Effects of temperature on thick branes and the fermion (quasi-)localization

TL;DR

This paper studies how temperature influences the structure and fermion localization on various types of thick branes in five-dimensional warped spacetime, revealing critical temperature effects and resonance behaviors.

Contribution

It provides a detailed analysis of temperature effects on flat, dS, and AdS thick branes, including fermion resonance spectra and the existence of critical temperature thresholds.

Findings

Flat branes exhibit a critical temperature where solutions become non-unique.

Fermion KK modes show continuous spectra with temperature-dependent resonances.

AdS branes have discrete spectra with non-monotonic mass changes at different temperatures.

Abstract

Following Campos's work [Phys. Rev. Lett. 88, 141602 (2002)], we investigate the effects of temperature on flat, de Sitter (dS), and anti-de Following Campos's work [Phys. Rev. Lett. \textbf{88}, 141602 (2002)], we investigate the effects of temperature on flat, de Sitter (dS), and anti-de Sitter (AdS) thick branes in five-dimensional (5D) warped spacetime, and on the fermion (quasi-)localization. First, in the case of flat brane, when the critical temperature reaches, the solution of the background scalar field and the warp factor is not unique. So the thickness of the flat thick brane is uncertain at the critical value of the temperature parameter, which is found to be lower than the one in flat 5D spacetime. The mass spectra of the fermion Kaluza-Klein (KK) modes are continuous, and there is a series of fermion resonances. The number and lifetime of the resonances are finite and increase with the temperature parameter, but the mass of the resonances decreases with the temperature parameter. Second, in the case of dS brane, we do not find such a critical value of the temperature parameter. The mass spectra of the fermion KK modes are also continuous, and there is a series of fermion resonances. The effects of temperature on resonance number, lifetime, and mass are the same with the case of flat brane. Last, in the case of AdS brane, {the critical value of the temperature parameter can less or greater than the one in the flat 5D spacetime.} The spectra of fermion KK modes are discrete, and the mass of fermion KK modes does not decrease monotonically with increasing temperature parameter.