Built on

N. Aghanim et al. (Planck), Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 641
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1907
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X. Chen, F. Feroz, and M. Hobson, Bayesian posterior repartitioning for nested sampling (2022), arXiv:1908.04655 [stat.CO]
Original
1908
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A. Lewis, Getdist: a python package for analysing monte carlo samples (2019), arXiv:1910.13970 [astro-ph.IM]
Original
1910
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J. A. Frieman, C. T. Hill, A. Stebbins, and I. Waga, Cosmology with ultralight pseudo nambu-goldstone bosons, Physical Review Letters 75
1995
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K. Coble, S. Dodelson, and J. A. Frieman, Dynamical Lambda models of structure formation, Phys. Rev. D 55
1997
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P. T. P. Viana and A. R. Liddle, Perturbation evolution in cosmologies with a decaying cosmological constant, Phys. Rev. D 57
1998
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J. A. Frieman and I. Waga, Constraints from high redshift supernovae upon scalar field cosmologies, Phys. Rev. D 57
1998
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E. J. Copeland, A. R. Liddle, and D. Wands, Exponential potentials and cosmological scaling solutions, Phys. Rev. D57
1998
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I. Waga and J. A. Frieman, New constraints from high redshift supernovae and lensing statistics upon scalar field cosmologies, Physical Review D 62
2000
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M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter, Int. J. Mod. Phys. D 10
2001
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M. Kawasaki, T. Moroi, and T. Takahashi, Cosmic microwave background anisotropy with cosine type quintessence, Phys. Rev. D 64
2001
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S. C. C. Ng and D. L. Wiltshire, Properties of cosmologies with dynamical pseudo Nambu-Goldstone bosons, Phys. Rev. D 63
2001
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E. V. Linder, Exploring the expansion history of the universe, Phys. Rev. Lett. 90
2003
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J. Skilling, Nested Sampling, AIP Conf. Proc. 735
2004
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R. R. Caldwell and E. V. Linder, Limits of quintessence, Physical Review Letters 95
2005
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L. J. Hall, Y. Nomura, and S. J. Oliver, Evolving dark energy with w ≠ − 1 w\neq-1 , Phys. Rev. Lett. 95
2005
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J. Torrado and A. Lewis, Cobaya: Code for Bayesian Analysis of hierarchical physical models, JCAP 05
Original
2005
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L. Amendola and R. Barbieri, Dark matter from an ultra-light pseudo-Goldsone-boson, Phys. Lett. B 642
2006
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F. X. Linares Cedeño, A. X. González-Morales, and L. A. Ureña López, Ultralight DM bosons with an axion-like potential: scale-dependent constraints revisited, JCAP 01
Original
2006
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J. Skilling, Nested sampling for general Bayesian computation, Bayesian Analysis 1
2006
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K. Dutta and L. Sorbo, Confronting pseudo-nambu-goldstone-boson quintessence with data, Physical Review D 75
2007
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E. V. Linder, The Mirage of w=-1, arXiv e-prints (2007), arXiv:0708.0024 [astro-ph]
Original
2007
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A. Abrahamse, A. Albrecht, M. Barnard, and B. Bozek, Exploring parameter constraints on quintessential dark energy: The pseudo-Nambu-Goldstone-boson model, Phys. Rev. D 77
Original
2008
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R. Trotta, Bayes in the sky: Bayesian inference and model selection in cosmology, Contemp. Phys. 49
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2008
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A. Arvanitaki, S. Dimopoulos, S. Dubovsky, N. Kaloper, and J. March-Russell, String Axiverse, Phys. Rev. D 81
Original
2010
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T. Fujita, K. Murai, H. Nakatsuka, and S. Tsujikawa, Detection of isotropic cosmic birefringence and its implications for axionlike particles including dark energy, Phys. Rev. D 103
Original
2011
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M. Levi et al. , The DESI Experiment, a whitepaper for Snowmass 2013, arXiv e-prints , arXiv:1308.0847 (2013), arXiv:1308.0847 [astro-ph.CO]
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2013
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R. Hlozek, D. Grin, D. J. E. Marsh, and P. G. Ferreira, A search for ultralight axions using precision cosmological data, Phys. Rev. D91
Original
2015
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W. J. Handley, M. P. Hobson, and A. N. Lasenby, PolyChord: nested sampling for cosmology, Mon. Not. Roy. Astron. Soc. 450
Original
2015
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W. J. Handley, M. P. Hobson, and A. N. Lasenby, POLYCHORD: next-generation nested sampling, Mon. Not. Roy. Astron. Soc. 453
Original
2015
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E. V. Linder, Quintessence’s last stand?, Phys. Rev. D 91
Original
2015
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DESI Collaboration, A. Aghamousa, et al. , The DESI Experiment Part I: Science,Targeting, and Survey Design, arXiv e-prints , arXiv:1611.00036 (2016), arXiv:1611.00036 [astro-ph.IM]
Original
2016
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DESI Collaboration and A. o. Aghamousa, The DESI Experiment Part II: Instrument Design, arXiv e-prints , arXiv:1611.00037 (2016), arXiv:1611.00037 [astro-ph.IM]
Original
2016
Earlier work this paper cites.

Similar

L. A. Ureña López, New perturbative method for analytical solutions in single-field models of inflation, Phys. Rev. D94
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2016
Cited alongside, same era.
H. Zou et al. , Project Overview of the Beijing-Arizona Sky Survey, PASP 129
Original
2017
Cited alongside, same era.
V. Smer-Barreto and A. R. Liddle, Planck satellite constraints on pseudo-nambu-goldstone boson quintessence, Journal of Cosmology and Astroparticle Physics 2017
2017
Cited alongside, same era.
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2017
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F. X. L. Cedeño, A. X. González-Morales, and L. A. Ureña López, Cosmological signatures of ultralight dark matter with an axionlike potential, Phys. Rev. D 96

Then

DESI Collaboration, A. G. Adame, et al. , DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest, arXiv e-prints , arXiv:2404.03001 (2024e) , arXiv:2404.03001 [astro-ph.CO]
Original
2024
Later among the works it cites.
A. G. Adame et al. (DESI), DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars, arXiv e-prints (2024a), arXiv:2411.12021 [astro-ph.CO]
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2024
Later among the works it cites.
DESI Collaboration, A. G. Adame, et al. , DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations, arXiv e-prints , arXiv:2404.03002 (2024f) , arXiv:2404.03002 [astro-ph.CO]
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Later among the works it cites.
A. G. Adame et al. (DESI), DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements, arXiv e-prints (2024b), arXiv:2411.12022 [astro-ph.CO]
Original
2024
Later among the works it cites.

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2025

Updated cosmological constraints on axion dark energy with DESI

Ureña-López, L. A., Lozano-Rodríguez, F., Román-Herrera, J. O. et al.

Understand

We present updated constraints on the parameters of an axion dark energy model, for which we took into account the properties of its characteristic potential and its full cosmological evolution.

We show that the values of the axion parameters appear sufficiently constrained by the data, including the latest DESI DR1, and are consistent with the theoretical expectations of a field mass $m_a$ in the ultralight regime $\log (m_a c^2/~\mathrm{eV}) \simeq -32.60~\pm~0.12$, and an effective energy scale $f_a$ close to the reduced Planck energy $\log (f_a/~ M_\mathrm{Pl}) \simeq -0.28~\pm~0.19$.
Our results also support the idea of dynamical dark energy, although Bayesian evidence still favors the phenomenological dark energy model $w_0w_a$ over the axion dark energy, with the Bayes factor indicating moderate and weak strength of the evidence, respectively, when the models are compared to the cosmological constant $\Lambda$.
However, the results suggest that axion dark energy remains a well-motivated model and its parameters may be better constrained if the upcoming DESI data show further evidence for dynamical dark energy.

Built on

N. Aghanim et al. (Planck), Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
X. Chen, F. Feroz, and M. Hobson, Bayesian posterior repartitioning for nested sampling (2022), arXiv:1908.04655 [stat.CO]
Original
1908
Earlier work this paper cites.
A. Lewis, Getdist: a python package for analysing monte carlo samples (2019), arXiv:1910.13970 [astro-ph.IM]
Original
1910
Earlier work this paper cites.
J. A. Frieman, C. T. Hill, A. Stebbins, and I. Waga, Cosmology with ultralight pseudo nambu-goldstone bosons, Physical Review Letters 75
1995
Earlier work this paper cites.
K. Coble, S. Dodelson, and J. A. Frieman, Dynamical Lambda models of structure formation, Phys. Rev. D 55
1997
Earlier work this paper cites.
P. T. P. Viana and A. R. Liddle, Perturbation evolution in cosmologies with a decaying cosmological constant, Phys. Rev. D 57
1998
Earlier work this paper cites.
J. A. Frieman and I. Waga, Constraints from high redshift supernovae upon scalar field cosmologies, Phys. Rev. D 57
1998
Earlier work this paper cites.
E. J. Copeland, A. R. Liddle, and D. Wands, Exponential potentials and cosmological scaling solutions, Phys. Rev. D57
1998
Earlier work this paper cites.
I. Waga and J. A. Frieman, New constraints from high redshift supernovae and lensing statistics upon scalar field cosmologies, Physical Review 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.
M. Kawasaki, T. Moroi, and T. Takahashi, Cosmic microwave background anisotropy with cosine type quintessence, Phys. Rev. D 64
2001
Earlier work this paper cites.
S. C. C. Ng and D. L. Wiltshire, Properties of cosmologies with dynamical pseudo Nambu-Goldstone bosons, 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.
J. Skilling, Nested Sampling, AIP Conf. Proc. 735
2004
Earlier work this paper cites.
R. R. Caldwell and E. V. Linder, Limits of quintessence, Physical Review Letters 95
2005
Earlier work this paper cites.
L. J. Hall, Y. Nomura, and S. J. Oliver, Evolving dark energy with w ≠ − 1 w\neq-1 , Phys. Rev. Lett. 95
2005
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.
L. Amendola and R. Barbieri, Dark matter from an ultra-light pseudo-Goldsone-boson, Phys. Lett. B 642
2006
Earlier work this paper cites.
F. X. Linares Cedeño, A. X. González-Morales, and L. A. Ureña López, Ultralight DM bosons with an axion-like potential: scale-dependent constraints revisited, JCAP 01
Original
2006
Earlier work this paper cites.
J. Skilling, Nested sampling for general Bayesian computation, Bayesian Analysis 1
2006
Earlier work this paper cites.
K. Dutta and L. Sorbo, Confronting pseudo-nambu-goldstone-boson quintessence with data, Physical Review D 75
2007
Earlier work this paper cites.
E. V. Linder, The Mirage of w=-1, arXiv e-prints (2007), arXiv:0708.0024 [astro-ph]
Original
2007
Earlier work this paper cites.
A. Abrahamse, A. Albrecht, M. Barnard, and B. Bozek, Exploring parameter constraints on quintessential dark energy: The pseudo-Nambu-Goldstone-boson model, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.
R. Trotta, Bayes in the sky: Bayesian inference and model selection in cosmology, Contemp. Phys. 49
Original
2008
Earlier work this paper cites.
A. Arvanitaki, S. Dimopoulos, S. Dubovsky, N. Kaloper, and J. March-Russell, String Axiverse, Phys. Rev. D 81
Original
2010
Earlier work this paper cites.
T. Fujita, K. Murai, H. Nakatsuka, and S. Tsujikawa, Detection of isotropic cosmic birefringence and its implications for axionlike particles including dark energy, Phys. Rev. D 103
Original
2011
Earlier work this paper cites.
M. Levi et al. , The DESI Experiment, a whitepaper for Snowmass 2013, arXiv e-prints , arXiv:1308.0847 (2013), arXiv:1308.0847 [astro-ph.CO]
Original
2013
Earlier work this paper cites.
R. Hlozek, D. Grin, D. J. E. Marsh, and P. G. Ferreira, A search for ultralight axions using precision cosmological data, Phys. Rev. D91
Original
2015
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.
W. J. Handley, M. P. Hobson, and A. N. Lasenby, POLYCHORD: next-generation nested sampling, Mon. Not. Roy. Astron. Soc. 453
Original
2015
Earlier work this paper cites.
E. V. Linder, Quintessence’s last stand?, Phys. Rev. D 91
Original
2015
Earlier work this paper cites.
DESI Collaboration, A. Aghamousa, et al. , The DESI Experiment Part I: Science,Targeting, and Survey Design, arXiv e-prints , arXiv:1611.00036 (2016), arXiv:1611.00036 [astro-ph.IM]
Original
2016
Earlier work this paper cites.
DESI Collaboration and A. o. Aghamousa, The DESI Experiment Part II: Instrument Design, arXiv e-prints , arXiv:1611.00037 (2016), arXiv:1611.00037 [astro-ph.IM]
Original
2016
Earlier work this paper cites.

Similar

L. A. Ureña López, New perturbative method for analytical solutions in single-field models of inflation, Phys. Rev. D94
Original
2016
Cited alongside, same era.
H. Zou et al. , Project Overview of the Beijing-Arizona Sky Survey, PASP 129
Original
2017
Cited alongside, same era.
V. Smer-Barreto and A. R. Liddle, Planck satellite constraints on pseudo-nambu-goldstone boson quintessence, Journal of Cosmology and Astroparticle Physics 2017
2017
Cited alongside, same era.
L. Hui, J. P. Ostriker, S. Tremaine, and E. Witten, Ultralight scalars as cosmological dark matter, Phys. Rev. D 95
Original
2017
Cited alongside, same era.
F. X. L. Cedeño, A. X. González-Morales, and L. A. Ureña López, Cosmological signatures of ultralight dark matter with an axionlike potential, Phys. Rev. D 96

Then

DESI Collaboration, A. G. Adame, et al. , DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest, arXiv e-prints , arXiv:2404.03001 (2024e) , arXiv:2404.03001 [astro-ph.CO]
Original
2024
Later among the works it cites.
A. G. Adame et al. (DESI), DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars, arXiv e-prints (2024a), arXiv:2411.12021 [astro-ph.CO]
Original
2024
Later among the works it cites.
DESI Collaboration, A. G. Adame, et al. , DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations, arXiv e-prints , arXiv:2404.03002 (2024f) , arXiv:2404.03002 [astro-ph.CO]
Original
2024
Later among the works it cites.
A. G. Adame et al. (DESI), DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements, arXiv e-prints (2024b), arXiv:2411.12022 [astro-ph.CO]
Original
2024
Later among the works it cites.

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

Original

2017

Cited alongside, same era.

H.-Y. Schive and T. Chiueh, Halo Abundance and Assembly History with Extreme-Axion Wave Dark Matter at z ≥ 4 z\geq 4 , MNRAS (2017), arXiv:1706.03723 [astro-ph.CO]

Original

2017

Cited alongside, same era.

L. Visinelli, Light Axion-Like Dark Matter must have Anthropic Origins, (2017), arXiv:1703.08798 [astro-ph.CO]

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2017

Cited alongside, same era.

N. Roy, A. X. Gonzalez-Morales, and L. A. Urena-Lopez, New general parametrization of quintessence fields and its observational constraints, Phys. Rev. D 98

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2018

Cited alongside, same era.

A. Dey et al. , Overview of the DESI Legacy Imaging Surveys, AJ 157

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2019

Cited alongside, same era.

L. A. Ureña López, Brief Review on Scalar Field Dark Matter Models, Front. Astron. Space Sci. 6

2019

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K.-H. Leong, H.-Y. Schive, U.-H. Zhang, and T. Chiueh, Testing extreme-axion wave-like dark matter using the BOSS Lyman-alpha forest data, Mon. Not. Roy. Astron. Soc. 484

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Original

2024