Built on

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1995
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C.-P. Ma and E. Bertschinger, Astrophys. J. 455
1995
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W. Hu and N. Sugiyama, Astrophys. J. 471
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A. G. Riess et al. (Supernova Search Team), Astron. J. 116
1998
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W. Hu and D. J. Eisenstein, Astrophys. J. 498
1998
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S. Perlmutter et al. (Supernova Cosmology Project), Astrophys. J. 517
1999
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A. Lewis, A. Challinor, and A. Lasenby, Astrophys. J. 538
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R. Caldwell, A. Cooray, and A. Melchiorri, Phys. Rev. D76
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W. Hu and I. Sawicki, Phys. Rev. D76
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L. Amendola, M. Kunz, and D. Sapone, JCAP 0804
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E. Bertschinger and P. Zukin, Phys. Rev. D78
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L. Hui and K. P. Parfrey, Phys. Rev. D77
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A. Silvestri and M. Trodden, Rept. Prog. Phys. 72
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L. Pogosian, A. Silvestri, K. Koyama, and G.-B. Zhao, Phys. Rev. D81
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A. Hojjati, L. Pogosian, and G.-B. Zhao, JCAP 1108
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2018

Phenomenology of Modified Gravity at Recombination

Lin, Meng-Xiang, Raveri, Marco, Hu, Wayne

Understand

We discuss the phenomenological imprints of modifications to gravity in the early universe with a specific focus on the time of recombination.

We derive several interesting results regarding the effect that such modifications have on cosmological observables, especially on the driving and phasing of acoustic oscillations, observed in the CMB and BAO, as well as the weak gravitational lensing of the CMB and of galaxy shapes.
This widens the pool of measurements that can be used to test gravity with present and future surveys, in particular realizing the full constraining power of the structure of the primary peaks of the CMB spectrum.
We investigate whether such a phenomenology can relax tensions between cosmological measurements and find that a modification of the gravitational constant at recombination would help in reconciling measurements of the CMB with local measurements of the Hubble constant.

Built on

W. Hu and N. Sugiyama, Astrophys. J. 444
1995
Earlier work this paper cites.
C.-P. Ma and E. Bertschinger, Astrophys. J. 455
1995
Earlier work this paper cites.
W. Hu and N. Sugiyama, Astrophys. J. 471
1996
Earlier work this paper cites.
A. G. Riess et al. (Supernova Search Team), Astron. J. 116
1998
Earlier work this paper cites.
W. Hu and D. J. Eisenstein, Astrophys. J. 498
1998
Earlier work this paper cites.
S. Perlmutter et al. (Supernova Cosmology Project), Astrophys. J. 517
1999
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Astrophys. J. 538
2000
Earlier work this paper cites.
R. Caldwell, A. Cooray, and A. Melchiorri, Phys. Rev. D76
2007
Earlier work this paper cites.
W. Hu and I. Sawicki, Phys. Rev. D76
Original
2007
Earlier work this paper cites.
L. Amendola, M. Kunz, and D. Sapone, JCAP 0804
Original
2008
Earlier work this paper cites.
E. Bertschinger and P. Zukin, Phys. Rev. D78
Original
2008
Earlier work this paper cites.
L. Hui and K. P. Parfrey, Phys. Rev. D77
Original
2008
Earlier work this paper cites.
A. Silvestri and M. Trodden, Rept. Prog. Phys. 72
Original
2009
Earlier work this paper cites.
P. A. Abell et al. (LSST Science, LSST Project), (2009), arXiv:0912.0201 [astro-ph.IM]
Original
2009
Earlier work this paper cites.
L. Pogosian, A. Silvestri, K. Koyama, and G.-B. Zhao, Phys. Rev. D81
Original
2010
Earlier work this paper cites.
R. Laureijs et al. (EUCLID), (2011), arXiv:1110.3193 [astro-ph.CO]
Original
2011
Earlier work this paper cites.
A. Hojjati, L. Pogosian, and G.-B. Zhao, JCAP 1108
Original
2011
Earlier work this paper cites.