Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theories
We consider the evolution of cosmological gravitational waves in scalar–tensor theory and F(R) gravity theory as typical models of the modified gravity. Although the propagation speed is not changed from the speed of light, the propagation phase changes when we compare the propagation in these modif...
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doaj-8f0a92eb88fe40459017cc9b01b1e56b2020-11-24T20:57:49ZengElsevierPhysics Letters B0370-26932018-04-01779425429Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theoriesShin'ichi Nojiri0Sergei D. Odintsov1Department of Physics, Nagoya University, Nagoya 464-8602, Japan; Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya 464-8602, Japan; KEK Theory Center, High Energy Accelerator Research Organization (KEK), Oho 1-1, Tsukuba, Ibaraki 305-0801, Japan; Corresponding author.ICREA, Passeig Luis Companys, 23, 08010 Barcelona, Spain; Inst. Space Sciences (ICE-CSIC), C. Can Magrans s/n, 08193 Barcelona, Spain; Inst. Space Sciences of Catalonia (IEEC), 08034 Barcelona, Spain; National Research Tomsk State University, 634050 Tomsk, Russia; Tomsk State Pedagogical University, 634061 Tomsk, Russia; Int. Lab. Theor. Cosmology, TUSUR, 534050 Tomsk, RussiaWe consider the evolution of cosmological gravitational waves in scalar–tensor theory and F(R) gravity theory as typical models of the modified gravity. Although the propagation speed is not changed from the speed of light, the propagation phase changes when we compare the propagation in these modified gravity theories with the propagation in the ΛCDM model. The phase change might be detected in future observations. Keywords: Gravitational waves, Alternative theories of gravity, Cosmologyhttp://www.sciencedirect.com/science/article/pii/S0370269318300960 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Shin'ichi Nojiri Sergei D. Odintsov |
spellingShingle |
Shin'ichi Nojiri Sergei D. Odintsov Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theories Physics Letters B |
author_facet |
Shin'ichi Nojiri Sergei D. Odintsov |
author_sort |
Shin'ichi Nojiri |
title |
Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theories |
title_short |
Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theories |
title_full |
Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theories |
title_fullStr |
Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theories |
title_full_unstemmed |
Cosmological bound from the neutron star merger GW170817 in scalar–tensor and F(R) gravity theories |
title_sort |
cosmological bound from the neutron star merger gw170817 in scalar–tensor and f(r) gravity theories |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2018-04-01 |
description |
We consider the evolution of cosmological gravitational waves in scalar–tensor theory and F(R) gravity theory as typical models of the modified gravity. Although the propagation speed is not changed from the speed of light, the propagation phase changes when we compare the propagation in these modified gravity theories with the propagation in the ΛCDM model. The phase change might be detected in future observations. Keywords: Gravitational waves, Alternative theories of gravity, Cosmology |
url |
http://www.sciencedirect.com/science/article/pii/S0370269318300960 |
work_keys_str_mv |
AT shinichinojiri cosmologicalboundfromtheneutronstarmergergw170817inscalartensorandfrgravitytheories AT sergeidodintsov cosmologicalboundfromtheneutronstarmergergw170817inscalartensorandfrgravitytheories |
_version_ |
1716787391658721280 |