Built on

A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond Λ \Lambda CDM, Astrophys. J. 876
Original
1903
Earlier work this paper cites.
Schöneberg, Nils and Lesgourgues, Julien and Hooper, Deanna C., The BAO+BBN take on the Hubble tension, (2019), arXiv:1907.11594 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
K. C. Wong et al. , H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3 σ \sigma tension between early- and late-Universe probes, Mon. Not. Roy. Astron. Soc. 498
Original
1907
Earlier work this paper cites.
A. Kogut, M. Abitbol, J. Chluba, J. Delabrouille, D. Fixsen, J. Hill, S. Patil, and A. Rotti, CMB Spectral Distortions: Status and Prospects, (2019), arXiv:1907.13195 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin, Oscillating scalar fields and the Hubble tension: a resolution with novel signatures, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, O. Mena, and S. Vagnozzi, Interacting dark energy in the early 2020s: A promising solution to the H 0 H_{0} and cosmic shear tensions, Phys. Dark Univ. 30
Original
1908
Earlier work this paper cites.
J. Chluba et al. , New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background, (2019), arXiv:1909.01593 [astro-ph.CO]
Original
1909
Earlier work this paper cites.
M. Lucca, N. Schöneberg, D. C. Hooper, J. Lesgourgues, and J. Chluba, The synergy between CMB spectral distortions and anisotropies, (2019), 1910.04619
Original
1910
Earlier work this paper cites.
C.-P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges, Astrophys. J. 455
1995
Earlier work this paper cites.
R. E. Kass and A. E. Raftery, Bayes factors, Journal of the American Statistical Association 90
1995
Earlier work this paper cites.
J. Lima, Thermodynamics of decaying vacuum cosmologies, Phys. Rev. D 54
1996
Earlier work this paper cites.
W. Hu and M. J. White, The Damping tail of CMB anisotropies, Astrophys. J. 479
1997
Earlier work this paper cites.
S. Seager, D. D. Sasselov, and D. Scott, A new calculation of the recombination epoch, Astrophys. J. 523
1999
Earlier work this paper cites.
J. Lima, A. Silva, and S. Viegas, Is the radiation temperature redshift relation of the standard cosmology in accordance with the data?, Mon. Not. Roy. Astron. Soc. 312
2000
Earlier work this paper cites.
S. Seager, D. D. Sasselov, and D. Scott, How exactly did the universe become neutral?, The Astrophysical Journal Supplement Series 128
2000
Earlier work this paper cites.
C. Krishnan, E. O. Colgáin, Ruchika, A. A. Sen, M. Sheikh-Jabbari, and T. Yang, Is there an early Universe solution to Hubble tension?, Phys. Rev. D 102
Original
2002
Earlier work this paper cites.
M. Lucca and D. C. Hooper, Shedding light on dark matter-dark energy interactions, Phys. Rev. D 102
Original
2002
Earlier work this paper cites.
G. Benevento, W. Hu, and M. Raveri, Can Late Dark Energy Transitions Raise the Hubble constant?, Phys. Rev. D 101
Original
2002
Earlier work this paper cites.
J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, Early Dark Energy Does Not Restore Cosmological Concordance, (2020), arXiv:2003.07355 [astro-ph.CO]
Original
2003
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.

Similar

R. Bean and O. Dore, Probing dark energy perturbations: The Dark energy equation of state and speed of sound as measured by WMAP, Phys. Rev. D 69
2004
Cited alongside, same era.
V. Mukhanov, Physical Foundations of Cosmology (Cambridge University Press, Oxford, 2005)
2005
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F. Niedermann and M. S. Sloth, Resolving the Hubble tension with new early dark energy, Phys. Rev. D 102
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2008
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Original

Then

E. Di Valentino, A. Melchiorri, and O. Mena, Can interacting dark energy solve the H 0 H_{0} tension?, Phys. Rev. D96
Original
2017
Later among the works it cites.
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
Later among the works it cites.
A. Heavens, Y. Fantaye, A. Mootoovaloo, H. Eggers, Z. Hosenie, S. Kroon, and E. Sellentin, Marginal Likelihoods from Monte Carlo Markov Chains, (2017), arXiv:1704.03472 [stat.CO]
Original
2017
Later among the works it cites.
M. A. Troxel et al. (DES), Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear, Phys. Rev. D 98
Original
2018
Later among the works it cites.

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2021

Multi-interacting dark energy and its cosmological implications

Lucca, Matteo

Understand

In the effort to define the main features a successful solution to the Hubble tension should have, growing evidence has emerged pointing to the need for models able to modify the expansion (and possibly thermal) history of the universe both prior and after recombination, and that could thereby restore the overall concordance between early- and late-time observations without introducing nor worsening other cosmological tensions in the process.

In precisely this spirit, here we consider a multi-interacting dark energy model with two complementary interaction channels: one with the dark matter and one with the photons.
The former most significantly affects the matter dominated epoch as well as the very late universe, and has been shown to be able to significantly resolve the $S_8$ tension.
The latter has been introduced in this work to allow for a larger and natural time dependence of the evolution of the universe since it mostly impacts the radiation dominated epoch as well as the temperature scaling of the photons, as extensively explained in the text.

Built on

A. G. Riess, S. Casertano, W. Yuan, L. M. Macri, and D. Scolnic, Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond Λ \Lambda CDM, Astrophys. J. 876
Original
1903
Earlier work this paper cites.
Schöneberg, Nils and Lesgourgues, Julien and Hooper, Deanna C., The BAO+BBN take on the Hubble tension, (2019), arXiv:1907.11594 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
K. C. Wong et al. , H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3 σ \sigma tension between early- and late-Universe probes, Mon. Not. Roy. Astron. Soc. 498
Original
1907
Earlier work this paper cites.
A. Kogut, M. Abitbol, J. Chluba, J. Delabrouille, D. Fixsen, J. Hill, S. Patil, and A. Rotti, CMB Spectral Distortions: Status and Prospects, (2019), arXiv:1907.13195 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin, Oscillating scalar fields and the Hubble tension: a resolution with novel signatures, Phys. Rev. D 101
Original
1908
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, O. Mena, and S. Vagnozzi, Interacting dark energy in the early 2020s: A promising solution to the H 0 H_{0} and cosmic shear tensions, Phys. Dark Univ. 30
Original
1908
Earlier work this paper cites.
J. Chluba et al. , New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background, (2019), arXiv:1909.01593 [astro-ph.CO]
Original
1909
Earlier work this paper cites.
M. Lucca, N. Schöneberg, D. C. Hooper, J. Lesgourgues, and J. Chluba, The synergy between CMB spectral distortions and anisotropies, (2019), 1910.04619
Original
1910
Earlier work this paper cites.
C.-P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges, Astrophys. J. 455
1995
Earlier work this paper cites.
R. E. Kass and A. E. Raftery, Bayes factors, Journal of the American Statistical Association 90
1995
Earlier work this paper cites.
J. Lima, Thermodynamics of decaying vacuum cosmologies, Phys. Rev. D 54
1996
Earlier work this paper cites.
W. Hu and M. J. White, The Damping tail of CMB anisotropies, Astrophys. J. 479
1997
Earlier work this paper cites.
S. Seager, D. D. Sasselov, and D. Scott, A new calculation of the recombination epoch, Astrophys. J. 523
1999
Earlier work this paper cites.
J. Lima, A. Silva, and S. Viegas, Is the radiation temperature redshift relation of the standard cosmology in accordance with the data?, Mon. Not. Roy. Astron. Soc. 312
2000
Earlier work this paper cites.
S. Seager, D. D. Sasselov, and D. Scott, How exactly did the universe become neutral?, The Astrophysical Journal Supplement Series 128
2000
Earlier work this paper cites.
C. Krishnan, E. O. Colgáin, Ruchika, A. A. Sen, M. Sheikh-Jabbari, and T. Yang, Is there an early Universe solution to Hubble tension?, Phys. Rev. D 102
Original
2002
Earlier work this paper cites.
M. Lucca and D. C. Hooper, Shedding light on dark matter-dark energy interactions, Phys. Rev. D 102
Original
2002
Earlier work this paper cites.
G. Benevento, W. Hu, and M. Raveri, Can Late Dark Energy Transitions Raise the Hubble constant?, Phys. Rev. D 101
Original
2002
Earlier work this paper cites.
J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, Early Dark Energy Does Not Restore Cosmological Concordance, (2020), arXiv:2003.07355 [astro-ph.CO]
Original
2003
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.

Similar

R. Bean and O. Dore, Probing dark energy perturbations: The Dark energy equation of state and speed of sound as measured by WMAP, Phys. Rev. D 69
2004
Cited alongside, same era.
V. Mukhanov, Physical Foundations of Cosmology (Cambridge University Press, Oxford, 2005)
2005
Cited alongside, same era.
F. Niedermann and M. S. Sloth, Resolving the Hubble tension with new early dark energy, Phys. Rev. D 102
Original
2006
Cited alongside, same era.
E. Di Valentino et al. , Cosmology Intertwined II: The Hubble Constant Tension, (2020a), arXiv:2008.11284 [astro-ph.CO]
Original
2008
Cited alongside, same era.
E. Di Valentino et al. , Cosmology Intertwined III: f σ 8 f\sigma_{8} and S 8 S_{8} , (2020b), arXiv:2008.11285 [astro-ph.CO]
Original

Then

E. Di Valentino, A. Melchiorri, and O. Mena, Can interacting dark energy solve the H 0 H_{0} tension?, Phys. Rev. D96
Original
2017
Later among the works it cites.
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
Later among the works it cites.
A. Heavens, Y. Fantaye, A. Mootoovaloo, H. Eggers, Z. Hosenie, S. Kroon, and E. Sellentin, Marginal Likelihoods from Monte Carlo Markov Chains, (2017), arXiv:1704.03472 [stat.CO]
Original
2017
Later among the works it cites.
M. A. Troxel et al. (DES), Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear, Phys. Rev. D 98
Original
2018
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…

2008

Cited alongside, same era.

J. Väliviita, E. Majerotto, and R. Maartens, Large-scale instability in interacting dark energy and dark matter fluids, JCAP 2008

2008

Cited alongside, same era.

D. Scott and A. Moss, Matter temperature during cosmological recombination, MNRAS 397