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The recent evidence for dynamical dark energy from DESI, in combination with other cosmological data, has generated significant interest in understanding the nature of dark energy and its underlying microphysics.
1902
Earlier work this paper cites.
R. Kallosh and A. Linde, On hilltop and brane inflation after Planck , JCAP 09
1906
Earlier work this paper cites.
1908
Earlier work this paper cites.
1909
Earlier work this paper cites.
1911
Earlier work this paper cites.
N. Metropolis, A.W. Rosenbluth, M.N. Rosenbluth, A.H. Teller and E. Teller, Equation of state calculations by fast computing machines , The Journal of Chemical Physics 21
1953
Earlier work this paper cites.
W.K. Hastings, Monte Carlo sampling methods using Markov chains and their applications , Biometrika 57
1970
Earlier work this paper cites.
A. Gelman and D.B. Rubin, Inference from Iterative Simulation Using Multiple Sequences , Statistical Science 7
1992
Earlier work this paper cites.
S. Dodelson, W.H. Kinney and E.W. Kolb, Cosmic microwave background measurements can discriminate among inflation models , Phys. Rev. D 56
1997
Earlier work this paper cites.
G. Efstathiou, Constraining the equation of state of the universe from distant type Ia supernovae and cosmic microwave background anisotropies , Mon. Not. Roy. Astron. Soc. 310
1999
Earlier work this paper cites.
A.R. Cooray and D. Huterer, Gravitational lensing as a probe of quintessence , Astrophys. J. Lett. 513
1999
Earlier work this paper cites.
L. Amendola, Coupled quintessence , Phys. Rev. D 62
2000
Earlier work this paper cites.
M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter , Int. J. Mod. Phys. D 10
2001
Earlier work this paper cites.
X. Li and A. Shafieloo, Evidence for Emergent Dark Energy , Astrophys. J. 902
2001
Earlier work this paper cites.
A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach , Phys. Rev. D66
2002
Earlier work this paper cites.
P.J.E. Peebles and B. Ratra, The Cosmological Constant and Dark Energy , Rev. Mod. Phys. 75
2003
Earlier work this paper cites.
E.V. Linder, Exploring the expansion history of the universe , Phys. Rev. Lett. 90
2003
Earlier work this paper cites.
2004
Earlier work this paper cites.
H.K. Jassal, J.S. Bagla and T. Padmanabhan, Observational constraints on low redshift evolution of dark energy: How consistent are different observations? , Phys. Rev. D 72
2005
Earlier work this paper cites.
Y.-g. Gong and Y.-Z. Zhang, Probing the curvature and dark energy , Phys. Rev. D 72
2005
Earlier work this paper cites.
R.R. Caldwell and E.V. Linder, The Limits of quintessence , Phys. Rev. Lett. 95
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
E.V. Linder, The paths of quintessence , Phys. Rev. D 73
2006
Earlier work this paper cites.
R.J. Scherrer, Dark energy models in the w-w’ plane , Phys. Rev. D 73
2006
Earlier work this paper cites.
T.E. Oliphant, A guide to NumPy , vol. 1, Trelgol Publishing USA (2006)
2006
Earlier work this paper cites.
J.D. Hunter, Matplotlib: A 2d graphics environment , Computing in Science & Engineering 9
2007
Earlier work this paper cites.
2008
Earlier work this paper cites.
E.M. Barboza, Jr. and J.S. Alcaniz, A parametric model for dark energy , Phys. Lett. B 666
2008
Earlier work this paper cites.
R.J. Scherrer and A.A. Sen, Thawing quintessence with a nearly flat potential , Phys. Rev. D 77
2008
Earlier work this paper cites.
S. Dutta and R.J. Scherrer, Hilltop Quintessence , Phys. Rev. D 78
2008
Earlier work this paper cites.
T. Chiba, Slow-Roll Thawing Quintessence , Phys. Rev. D 79
2009
Earlier work this paper cites.
2011
Cited alongside, same era.
S. Van Der Walt, S.C. Colbert and G. Varoquaux, The numpy array: a structure for efficient numerical computation , Computing in Science & Engineering 13
2011
Cited alongside, same era.
2012
Cited alongside, same era.
A. Lewis, Efficient sampling of fast and slow cosmological parameters , Phys. Rev. D87
2013
Cited alongside, same era.
N. Roy, Dynamical dark energy in the light of DESI 2024 data , arXiv:2406.00634
2024
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A. Notari, M. Redi and A. Tesi, Consistent theories for the DESI dark energy fit , JCAP 11
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2014
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2014
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J. Martin, C. Ringeval and V. Vennin, Encyclopædia Inflationaris , Phys. Dark Univ. 5-6
2014
Cited alongside, same era.
2015
Cited alongside, same era.
E.V. Linder, Quintessence’s last stand? , Phys. Rev. D 91
2015
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2016
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2016
Cited alongside, same era.
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W. Yin, Cosmic clues: DESI, dark energy, and the cosmological constant problem , JHEP 05
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M. Cortês and A.R. Liddle, Interpreting DESI’s evidence for evolving dark energy , JCAP 12
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W.J. Wolf, Minimizing the tensor-to-scalar ratio in single-field inflation models , Phys. Rev. D 110
2024
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2025
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B.R. Dinda and R. Maartens, Model-agnostic assessment of dark energy after DESI DR1 BAO , JCAP 01
2025
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