Gravitational wave luminosity distance for Starobinsky gravity in viscous cosmological models
Abstract In this paper, in the Starobinsky gravity (SG) model, the gravitational wave (GW) luminosity distance $$d_L^{GW}(z)$$ d L GW ( z ) is analytically and numerically investigated by considering the dark matter as the two different kinds of shear viscous fluids in universe. Concretely, on the b...
Saved in:
Main Authors: | Jia-nan Chi, Ya-Bo Wu, Yu Sang, Xue Zhang, Yi-liang Hu, Wen-zhong Liu, Bo-hai Chen |
---|---|
Format: | Article |
Language: | English |
Published: |
SpringerOpen
2025-01-01
|
Series: | European Physical Journal C: Particles and Fields |
Online Access: | https://doi.org/10.1140/epjc/s10052-024-13564-1 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Anisotropic Bulk Viscous String Cosmological Model in a Scalar-Tensor Theory of Gravitation
by: D. R. K. Reddy, et al.
Published: (2013-01-01) -
Weyl fermion creation by cosmological gravitational wave background at 1-loop
by: Azadeh Maleknejad, et al.
Published: (2025-01-01) -
Luminosity Distance and Extinction by Submicrometer-sized Grains
by: R. Siebenmorgen, et al.
Published: (2025-01-01) -
Viscous damping of gravity waves over a permeable bed
by: K. K. Puri
Published: (1978-01-01) -
Acoustic-gravity waves in a viscous and thermally conducting isothermal atmosphere
by: H. Y. Alkahby
Published: (1995-01-01)