 05:036, 2013.
  * Arbey and Coupechoux (2021) A. Arbey and J.F. Coupechoux.  Unifying dark matter, dark energy and inflation with a fuzzy dark fluid.  _JCAP_ , 01:033, 2021.
  * Brandenberger et al. (2019a) R. Brandenberger, R.R. Cuzinatto, J. Fröhlich, and R. Namba.  New Scalar Field Quartessence.  _JCAP_ , 02:043, 2019a.
  * Koivisto et al. (2014) T. Koivisto, D. Wills, and I. Zavala.  Dark D-brane Cosmology.  _JCAP_ , 1406:036, 2014.
  * McAllister and Silverstein (2008) L. McAllister and E. Silverstein.  String Cosmology: A Review.  _Gen. Rel. Grav._ , 40:565–605, 2008.
  * Garriga and Mukhanov (1999) J. Garriga and V.F. Mukhanov.  Perturbations in k-inflation.  _Phys. Lett. B_ , 458:219–225, 1999.
  * Silverstein and Tong (2004) E. Silverstein and D. Tong.  Scalar speed limits and cosmology: Acceleration from D-cceleration.  _Phys. Rev. D_ , 70:103505, 2004.
  * Alishahiha et al. (2004) M. Alishahiha, E. Silverstein, and D. Tong.  DBI in the sky.  _Phys. Rev. D_ , 70:123505, 2004.
  * Panda et al. (2006) S. Panda, M. Sami, and S. Tsujikawa.  Inflation and dark energy arising from geometrical tachyons.  _Phys. Rev. D_ , 73:023515, 2006.
  * Chimento and Lazkoz (2008) L.P. Chimento and R. Lazkoz.  Bridging geometries and potentials in DBI cosmologies.  _Gen. Rel. Grav._ , 40:2543–2555, 2008.
  * Abramo et al. (2004) L.R. Abramo, F. Finelli, and T.S. Pereira.  Constraining Born-Infeld models of dark energy with CMB anisotropies.  _Phys. Rev. D_ , 70:063517, 2004.
  * Martin and Yamaguchi (2008) J. Martin and M. Yamaguchi.  DBI-essence.  _Phys. Rev. D_ , 77:123508, 2008.
  * Guo and Ohta (2008) Z.K. Guo and N. Ohta.  Cosmological Evolution of Dirac-Born-Infeld Field.  _JCAP_ , 04:035, 2008.
  * Gumjudpai and Ward (2009) B. Gumjudpai and J. Ward.  Generalised DBI-Quintessence.  _Phys. Rev. D_ , 80:023528, 2009.
  * Ahn et al. (2010) C. Ahn, C. Kim, and E.V. Linder.  Cosmological Constant Behavior in DBI Theory.  _Phys. Lett. B_ , 684:181–184, 2010.
  * Ahn et al. (2009) C. Ahn, C. Kim, and E.V. Linder.  Dark Energy Properties in DBI Theory.  _Phys. Rev. D_ , 80:123016, 2009.
  * Chimento et al. (2009) L.P. Chimento, R. Lazkoz, and I. Sendra.  Dbi models for the unification of dark matter and dark energy.  _General Relativity and Gravitation_ , 42(5):1189–1209, Oct 2009.
  * Copeland et al. (2010) E.J. Copeland, S. Mizuno, and M. Shaeri.  Cosmological Dynamics of a Dirac-Born-Infeld field.  _Phys. Rev. D_ , 81:123501, 2010.
  * Brax et al. (2013) P. Brax, C. Burrage, and A.C. Davis.  Screening fifth forces in k-essence and DBI models.  _JCAP_ , 01:020, 2013.
  * Kaeonikhom et al. (2012) C. Kaeonikhom, D. Singleton, S.V. Sushkov, and N. Yongram.  Dynamics of Dirac-Born-Infeld dark energy interacting with dark matter.  _Phys. Rev. D_ , 86:124049, 2012.
  * Burrage and Khoury (2014) C. Burrage and J. Khoury.  Screening of scalar fields in Dirac-Born-Infeld theory.  _Phys. Rev. D_ , 90(2):024001, 2014.
  * Mahata and Chakraborty (2015) N. Mahata and S. Chakraborty.  Dynamical system analysis for DBI dark energy interacting with dark matter.  _Mod. Phys. Lett. A_ , 30(02):1550009, 2015.
  * Panpanich et al. (2017) S. Panpanich, K.i. Maeda, and S. Mizuno.  Cosmological Dynamics of D-BIonic and DBI Scalar Field and Coincidence Problem of Dark Energy.  _Phys. Rev. D_ , 95(10):103520, 2017.
  * Koivisto and Wills (2013) T.S. Koivisto and D.E. Wills.  Matters on a moving brane.  _Int. J. Mod. Phys. D_ , 22:1342024, 2013.
  * Koivisto and Urban (2015a) T.S. Koivisto and F.R. Urban.  Disformal vectors and anisotropies on a warped braneHulluilla on Halvat Huvit.  _JCAP_ , 1503(03):003, 2015a.
  * Koivisto and Urban (2015b) T.S. Koivisto and F.R. Urban.  Doubly-boosted vector cosmologies from disformal metrics.  _Phys. Scripta_ , 90(9):095301, 2015b.
  * Cembranos and Maroto (2016) J.A.R. Cembranos and A.L. Maroto.  Disformal scalars as dark matter candidates: Branon phenomenology.  _Int. J. Mod. Phys._ , 31(14n15):1630015, 2016\.
  * de Rham and Gabadadze (2010) C. de Rham and G. Gabadadze.  Generalization of the Fierz-Pauli Action.  _Phys. Rev._ , D82:044020, 2010.
  * Clayton and Moffat (1999) M.A. Clayton and J.W. Moffat.  Dynamical mechanism for varying light velocity as a solution to cosmological problems.  _Phys. Lett._ , B460:263–270, 1999.
  * Bettoni et al. (2011) D. Bettoni, S. Liberati, and L. Sindoni.  Extended LCDM: generalized non-minimal coupling for dark matter fluids.  _JCAP_ , 1111:007, 2011.
  * Deruelle and Rua (2014) N. Deruelle and J. Rua.  Disformal Transformations, Veiled General Relativity and Mimetic Gravity.  _JCAP_ , 1409:002, 2014.
  * Brax (2012) P. Brax.  Lorentz Invariance Violation in Modified Gravity.  _Phys. Lett._ , B712:155–160, 2012.
  * Olmo et al. (2009) G.J. Olmo, H. Sanchis-Alepuz, and S. Tripathi.  Dynamical Aspects of Generalized Palatini Theories of Gravity.  _Phys. Rev._ , D80:024013, 2009.
  * Sakstein (2015) J. Sakstein.  Towards Viable Cosmological Models of Disformal Theories of Gravity.  _Phys. Rev._ , D91(2):024036, 2015.
  * Ezquiaga et al. (2017) J.M. Ezquiaga, J. García-Bellido, and M. Zumalacárregui.  Field redefinitions in theories beyond Einstein gravity using the language of differential forms.  _Phys. Rev._ , D95(8):084039, 2017.
  * Kaloper (2004) N. Kaloper.  Disformal inflation.  _Phys. Lett._ , B583:1–13, 2004.
  * van de Bruck et al. (2016b) C. van de Bruck, T. Koivisto, and C. Longden.  Disformally coupled inflation.  _JCAP_ , 1603(03):006, 2016b.
  * Koivisto (2008) T.S. Koivisto.  Disformal quintessence, 11 2008.
  * Zumalacarregui et al. (2010) M. Zumalacarregui, T.S. Koivisto, D.F. Mota, and P. Ruiz-Lapuente.  Disformal Scalar Fields and the Dark Sector of the Universe.  _JCAP_ , 1005:038, 2010.
  * Noller (2012) J. Noller.  Derivative Chameleons.  _JCAP_ , 1207:013, 2012.
  * Bettoni et al. (2012) D. Bettoni, V. Pettorino, S. Liberati, and C. Baccigalupi.  Non-minimally coupled dark matter: effective pressure and structure formation.  _JCAP_ , 1207:027, 2012.
  * Koivisto et al. (2012) T.S. Koivisto, D.F. Mota, and M. Zumalacarregui.  Screening Modifications of Gravity through Disformally Coupled Fields.  _Phys. Rev. Lett._ , 109:241102, 2012.
  * Zumalacarregui et al. (2013) M. Zumalacarregui, T.S. Koivisto, and D.F. Mota.  DBI Galileons in the Einstein Frame: Local Gravity and Cosmology.  _Phys. Rev. D_ , 87:083010, 2013.
  * Sakstein and Verner (2015) J. Sakstein and S. Verner.  Disformal Gravity Theories: A Jordan Frame Analysis.  _Phys. Rev._ , D92(12):123005, 2015.
  * Bettoni and Liberati (2015) D. Bettoni and S. Liberati.  Dynamics of non-minimally coupled perfect fluids.  _JCAP_ , 1508(08):023, 2015.
  * Teixeira et al. (2019) E.M. Teixeira, A. Nunes, and N.J. Nunes.  Conformally Coupled Tachyonic Dark Energy.  _Phys. Rev. D_ , 100(4):043539, 2019.
  * Das et al. (2006) S. Das, P.S. Corasaniti, and J. Khoury.  Super-acceleration as signature of dark sector interaction.  _Phys. Rev. D_ , 73:083509, 2006.
  * Bahamonde et al. (2018) S. Bahamonde, C.G. Böhmer, S. Carloni, E.J. Copeland, W. Fang, and N. Tamanini.  Dynamical systems applied to cosmology: dark energy and modified gravity.  _Phys. Rept._ , 775-777:1–122, 2018.
  * Pettorino et al. (2013) V. Pettorino, L. Amendola, and C. Wetterich.  How early is early dark energy?  _Phys. Rev. D_ , 87:083009, 2013.
  * Tsujikawa (2007) S. Tsujikawa.  Matter density perturbations and effective gravitational constant in modified gravity models of dark energy.  _Phys. Rev. D_ , 76:023514, 2007.
  * Di Valentino et al. (2022) E. Di Valentino, W. Giarè, A. Melchiorri, and J. Silk.  Health checkup test of the standard cosmological model in view of recent cosmic microwave background anisotropies experiments.  _Phys. Rev. D_ , 106(10):103506, 2022.
  * Di Valentino (2017) E. Di Valentino.  Crack in the cosmological paradigm.  _Nature Astron._ , 1(9):569–570, 2017.
  * Di Valentino and Mena (2020) E. Di Valentino and O. Mena.  A fake Interacting Dark Energy detection?  _Mon. Not. Roy. Astron. Soc._ , 500(1):L22–L26, 2020.
  * Di Valentino and Bridle (2018) E. Di Valentino and S. Bridle.  Exploring the tension between current cosmic microwave background and cosmic shear data.  _Symmetry_ , 10(11), 2018.
  * Jungman et al. (1996) G. Jungman, M. Kamionkowski, and K. Griest.  Supersymmetric dark matter.  _Phys. Rept._ , 267:195–373, 1996.
  * Bertone et al. (2005) G. Bertone, D. Hooper, and J. Silk.  Particle dark matter: Evidence, candidates and constraints.  _Phys. Rept._ , 405:279–390, 2005.
  * Holman et al. (1983) R. Holman, G. Lazarides, and Q. Shafi.  Axions and the Dark Matter of the Universe.  _Phys. Rev. D_ , 27:995, 1983.
  * Blumenthal et al. (1984) G.R. Blumenthal, S.M. Faber, J.R. Primack, and M.J. Rees.  Formation of Galaxies and Large Scale Structure with Cold Dark Matter.  _Nature_ , 311:517–525, 1984.
  * Chung et al. (1998) D.J.H. Chung, E.W. Kolb, and A. Riotto.  Superheavy dark matter.  _Phys. Rev. D_ , 59:023501, 1998.
  * Hlozek et al. (2015) R. Hlozek, D. Grin, D.J.E. Marsh, and P.G. Ferreira.  A search for ultralight axions using precision cosmological data.  _Phys. Rev. D_ , 91(10):103512, 2015.
  * Marsh (2016) D.J.E. Marsh.  Axion Cosmology.  _Phys. Rept._ , 643:1–79, 2016.
  * Ballesteros et al. (2017) G. Ballesteros, J. Redondo, A. Ringwald, and C. Tamarit.  Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism.  _Phys. Rev. Lett._ , 118(7):071802, 2017.
  * Hlozek et al. (2018) R. Hlozek, D.J.E. Marsh, and D. Grin.  Using the Full Power of the Cosmic Microwave Background to Probe Axion Dark Matter.  _Mon. Not. Roy. Astron. Soc._ , 476(3):3063–3085, 2018.
  * Roszkowski et al. (2018) L. Roszkowski, E.M. Sessolo, and S. Trojanowski.  WIMP dark matter candidates and searches—current status and future prospects.  _Rept. Prog. Phys._ , 81(6):066201, 2018.
  * D’Amico et al. (2016) G. D’Amico, T. Hamill, and N. Kaloper.  Quantum field theory of interacting dark matter and dark energy: Dark monodromies.  _Phys. Rev. D_ , 94(10):103526, 2016.
  * Carrillo González and Trodden (2018) M. Carrillo González and M. Trodden.  Field Theories and Fluids for an Interacting Dark Sector.  _Phys. Rev. D_ , 97(4):043508, 2018.  [Erratum: Phys.Rev.D 101, 089901 (2020)].
  * Benisty and Guendelman (2018) D. Benisty and E.I. Guendelman.  Unified dark energy and dark matter from dynamical spacetime.  _Phys. Rev. D_ , 98(2):023506, 2018.
  * Brandenberger et al. (2019b) R. Brandenberger, J. Fröhlich, and R. Namba.  Unified Dark Matter, Dark Energy and baryogenesis via a “cosmological wetting transition”.  _JCAP_ , 09:069, 2019b.
  * Brandenberger and Fröhlich (2021) R. Brandenberger and J. Fröhlich.  Dark Energy, Dark Matter and Baryogenesis from a Model of a Complex Axion Field.  _JCAP_ , 04:030, 2021.
  * Johnson and Shankaranarayanan (2021) J.P. Johnson and S. Shankaranarayanan.  Cosmological perturbations in the interacting dark sector: Mapping fields and fluids.  _Phys. Rev. D_ , 103(2):023510, 2021.
  * Sá (2021) P.M. Sá.  Late-time evolution of the Universe within a two-scalar-field cosmological model.  _Phys. Rev. D_ , 103:123517, 2021.
  * Johnson et al. (2022) J.P. Johnson, A. Sangwan, and S. Shankaranarayanan.  Observational constraints and predictions of the interacting dark sector with field-fluid mapping.  _JCAP_ , 01(01):024, 2022.
  * Linde (1994) A.D. Linde.  Hybrid inflation.  _Phys. Rev. D_ , 49:748–754, 1994.
  * Axenides and Dimopoulos (2004) M. Axenides and K. Dimopoulos.  Hybrid dark sector: Locked quintessence and dark matter.  _JCAP_ , 07:010, 2004.
  * Turner (1983) M.S. Turner.  Coherent scalar-field oscillations in an expanding universe.  _Phys. Rev. D_ , 28:1243–1247, Sep 1983.
  * Marsh et al. (2014) D.J.E. Marsh, D. Grin, R. Hlozek, and P.G. Ferreira.  Tensor Interpretation of BICEP2 Results Severely Constrains Axion Dark Matter.  _Phys. Rev. Lett._ , 113(1):011801, 2014.
  * Folkerts et al. (2014) S. Folkerts, C. Germani, and J. Redondo.  Axion Dark Matter and Planck favor non-minimal couplings to gravity.  _Phys. Lett. B_ , 728:532–536, 2014.
  * Hu et al. (2000) W. Hu, R. Barkana, and A. Gruzinov.  Cold and fuzzy dark matter.  _Phys. Rev. Lett._ , 85:1158–1161, 2000.
  * Hui et al. (2017) L. Hui, J.P. Ostriker, S. Tremaine, and E. Witten.  Ultralight scalars as cosmological dark matter.  _Phys. Rev. D_ , 95(4):043541, 2017.
  * Kolb et al. (1999) E.W. Kolb, D.J.H. Chung, and A. Riotto.  WIMPzillas!  _AIP Conf. Proc._ , 484(1):91–105, 1999.
  * Kofman et al. (1997) L. Kofman, A.D. Linde, and A.A. Starobinsky.  Towards the theory of reheating after inflation.  _Phys. Rev. D_ , 56:3258–3295, 1997.
  * Lyth and Riotto (1999) D.H. Lyth and A. Riotto.  Particle physics models of inflation and the cosmological density perturbation.  _Phys. Rept._ , 314:1–146, 1999.
  * Ferreira and Joyce (1998) P.G. Ferreira and M. Joyce.  Cosmology with a primordial scaling field.  _Phys. Rev. D_ , 58:023503, 1998.
  * Amendola (2001) L. Amendola.  Dark energy and the Boomerang data.  _Phys. Rev. Lett._ , 86:196–199, 2001.
  * Pettorino (2013) V. Pettorino.  Testing modified gravity with Planck: the case of coupled dark energy.  _Phys. Rev. D_ , 88:063519, 2013.
  * Xia (2013) J.Q. Xia.  New Limits on Coupled Dark Energy from Planck.  _JCAP_ , 11:022, 2013.
  * Agrawal et al. (2021) P. Agrawal, G. Obied, and C. Vafa.  $H_{0}$ tension, swampland conjectures, and the epoch of fading dark matter.  _Phys. Rev. D_ , 103(4):043523, 2021.
  * Pettorino and Baccigalupi (2008) V. Pettorino and C. Baccigalupi.  Coupled and Extended Quintessence: theoretical differences and structure formation.  _Phys. Rev. D_ , 77:103003, 2008.
  * Marulli et al. (2021) F. Marulli, A. Veropalumbo, J.E. García-Farieta, M. Moresco, L. Moscardini, and A. Cimatti.  C3 Cluster Clustering Cosmology I. New Constraints on the Cosmic Growth Rate at z $\sim$ 0.3 from Redshift-space Clustering Anisotropies.  _Astrophys. J._ , 920(1):13, 2021.
  * Cai et al. (2018) R.G. Cai, T.B. Liu, X.W. Liu, S.J. Wang, and T. Yang.  Probing cosmic anisotropy with gravitational waves as standard sirens.  _Phys. Rev._ , D97(10):103005, 2018.
  * Hilborn (2018) R.C. Hilborn.  Gravitational waves from orbiting binaries without general relativity.  _Am. J. Phys._ , 86(3):186–197, 2018.
  * Li (2013) T.G.F. Li.  _Extracting Physics from Gravitational Waves: Testing the Strong-field Dynamics of General Relativity and Inferring the Large-scale Structure of the Universe_.  PhD thesis, Vrije U., Amsterdam, 2013.
  * Abadie et al. (2010) J. Abadie et al.  Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run.  _Nucl. Instrum. Meth. A_ , 624:223–240, 2010.
  * Nishizawa et al. (2011) A. Nishizawa, A. Taruya, and S. Saito.  Tracing the redshift evolution of Hubble parameter with gravitational-wave standard sirens.  _Phys. Rev. D_ , 83:084045, 2011.
  * Gair et al. (2017) J.R. Gair, S. Babak, A. Sesana, P. Amaro-Seoane, E. Barausse, C.P.L. Berry, E. Berti, and C. Sopuerta.  Prospects for observing extreme-mass-ratio inspirals with LISA.  _J. Phys. Conf. Ser._ , 840(1):012021, 2017.
  * Caprini and Tamanini (2016) C. Caprini and N. Tamanini.  Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission.  _JCAP_ , 10:006, 2016.
  * Seoane et al. (2013) P.A. Seoane et al.  The Gravitational Universe, 5 2013.
  * Amaro-Seoane et al. (2013) P. Amaro-Seoane et al.  eLISA/NGO: Astrophysics and cosmology in the gravitational-wave millihertz regime.  _GW Notes_ , 6:4–110, 2013.
  * Mapelli et al. (2010) M. Mapelli, C. Huwyler, L. Mayer, P. Jetzer, and A. Vecchio.  Gravitational waves from intermediate-mass black holes in young clusters.  _Astrophys. J._ , 719:987–995, 2010.
  * Klein et al. (2016) A. Klein et al.  Science with the space-based interferometer eLISA: Supermassive black hole binaries.  _Phys. Rev._ , D93(2):024003, 2016.
  * Tamanini et al. (2016) N. Tamanini, C. Caprini, E. Barausse, A. Sesana, A. Klein, and A. Petiteau.  Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens.  _JCAP_ , 1604(04):002, 2016.
  * Hou et al. (2023) W.T. Hou, J.Z. Qi, T. Han, J.F. Zhang, S. Cao, and X. Zhang.  Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation.  _JCAP_ , 05:017, 2023.
  * Hubeny (2015) V.E. Hubeny.  The AdS/CFT Correspondence.  _Class. Quant. Grav._ , 32(12):124010, 2015.
  * Shandera and Tye (2006) S.E. Shandera and S.H.H. Tye.  Observing brane inflation.  _JCAP_ , 05:007, 2006.
  * Bean et al. (2007) R. Bean, S.E. Shandera, S.H. Henry Tye, and J. Xu.  Comparing brane inflation to WMAP.  _JCAP_ , 05:004, 2007.
  * Durrer et al. (2005) R. Durrer, M. Kunz, and M. Sakellariadou.  Why do we live in 3+1 dimensions?  _Phys. Lett. B_ , 614:125–130, 2005.
  * Chen (2008) X. Chen.  Fine-Tuning in DBI Inflationary Mechanism.  _JCAP_ , 12:009, 2008.
  * Maldacena (1998) J.M. Maldacena.  The Large N limit of superconformal field theories and supergravity.  _Adv. Theor. Math. Phys._ , 2:231–252, 1998.