[1] A. G. Riess et al., Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Astron. J. 116, 1009–1038, (1998).
[2] S. Perlmutter et al., Measurements of Ω and Λ from 42 High-Redshift Supernovae, Astrophys. J. 517, 565–586, (1999).
[3] Planck Collaboration, Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641, A6, (2020).
[4] D. J. Eisenstein et al., Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies, Astrophys. J. 633, 560–574, (2005).
[5] S. Alam et al. (eBOSS Collaboration), Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory, Phys. Rev. D 103, 083533, (2021).
[6] T. Erben et al., CFHTLenS: the CanadaFranceHawaii Telescope Lensing Survey - imaging data and catalog products, Mon. Not. R. Astron. Soc. 433, 2545–2563, (2013).
[7] T. M. C. Abbott et al. (DES Collaboration), Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing, Phys. Rev. D 98, 043526, (2018).
[8] S. Weinberg, The cosmological constant problem, Rev. Mod. Phys. 61, 1–23, (1989).
[9] P. J. E. Peebles and B. Ratra, The cosmological constant and dark energy, Rev. Mod. Phys. 75, 559–606, (2003).
[10] J. Martin, Everything you always wanted to know about the cosmological constant problem (but were afraid to ask), Comptes Rendus Physique 13, 566–665, (2012).
[11] A. G. Riess et al., Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond ΛCDM, Astrophys. J. 876, 85, (2019).
[12] L. Verde, T. Treu, and A. G. Riess, Tensions between the Early and the Late Universe, Nat. Astron. 3, 891–895, (2019).
[13] B. Ratra and P. J. E. Peebles, Cosmological consequences of a rolling homogeneous scalar field, Phys. Rev. D 37, 3406–3427, (1988).
[14] R. R. Caldwell, R. Dave, and P. J. Steinhardt, Cosmological Imprint of an Energy Component with General Equation of State, Phys. Rev. Lett. 80, 1582–1585, (1998).
[15] R. R. Caldwell, A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state, Phys. Lett. B 545, 23–29, (2002).
[16] C. Armendariz-Picon, V. Mukhanov, and P. J. Steinhardt, Essentials of k-essence, Phys. Rev. D 63, 103510, (2001).
[17] T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified gravity and cosmology, Phys. Rep. 513, 1–189, (2012).
[18] A. Joyce, B. Jain, J. Khoury, and M. Trodden, Beyond the cosmological standard model, Phys. Rep. 568, 1–98, (2015). [19] M. Chevallier and D. Polarski, Accelerating Universes with Scaling Dark Matter, Int. J. Mod. Phys. D 10, 213–224, (2001).
[20] E. V. Linder, Exploring the Expansion History of the Universe, Phys. Rev. Lett. 90, 091301, (2003).
[21] D. Huterer and D. L. Shafer, Dark energy two decades after: Observables, probes, consistency tests, Rep. Prog. Phys. 81, 016901, (2017).
[22] S. Nojiri and S. D. Odintsov, Inhomogeneous equation of state of the Universe: Phantom era, future singularity and crossing the phantom barrier, Phys. Rev. D 72, 023003, (2005).
[23] S. Capozziello, V. F. Cardone, and A. Troisi, Dark energy and dark matter as curvature effects, Phys. Rev. D 73, 104019, (2006).
[24] K. Bamba, S. Capozziello, S. Nojiri, and S. D. Odintsov, Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests, Astrophys. Space Sci. 342, 155–228, (2012).
[25] L. Amendola et al., Cosmology and fundamental physics with the Euclid satellite, Living Rev. Relativ. 21, 2, (2018).
[26] Z. Ivezic et al., LSST: From Science Drivers to Reference Design and Anticipated Data Products, Astrophys. J. 873, 111, (2019).
[27] D. Spergel et al., Wide-Field Infrared Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA Final Report, arXiv:1503.03757, (2015).
[28] E. J. Copeland, M. Sami, and S. Tsujikawa, Dynamics of dark energy, Int. J. Mod. Phys. D 15, 1753–1936, (2006).
[29] L. Amendola and S. Tsujikawa, Dark Energy: Theory and Observations, Cambridge University Press, Cambridge, 2010.