Late time evolution of the gravitational wave damping in the early Universe
Gavriil Shchedrin

TL;DR
This paper derives an analytical series solution describing how gravitational waves are damped over time in the early Universe due to neutrino streaming, enhancing understanding of early cosmological dynamics.
Contribution
It introduces a new compact formula for convolutions of spherical Bessel functions, enabling an exact series solution for gravitational wave damping.
Findings
Analytical late-time solution for gravitational wave damping.
Series expressed as spherical Bessel functions of even order.
New convolution formula for spherical Bessel functions.
Abstract
An analytical solution for time evolution of the gravitational wave damping in the early Universe due to freely streaming neutrinos is found in the late time regime. The solution is represented by a convergent series of spherical Bessel functions of even order and was possible with the help of a new compact formula for the convolution of spherical Bessel functions of integer order.
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Geophysics and Gravity Measurements
