Cosmic strings in a model of non-relativistic gravity
D.Momeni

TL;DR
This paper explores cosmic string solutions within Hořava's non-relativistic gravity, revealing how coupling constants influence string properties and proposing potential cosmological tests for the theory's validity.
Contribution
It derives the most general cosmic string solutions in Hořava gravity and analyzes how coupling constants modify their characteristics compared to general relativity.
Findings
Coupling constants distort the mass parameter of cosmic strings.
Explicit function for mass per unit length as a function of coupling constants.
Order of magnitude estimate for coupling constants suggests possible cosmological tests.
Abstract
Hoava proposed a non-relativistic renormalizable theory of gravitation, which is reduced to general relativity (GR) in large distances (infra-red regime (IR)). It is believed that this theory is an ultra-violet (UV) completion for the classical theory of gravitation. In this paper, after a brief review of some fundamental features of this theory, we investigate it for a static cylindrical symmetric solution which describes \emph{Cosmic string} as a special case. We have also investigated some possible solutions, and have seen that how the classical GR field equations are modified for generic potential . In one case there is an algebraic constraint on the values of three coupling constants. Finally as a pioneering work we deduce the most general \emph{cosmic string} in this theory. We explicitly show that how the \emph{coupling constants} distort the mass…
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