The kinetic gas universe
arXiv:2005.13561 · doi:10.1140/epjc/s10052-020-8391-y
Abstract
A description of many-particle systems, which is more fundamental than the fluid approach, is to consider them as a kinetic gas. In this approach the dynamical variable in which the properties of the system are encoded, is the distribution of the gas particles in position and velocity space, called 1-particle distribution function (1PDF). However, when the gravitational field of a kinetic gas is derived via the Einstein-Vlasov equations, the information about the velocity distribution of the gas particles is averaged out and therefore lost. We propose to derive the gravitational field of a kinetic gas directly from its 1PDF, taking the velocity distribution fully into account. We conjecture that this refined approach could possibly account for the observed dark energy phenomenology.
4 pages, Essay written for the Gravity Research Foundation competition 2020, Journal references updated
References in corpus (1)
Cited by in corpus (4)
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- Relativistic deformed kinematics: from flat to curved spacetimes