English

On Quantum Radiation in Curved Spacetime

High Energy Physics - Theory 2009-11-07 v2 Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

In the context of quantum field theories in curved spacetime, we compute the effective action of the transition amplitude from vacuum to vacuum in the presence of an external gravitational field. The imaginary part of resulted effective action determines the probability of vacuum decay via quantum tunneling process, giving the rate and spectrum of particle creations. We show that gravitational field polarizes vacuum and discretizes its spectrum for such a polarization gains gravitational energy. On the basis of gravitational vacuum polarization, we discuss the quantum origin of vacuum decay in curved spacetime as pair-creations of particles and anti-particles. The thermal spectrum of particle creations is attributed to (i) the CPT invariance of pair-creations(annihilations) from(into) vacuum and (ii) vacuum acts as a reserve with the temperature determined by gravitational energy-gain.

Keywords

Cite

@article{arxiv.hep-th/0204060,
  title  = {On Quantum Radiation in Curved Spacetime},
  author = {She-Sheng Xue},
  journal= {arXiv preprint arXiv:hep-th/0204060},
  year   = {2009}
}

Comments

18 pages, revised lengthy version

R2 v1 2026-07-22T15:10:01.961Z