TH Cosmo Coffee

Damping of gravitational waves by matter

by Dr. Subodh Patil (Niels Bohr Institute (DK))

Europe/Zurich
4-3-006 - TH Conference Room (CERN)

4-3-006 - TH Conference Room

CERN

100
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Description

 I'll discuss a recently developed treatment of damping of gravitational waves by matter, which can interpolate between the kinetic and hydrodynamic regimes, incorporating collisions. We identify two physically distinct damping mechanisms -- collisional and Landau damping. Maximal collisional damping of a gravitational wave, independent of the details of the matter collisions is significant only when its wavelength is comparable to the size of the horizon. Thus damping by intergalactic or interstellar matter for all but primordial gravitational radiation can be neglected. Although collisions in matter lead to a shear viscosity, they also act to erase anisotropic stresses, thus suppressing damping. Damping of primordial gravitational waves remains possible. We generalize Weinberg's calculation of gravitational wave damping, now including collisions and particles of finite mass and interpret the collisionless limit in terms of Landau damping. We comment on the possible processing of primordial gravitational waves during matter domination in various dark matter scenarios. The discussion will be based on arXiv:1707.05192.

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