Higher-derivative Lorentz-breaking dispersion relations: a thermal description
arXiv:2103.08738 · doi:10.1140/epjc/s10052-021-09639-y
Abstract
This paper is devoted to study the thermal aspects of a photon gas within the context of Planck-scale-modified dispersion relations. We study the spectrum of radiation and the correction to the \textit{StefanBoltzmann} law in different cases when the Lorentz symmetry is no longer preserved. Explicitly, we examine two models within the context of CPTeven and CPTodd sectors respectively. To do so, three distinct scenarios of the Universe are considered: the Cosmic Microwave Background (CMB), the electroweak epoch, and the inflationary era. Moreover, the equations of state in these cases turn out to display a dependence on Lorentz-breaking parameters. Finally, we also provide for both theories the analyses of the Helmholtz free energy, the mean energy, the entropy and the heat capacity.
24 pages, 13 figures
References in corpus (11)
- Quantum Gravity at a Lifshitz Point
- Electrodynamics with Lorentz-violating operators of arbitrary dimension
- The Superluminous Transient ASASSN-15lh as a Tidal Disruption Event from a Kerr Black Hole
- What Do We Know About Lorentz Invariance?
- Tests of Lorentz symmetry in the gravitational sector
- Lorentz-violating contributions of the Carroll-Field-Jackiw model to the CMB anisotropy
- Finite Temperature behavior of the CPT-even and parity-even electrodynamics of the Standard Model Extension
- Bouncing universe in a heat bath
- Lorentz Invariance Violation from String Theory
- Geometric effects on the electronic structure of curved nanotubes and curved graphene: the case of the helix, catenary, helicoid, and catenoid
- Fermions on a torus knot
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