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2021

Type Ia supernovae data with scalar-tensor gravity

Ballardini, Mario, Finelli, Fabio

Understand

We study the use of type Ia supernovae (SNe Ia) in the context of scalar-tensor theories of gravity, taking as a working example induced gravity, equivalent to Jordan-Brans-Dicke theory.

Winking at accurate and precision cosmology, we test the correction introduced by a time variation of the Newton's constant, predicted by scalar-tensor theories, on the SNe distance modulus relation.
We find that for induced gravity the coupling parameter is constrained from $\xi < 0.0095$ (95\% CL) using Pantheon SNe data alone down to $\xi < 0.00063$ (95\% CL) in combination with {\em Planck} data release DR3 and a compilation of baryon acoustic oscillations (BAO) measurements from BOSS DR12.
In this minimal case the improvements in terms of constraints on the cosmological parameters coming from the addition of SNe data to cosmic microwave background (CMB) and BAO measurements is limited, $\sim7\%$ on the 95\% CL upper bound on $\xi$.

Built on

W. D. Kenworthy, D. Scolnic and A. Riess, Astrophys. J
Original
1901
Earlier work this paper cites.
P. Agrawal, F. Y. Cyr-Racine, D. Pinner and L. Randall, [arXiv:1904.01016 [astro-ph.CO]]
Original
1904
Earlier work this paper cites.
D. Camarena and V. Marra, Phys. Rev. Res
Original
1906
Earlier work this paper cites.
M. Rossi, M. Ballardini, M. Braglia, F. Finelli, D. Paoletti, A. A. Starobinsky and C. Umiltà, Phys. Rev. D
Original
1906
Earlier work this paper cites.
H. Desmond, B. Jain and J. Sakstein, Phys. Rev. D
Original
1907
Earlier work this paper cites.
N. Aghanim
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, Phys. Rev. D
Original
1908
Earlier work this paper cites.
M. J. Reid, D. W. Pesce and A. G. Riess, Astrophys. J. Lett
Original
1908
Earlier work this paper cites.
L. Hart and J. Chluba, Mon. Not. Roy. Astron. Soc
Original
1912
Earlier work this paper cites.
P. Jordan, Nature
1949
Earlier work this paper cites.
C. Brans and R. H. Dicke, Phys. Rev
1961
Earlier work this paper cites.
F. Cooper and G. Venturi, Phys. Rev. D
1981
Earlier work this paper cites.
W. D. Arnett, Astrophys. J
1982
Earlier work this paper cites.
D. Branch and G. A. Tammann, Ann. Rev. Astron. Astrophys
1992
Earlier work this paper cites.
A. G. Riess
1998
Earlier work this paper cites.
R. Tripp, Astron. Astrophys
1998
Earlier work this paper cites.
S. Perlmutter
1999
Earlier work this paper cites.
L. Amendola, Phys. Rev. D
1999
Earlier work this paper cites.
B. Boisseau, G. Esposito-Farese, D. Polarski and A. A. Starobinsky, Phys. Rev. Lett
2000
Earlier work this paper cites.
V. Sahni and A. A. Starobinsky, Int. J. Mod. Phys. D
2000
Earlier work this paper cites.
B. Leibundgut, Ann. Rev. Astron. Astrophys
2001
Earlier work this paper cites.
S. M. Carroll, Living Rev. Rel
2001
Earlier work this paper cites.
E. Gaztanaga, E. Garcia-Berro, J. Isern, E. Bravo and I. Dominguez, Phys. Rev. D
2002
Earlier work this paper cites.
A. Riazuelo and J. P. Uzan, Phys. Rev. D
2002
Earlier work this paper cites.