Hot scalar radiation around a cosmic string setting bounds on the coupling parameter
arXiv:1604.08089 · doi:10.1007/JHEP03(2017)105
Abstract
In this work, by investigating the low temperature behaviour of a scalar field around a cosmic string, and assuming stable thermodynamic equilibrium, it is shown that the coupling parameter of the field with curvature must be restricted to a certain range of values whose bounds are determined by the deficit angle of the associated conical geometry.
12 pages, 1 figure. The material has been expanded and the manuscript matches the published version (JHEP)
References in corpus (3)
Cited by in corpus (5)
- Vacuum fluctuations of a scalar field near a reflecting boundary and their effects on the motion of a test particle
- Probing thermal fluctuations through scalar test particles
- Finite temperature charge and current densities around a cosmic string in AdS spacetime with compact dimension
- Ambiguities in the local thermal behavior of the scalar radiation in one-dimensional boxes
- Thermodynamic stability in an Einstein universe