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2020

Sources of $H_0$-tensions in dark energy scenarios

Haridasu, Balakrishna S., Viel, Matteo, Vittorio, Nicola

Understand

By focusing on the simple $w\neq-1$ extension to $\Lambda$CDM, we assess which epoch(s) possibly source the $H_0$-tension.

We consider Cosmic Microwave Background (CMB) data in three possible ways: $i)$ complete CMB data; $ii)$ excluding the $l<30$ temperature and polarization likelihoods; $iii)$ imposing early universe priors, that disentangle early and late time physics.
Through a joint analysis with low-redshift supernovae type-Ia and gravitationally lensed time delay datasets, {and neglecting galaxy clustering Baryonic Acoustic Oscillation (BAO) data}, we find that the inclusion of early universe CMB priors is consistent with the local estimate of $H_0$ while excluding the low-$l$+lowE likelihoods mildly relaxes the tension.
This is in contrast to joint analyses with the complete CMB data.

Built on

W. D. Kenworthy and D. Scolnic and A. Riess, arXiv e-prints , arXiv:1901.08681 (2019), arXiv:1901.08681 [astro-ph.CO]
Original
1901
Earlier work this paper cites.
M. Billi, A. Gruppuso, and N. Mandolesi, and L. Moscardini, and P. Natoli, Physics of the Dark Universe 26
Original
1901
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M. Raveri, Phys. Rev. D 101
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1902
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K. Vattis and S. M. Koushiappas and A. Loeb, arXiv e-prints , arXiv:1903.06220 (2019), arXiv:1903.06220 [astro-ph.CO]
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1903
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P. Agrawal, and F.-Y. Cyr-Racine, and D. Pinner, and L. Randall, (2019), arXiv:1904.01016 [astro-ph.CO]
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1904
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M. Blomqvist and H. du Mas des Bourboux et al. , arXiv e-prints (2019) , arXiv:1904.03430
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1904
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V. de Sainte Agathe and C. Balland et al. , arXiv e-prints (2019) , arXiv:1904.03400
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1904
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M.-X. Lin, and G. Benevento, and W. Hu, and M. Raveri, Phys. Rev. D 100
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1905
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N. Arendse and A. Agnello and R. J. Wojtak, Astron. Astrophys. 632
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1905
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S. Taubenberger, S. H. Suyu, E. Komatsu, I. Jee, S. Birrer, V. Bonvin, F. Courbin, and C. E. Rusu, and A. J. Shajib, and K. C. Wong, Astron. Astrophys. 628
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1905
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1907
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Original
1907
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M. Archidiacono, D. C. Hooper, R. Murgia, and S. Bohr, and J. Lesgourgues, and M. Viel, JCAP 1910
Original
1907
Earlier work this paper cites.
N. Schöneberg and J. Lesgourgues and D. C. Hooper, J. Cosmology Astropart. Phys. 2019
Original
1907
Earlier work this paper cites.
Luković, and V. V. , and B. S. Haridasu, and N. Vittorio, Mon. Not. Roy. Astron. Soc. , 2671 (2019) , arXiv:1907.11219 [astro-ph.CO]
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1907
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S. Vagnozzi, arXiv e-prints , arXiv:1907.07569 (2019), arXiv:1907.07569 [astro-ph.CO]
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1907
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W. Handley, arXiv e-prints , arXiv:1908.09139 (2019), arXiv:1908.09139 [astro-ph.CO]
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1908
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M. M. Ivanov and M. Simonović and M. Zaldarriaga, (2019), arXiv:1909.05277 [astro-ph.CO]
Original
1909
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1910
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A. Lewis, arXiv e-prints , arXiv:1910.13970 (2019), arXiv:1910.13970 [astro-ph.IM]
Original
1910
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J. Sakstein and M. Trodden, Phys. Rev. Lett. 124
Original
1911
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E. Di Valentino and A. Melchiorri and J. Silk, Nat. Astron. (2019), 10.1038/s41550-019-0906-9 , arXiv:1911.02087 [astro-ph.CO]
Original
1911
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M. Millon et al. , Astron. Astrophys. 639
Original
1912
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Z. Zhai, and C.-G. Park, and Y. Wang, and B. Ratra, arXiv e-prints , arXiv:1912.04921 (2019), arXiv:1912.04921 [astro-ph.CO]
Original
1912
Earlier work this paper cites.
D. J. Fixsen, Astrophys. J. 707
Original
1955
Earlier work this paper cites.
A. Gelman and D. B. Rubin, Statist. Sci. 7
1992
Earlier work this paper cites.
W. Hu and N. Sugiyama, Astrophys. J. 471
1996
Earlier work this paper cites.
A. G. Riess, Nature Reviews Physics 2
Original
2001
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G. Ye and Y.-S. Piao, arXiv e-prints , arXiv:2001.02451 (2020), arXiv:2001.02451 [astro-ph.CO]
Original
2001
Earlier work this paper cites.
H. Khoraminezhad, and M. Viel, and C. Baccigalupi, and M. Archidiacono, JCAP 07
Original
2001
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M.-Z. Lyu, and B. S. Haridasu, and M. Viel, and J.-Q. Xia, Astrophys. J. 900
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2001
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A. Lewis and S. Bridle, Physical Review D 66
2002
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R. Jimenez and A. Loeb, Astrophys. J. 573
2002
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J. C. Hill, and E. McDonough, and M. W. Toomey, and S. Alexander, arXiv e-prints , arXiv:2003.07355 (2020), arXiv:2003.07355 [astro-ph.CO]
Original
2003
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B. S. Haridasu and M. Viel, Mon. Not. Roy. Astron. Soc. (2020), 10.1093/mnras/staa1991 , arXiv:2004.07709 [astro-ph.CO]
Original
2004
Earlier work this paper cites.
G. Alestas and L. Kazantzidis and L. Perivolaropoulos, Phys. Rev. D 101
Original
2004
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A. Chudaykin and D. Gorbunov and N. Nedelko, JCAP 08
Original
2004
Earlier work this paper cites.
A. Gogoi and P. Chanda and S. Das, (2020), arXiv:2005.11889 [astro-ph.CO]
Original
2005
Earlier work this paper cites.
D. J. Eisenstein et al. (SDSS), Astrophys. J. 633
2005
Earlier work this paper cites.

Similar

A. Hryczuk and K. Jodł owski, Phys. Rev. D 102
Original
2006
Cited alongside, same era.
S. J. Clark and K. Vattis and S. M. Koushiappas, (2020), arXiv:2006.03678 [astro-ph.CO]
Original
2006
Cited alongside, same era.
Y. Wang and P. Mukherjee, Astrophys. J. 650
2006
Cited alongside, same era.
M. M. Ivanov, E. McDonough, J. C. Hill, M. Simonović, and M. W. Toomey, and S. Alexand er, and M. Zaldarriaga, arXiv e-prints , arXiv:2006.11235 (2020), arXiv:2006.11235 [astro-ph.CO]
Original
2006
Cited alongside, same era.
G. D’Amico, and L. Senatore, and P. Zhang, and H. Zheng, (2020), arXiv:2006.12420 [astro-ph.CO]
Original
2006
Cited alongside, same era.

Then

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Original
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N. Aghanim et al. (Planck), Astron. Astrophys. 596
Original
2016
Later among the works it cites.
D. J. Schwarz, and C. J. Copi, and D. Huterer, and G. D. Starkman, Classical and Quantum Gravity 33
Original
2016
Later among the works it cites.

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