Built on

T. Kobayashi, Horndeski theory and beyond: a review, Rept. Prog. Phys. 82
Original
1901
Earlier work this paper cites.
C. Dalang and L. Lombriser, Limitations on Standard Sirens tests of gravity from screening, JCAP 10
Original
1906
Earlier work this paper cites.
N. Aghanim et al. (Planck), Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
E. Bellini, I. Sawicki, and M. Zumalacárregui, hi_class background evolution, initial conditions and approximation schemes, J. Cosmology Astropart. Phys 2020
Original
1909
Earlier work this paper cites.
W. J. Wolf and M. Lagos, Standard Sirens as a Novel Probe of Dark Energy, Phys. Rev. Lett. 124
Original
1910
Earlier work this paper cites.
C. García-García, E. Bellini, P. G. Ferreira, D. Traykova, and M. Zumalacárregui, Theoretical priors in scalar-tensor cosmologies: Thawing quintessence, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
H. Jeffreys, The Theory of Probability , 1st ed., Oxford Classic Texts in the Physical Sciences (Oxford University Press, Oxford, 1939)
1939
Earlier work this paper cites.
C. G. Callan, Jr., S. R. Coleman, and R. Jackiw, A New improved energy - momentum tensor, Annals Phys. 59
1970
Earlier work this paper cites.
A. I. Vainshtein, To the problem of nonvanishing gravitation mass, Phys. Lett. B 39
1972
Earlier work this paper cites.
N. D. Birrell and P. C. W. Davies, Quantum Fields in Curved Space , Cambridge Monographs on Mathematical Physics (Cambridge University Press, 1982)
1982
Earlier work this paper cites.
M. S. Madsen, Scalar Fields in Curved Space-times, Class. Quant. Grav. 5
1988
Earlier work this paper cites.
I. L. Buchbinder, Effective Action in Quantum Gravity , 1st ed. (Routledge, 1992)
1992
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.
G. Esposito-Farese and D. Polarski, Scalar tensor gravity in an accelerating universe, Phys. Rev. D 63
2001
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.
M. Lagos and H. Zhu, Gravitational couplings in Chameleon models, JCAP 06
Original
2003
Earlier work this paper cites.
E. G. Adelberger, B. R. Heckel, and A. E. Nelson, Tests of the gravitational inverse-square law, Ann. Rev. Nuc. & Part. Sci. 53
2003
Earlier work this paper cites.
B. Bertotti, L. Iess, and P. Tortora, A test of General Relativity using radio links with the Cassini spacecraft, Nature 425
2003
Earlier work this paper cites.
J. Khoury and A. Weltman, Chameleon cosmology, Phys. Rev. D 69
2004
Earlier work this paper cites.
A. Gómez-Valent, V. Pettorino, and L. Amendola, Update on coupled dark energy and the H 0 H_{0} tension, Phys. Rev. D 101
Original
2004
Earlier work this paper cites.
J. Torrado and A. Lewis, Cobaya: Code for Bayesian Analysis of hierarchical physical models, JCAP 05
Original
2005
Earlier work this paper cites.
S. Räsänen, Accelerated expansion from structure formation, Journal of Cosmology and Astroparticle Physics 2006
2006
Earlier work this paper cites.
R. Trotta, Applications of Bayesian model selection to cosmological parameters, Mon. Not. Roy. Astron. Soc. 378
2007
Earlier work this paper cites.
S. Alam et al. (eBOSS), 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
Original
2007
Earlier work this paper cites.
S. Dutta and R. J. Scherrer, Hilltop Quintessence, Phys. Rev. D 78
Original
2008
Earlier work this paper cites.
N. J. Secrest, S. von Hausegger, M. Rameez, R. Mohayaee, S. Sarkar, and J. Colin, A Test of the Cosmological Principle with Quasars, Astrophys. J. Lett. 908
Original
2009
Earlier work this paper cites.
M. Park, K. M. Zurek, and S. Watson, A Unified Approach to Cosmic Acceleration, Phys. Rev. D 81
Original
2010
Earlier work this paper cites.
A. Heinesen, Multipole decomposition of the general luminosity distance Hubble law—a new framework for observational cosmology, Journal of Cosmology and Astroparticle Physics 2021
Original
2010
Earlier work this paper cites.
S. Nojiri and S. D. Odintsov, Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models, Phys. Rept. 505
Original
2011
Earlier work this paper cites.
D. Blas, J. Lesgourgues, and T. Tram, The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes, J. Cosmology Astropart. Phys 2011
Original
2011
Earlier work this paper cites.
F. Beutler, C. Blake, M. Colless, D. H. Jones, L. Staveley-Smith, G. B. Poole, L. Campbell, Q. Parker, W. Saunders, and F. Watson, The 6dF Galaxy Survey: z ≈ \approx 0 measurements of the growth rate and σ \sigma 8
Original
2012
Earlier work this paper cites.
C. Blake, S. Brough, M. Colless, C. Contreras, W. Couch, S. Croom, D. Croton, T. M. Davis, M. J. Drinkwater, K. Forster, D. Gilbank, M. Gladders, K. Glazebrook, B. Jelliffe, R. J. Jurek, I. h. Li, B. Madore, D. C. Martin, K. Pimbblet, G. B. Poole, M. Pracy, R. Sharp, E. Wisnioski, D. Woods, T. K. Wyder, and H. K. C. Yee, The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z ¡ 1, MNRAS 425
Original
2012
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D. E. Smith et al. , Gravity Field and Internal Structure of Mercury from MESSENGER, Science 336
2012
Earlier work this paper cites.
T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified Gravity and Cosmology, Phys. Rept. 513
Original
2012
Earlier work this paper cites.
T. Buchert and S. Räsänen, Backreaction in Late-Time Cosmology, Annual Review of Nuclear and Particle Science 62
Original
2012
Earlier work this paper cites.
C. M. Will, The Confrontation between General Relativity and Experiment, Living Rev. Rel. 17
Original
2014
Earlier work this paper cites.
W. J. Handley, M. P. Hobson, and A. N. Lasenby, PolyChord: nested sampling for cosmology, Mon. Not. Roy. Astron. Soc. 450
Original
2015
Earlier work this paper cites.
T. Buchert et al. , Is there proof that backreaction of inhomogeneities is irrelevant in cosmology?, Classical and Quantum Gravity 32
Original
2015
Earlier work this paper cites.
T. Okumura et al. , The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at z ∼ 1.4 z\sim 1.4 , Publ. Astron. Soc. Jap. 68
Original
2016
Earlier work this paper cites.

Similar

D. I. Kaiser, Nonminimal Couplings in the Early Universe: Multifield Models of Inflation and the Latest Observations, Fundam. Theor. Phys. 183
Original
2016
Cited alongside, same era.
S. Alam et al. (BOSS), The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, Mon. Not. Roy. Astron. Soc. 470
Original
2017
Cited alongside, same era.
R. S. Park et al. , Precession of Mercury’s Perihelion from Ranging to the MESSENGER Spacecraft, The Astronomical Journal 153
2017
Cited alongside, same era.
M. Zumalacárregui, E. Bellini, I. Sawicki, J. Lesgourgues, and P. G. Ferreira, hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System, J. Cosmology Astropart. Phys 2017
Original
2017
Cited alongside, same era.
F. G. Mohammad et al. , The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unbiased estimate of the growth rate of structure at ⟨ \langle z ⟩ \rangle = 0.85 using the clustering of luminous blue galaxies, Astron. Astrophys. 610

Then

D. Wang, The Self-Consistency of DESI Analysis and Comment on ”Does DESI 2024 Confirm Λ \Lambda CDM?”, (2024), arXiv:2404.13833 [astro-ph.CO]
Original
2024
Later among the works it cites.
B. R. Dinda, A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data, (2024), arXiv:2405.06618 [astro-ph.CO]
Original
2024
Later among the works it cites.
C.-G. Park, J. de Cruz Pérez, and B. Ratra, Using non-DESI data to confirm and strengthen the DESI 2024 spatially flat w0waCDM cosmological parametrization result, Phys. Rev. D 110
Original
2024
Later among the works it cites.
J.-Q. Jiang, D. Pedrotti, S. S. da Costa, and S. Vagnozzi, Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data, Phys. Rev. D 110
Original
2024
Later among the works it cites.

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alphaXiv searches the wider corpus for related work and actual follow-ups.

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Reading the bibliography…

2025

Assessing cosmological evidence for non-minimal coupling

Wolf, William J., García-García, Carlos, Anton, Theodore et al.

Understand

The recent observational evidence of deviations from the $\Lambda$-Cold Dark Matter ($\Lambda$CDM) model points towards the presence of evolving dark energy.

The simplest possibility consists of a cosmological scalar field $\varphi$, dubbed quintessence, driving the accelerated expansion.
We assess the evidence for the existence of such a scalar field.
We find that, if the accelerated expansion is driven by quintessence, the data favour a potential energy $V(\varphi)$ that is concave, i.e., $m^2=d^2V/d\varphi^2<0$.

Built on

T. Kobayashi, Horndeski theory and beyond: a review, Rept. Prog. Phys. 82
Original
1901
Earlier work this paper cites.
C. Dalang and L. Lombriser, Limitations on Standard Sirens tests of gravity from screening, JCAP 10
Original
1906
Earlier work this paper cites.
N. Aghanim et al. (Planck), Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
E. Bellini, I. Sawicki, and M. Zumalacárregui, hi_class background evolution, initial conditions and approximation schemes, J. Cosmology Astropart. Phys 2020
Original
1909
Earlier work this paper cites.
W. J. Wolf and M. Lagos, Standard Sirens as a Novel Probe of Dark Energy, Phys. Rev. Lett. 124
Original
1910
Earlier work this paper cites.
C. García-García, E. Bellini, P. G. Ferreira, D. Traykova, and M. Zumalacárregui, Theoretical priors in scalar-tensor cosmologies: Thawing quintessence, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
H. Jeffreys, The Theory of Probability , 1st ed., Oxford Classic Texts in the Physical Sciences (Oxford University Press, Oxford, 1939)
1939
Earlier work this paper cites.
C. G. Callan, Jr., S. R. Coleman, and R. Jackiw, A New improved energy - momentum tensor, Annals Phys. 59
1970
Earlier work this paper cites.
A. I. Vainshtein, To the problem of nonvanishing gravitation mass, Phys. Lett. B 39
1972
Earlier work this paper cites.
N. D. Birrell and P. C. W. Davies, Quantum Fields in Curved Space , Cambridge Monographs on Mathematical Physics (Cambridge University Press, 1982)
1982
Earlier work this paper cites.
M. S. Madsen, Scalar Fields in Curved Space-times, Class. Quant. Grav. 5
1988
Earlier work this paper cites.
I. L. Buchbinder, Effective Action in Quantum Gravity , 1st ed. (Routledge, 1992)
1992
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.
G. Esposito-Farese and D. Polarski, Scalar tensor gravity in an accelerating universe, Phys. Rev. D 63
2001
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.
M. Lagos and H. Zhu, Gravitational couplings in Chameleon models, JCAP 06
Original
2003
Earlier work this paper cites.
E. G. Adelberger, B. R. Heckel, and A. E. Nelson, Tests of the gravitational inverse-square law, Ann. Rev. Nuc. & Part. Sci. 53
2003
Earlier work this paper cites.
B. Bertotti, L. Iess, and P. Tortora, A test of General Relativity using radio links with the Cassini spacecraft, Nature 425
2003
Earlier work this paper cites.
J. Khoury and A. Weltman, Chameleon cosmology, Phys. Rev. D 69
2004
Earlier work this paper cites.
A. Gómez-Valent, V. Pettorino, and L. Amendola, Update on coupled dark energy and the H 0 H_{0} tension, Phys. Rev. D 101
Original
2004
Earlier work this paper cites.
J. Torrado and A. Lewis, Cobaya: Code for Bayesian Analysis of hierarchical physical models, JCAP 05
Original
2005
Earlier work this paper cites.
S. Räsänen, Accelerated expansion from structure formation, Journal of Cosmology and Astroparticle Physics 2006
2006
Earlier work this paper cites.
R. Trotta, Applications of Bayesian model selection to cosmological parameters, Mon. Not. Roy. Astron. Soc. 378
2007
Earlier work this paper cites.
S. Alam et al. (eBOSS), 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
Original
2007
Earlier work this paper cites.
S. Dutta and R. J. Scherrer, Hilltop Quintessence, Phys. Rev. D 78
Original
2008
Earlier work this paper cites.
N. J. Secrest, S. von Hausegger, M. Rameez, R. Mohayaee, S. Sarkar, and J. Colin, A Test of the Cosmological Principle with Quasars, Astrophys. J. Lett. 908
Original
2009
Earlier work this paper cites.
M. Park, K. M. Zurek, and S. Watson, A Unified Approach to Cosmic Acceleration, Phys. Rev. D 81
Original
2010
Earlier work this paper cites.
A. Heinesen, Multipole decomposition of the general luminosity distance Hubble law—a new framework for observational cosmology, Journal of Cosmology and Astroparticle Physics 2021
Original
2010
Earlier work this paper cites.
S. Nojiri and S. D. Odintsov, Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models, Phys. Rept. 505
Original
2011
Earlier work this paper cites.
D. Blas, J. Lesgourgues, and T. Tram, The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes, J. Cosmology Astropart. Phys 2011
Original
2011
Earlier work this paper cites.
F. Beutler, C. Blake, M. Colless, D. H. Jones, L. Staveley-Smith, G. B. Poole, L. Campbell, Q. Parker, W. Saunders, and F. Watson, The 6dF Galaxy Survey: z ≈ \approx 0 measurements of the growth rate and σ \sigma 8
Original
2012
Earlier work this paper cites.
C. Blake, S. Brough, M. Colless, C. Contreras, W. Couch, S. Croom, D. Croton, T. M. Davis, M. J. Drinkwater, K. Forster, D. Gilbank, M. Gladders, K. Glazebrook, B. Jelliffe, R. J. Jurek, I. h. Li, B. Madore, D. C. Martin, K. Pimbblet, G. B. Poole, M. Pracy, R. Sharp, E. Wisnioski, D. Woods, T. K. Wyder, and H. K. C. Yee, The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z ¡ 1, MNRAS 425
Original
2012
Earlier work this paper cites.
D. E. Smith et al. , Gravity Field and Internal Structure of Mercury from MESSENGER, Science 336
2012
Earlier work this paper cites.
T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified Gravity and Cosmology, Phys. Rept. 513
Original
2012
Earlier work this paper cites.
T. Buchert and S. Räsänen, Backreaction in Late-Time Cosmology, Annual Review of Nuclear and Particle Science 62
Original
2012
Earlier work this paper cites.
C. M. Will, The Confrontation between General Relativity and Experiment, Living Rev. Rel. 17
Original
2014
Earlier work this paper cites.
W. J. Handley, M. P. Hobson, and A. N. Lasenby, PolyChord: nested sampling for cosmology, Mon. Not. Roy. Astron. Soc. 450
Original
2015
Earlier work this paper cites.
T. Buchert et al. , Is there proof that backreaction of inhomogeneities is irrelevant in cosmology?, Classical and Quantum Gravity 32
Original
2015
Earlier work this paper cites.
T. Okumura et al. , The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at z ∼ 1.4 z\sim 1.4 , Publ. Astron. Soc. Jap. 68
Original
2016
Earlier work this paper cites.

Similar

D. I. Kaiser, Nonminimal Couplings in the Early Universe: Multifield Models of Inflation and the Latest Observations, Fundam. Theor. Phys. 183
Original
2016
Cited alongside, same era.
S. Alam et al. (BOSS), The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, Mon. Not. Roy. Astron. Soc. 470
Original
2017
Cited alongside, same era.
R. S. Park et al. , Precession of Mercury’s Perihelion from Ranging to the MESSENGER Spacecraft, The Astronomical Journal 153
2017
Cited alongside, same era.
M. Zumalacárregui, E. Bellini, I. Sawicki, J. Lesgourgues, and P. G. Ferreira, hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System, J. Cosmology Astropart. Phys 2017
Original
2017
Cited alongside, same era.
F. G. Mohammad et al. , The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unbiased estimate of the growth rate of structure at ⟨ \langle z ⟩ \rangle = 0.85 using the clustering of luminous blue galaxies, Astron. Astrophys. 610

Then

D. Wang, The Self-Consistency of DESI Analysis and Comment on ”Does DESI 2024 Confirm Λ \Lambda CDM?”, (2024), arXiv:2404.13833 [astro-ph.CO]
Original
2024
Later among the works it cites.
B. R. Dinda, A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data, (2024), arXiv:2405.06618 [astro-ph.CO]
Original
2024
Later among the works it cites.
C.-G. Park, J. de Cruz Pérez, and B. Ratra, Using non-DESI data to confirm and strengthen the DESI 2024 spatially flat w0waCDM cosmological parametrization result, Phys. Rev. D 110
Original
2024
Later among the works it cites.
J.-Q. Jiang, D. Pedrotti, S. S. da Costa, and S. Vagnozzi, Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data, Phys. Rev. D 110
Original
2024
Later among the works it cites.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

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alphaXiv is searching for related work…

Original

2018

Cited alongside, same era.

J. Sakstein, Tests of Gravity with Future Space-Based Experiments, Phys. Rev. D 97

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2018

Cited alongside, same era.

N. Aghanim et al. (Planck), Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641

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2021

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D. Traykova, E. Bellini, P. G. Ferreira, C. García-García, J. Noller, and M. Zumalacárregui, Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models, Phys. Rev. D 104

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2021

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2021

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P. Brax, S. Casas, H. Desmond, and B. Elder, Testing Screened Modified Gravity, Universe 8

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2021

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D. Scolnic et al. , The Pantheon+ Analysis: The Full Data Set and Light-curve Release, Astrophys. J. 938

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2022

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2022

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K. Lodha et al. , Extended Dark Energy analysis using DESI DR2 BAO measurements, (2025), arXiv:2503.14743 [astro-ph.CO]

Original

2025

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R. E. Keeley, K. N. Abazajian, M. Kaplinghat, and A. Shafieloo, The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations, (2025), arXiv:2502.12667 [astro-ph.CO]

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2025

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D. Shlivko, P. J. Steinhardt, and C. L. Steinhardt, Optimal parameterizations for observational constraints on thawing dark energy, (2025), arXiv:2504.02028 [astro-ph.CO]

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2025

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P. G. Ferreira, W. J. Wolf, and J. Read, The Spectre of Underdetermination in Modern Cosmology, (2025), arXiv:2501.06095 [physics.hist-ph]

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2025

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G. Borghetto, A. Malhotra, G. Tasinato, and I. Zavala, Bounded Dark Energy, (2025), arXiv:2503.11628 [astro-ph.CO]

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2025

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H. N. Luu, Y.-C. Qiu, and S. H. H. Tye, Dynamical dark energy from an ultralight axion, (2025), arXiv:2503.18120 [hep-ph]

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2025

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L. A. Ureña López et al. (DESI), Updated cosmological constraints on axion dark energy with DESI, (2025), arXiv:2503.20178 [astro-ph.CO]

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2025

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M. W. Hossain and A. Maqsood, Cosmological implications of Tracker scalar fields as dynamical dark energy, (2025), arXiv:2502.19274 [astro-ph.CO]

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2025

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M. Berti, E. Bellini, C. Bonvin, M. Kunz, M. Viel, and M. Zumalacarregui, Reconstructing the dark energy density in light of DESI BAO observations, (2025), arXiv:2503.13198 [astro-ph.CO]

Original

2025

Closest in time.

A. N. Ormondroyd, W. J. Handley, M. P. Hobson, and A. N. Lasenby, Nonparametric reconstructions of dynamical dark energy via flexknots, (2025), arXiv:2503.08658 [astro-ph.CO]

Original

2025

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E. Moghtaderi, B. R. Hull, J. Quintin, and G. Geshnizjani, How Much NEC Breaking Can the Universe Endure?, (2025), arXiv:2503.19955 [gr-qc]

Original

2025

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G. Ye and Y. Cai, NEC violation and ”beyond Horndeski” physics in light of DESI DR2, (2025), arXiv:2503.22515 [gr-qc]

Original

2025

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A. G. Ferrari, M. Ballardini, F. Finelli, and D. Paoletti, Scalar-Tensor Gravity and DESI 2024 BAO data, (2025), arXiv:2501.15298 [astro-ph.CO]

Original

2025

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A. Chudaykin, M. Kunz, and J. Carron, Modified gravity constraints with Planck ISW-lensing bispectrum, (2025), arXiv:2503.09893 [astro-ph.CO]

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2025

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J. Pan and G. Ye, Non-minimally coupled gravity constraints from DESI DR2 data, (2025), arXiv:2503.19898 [astro-ph.CO]

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2025

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U. Andrade et al. , Validation of the DESI DR2 Measurements of Baryon Acoustic Oscillations from Galaxies and Quasars, (2025), arXiv:2503.14742 [astro-ph.CO]

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2025

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T. M. C. Abbott et al. (DES), Dark Energy Survey: implications for cosmological expansion models from the final DES Baryon Acoustic Oscillation and Supernova data, (2025), arXiv:2503.06712 [astro-ph.CO]

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2025

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C. Briddon, T. Clifton, and P. Fleury, Emergent cosmological expansion in scalar–tensor theories of gravity, Class. Quant. Grav. 42

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T. Anton, P. G. Ferreira, C. García-García, and W. J. Wolf, Constructing observationally viable quintessence across cosmological and astrophysical scales, In prep. (2025)

2025

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A. Chakraborty, P. K. Chanda, S. Das, and K. Dutta, DESI results: Hint towards coupled dark matter and dark energy, (2025), arXiv:2503.10806 [astro-ph.CO]

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R. Shah, P. Mukherjee, and S. Pal, Interacting dark sectors in light of DESI DR2, (2025), arXiv:2503.21652 [astro-ph.CO]

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E. Silva, M. A. Sabogal, M. S. Souza, R. C. Nunes, E. Di Valentino, and S. Kumar, New Constraints on Interacting Dark Energy from DESI DR2 BAO Observations, (2025), arXiv:2503.23225 [astro-ph.CO]

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