Falling from Rest: Particle Creation in a Dropped Cavity
We discuss the process of particle creation in the case of a scalar quantum field confined to a small cavity, initially at rest, which is suddenly dropped in a static gravitational field. We show that, due to the transition from a Schwarzschild to a Minkowski background, as perceived by a comoving o...
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doaj-ecb829f83b7d44f499ead699539bdeff2021-07-23T14:09:01ZengMDPI AGSymmetry2073-89942021-06-01131139113910.3390/sym13071139Falling from Rest: Particle Creation in a Dropped CavityFrancesco Sorge0I.N.F.N. Sezione di Napoli, Complesso Universitario di Monte S. Angelo, Via Cintia, Edificio 6, I-80126 Napoli, ItalyWe discuss the process of particle creation in the case of a scalar quantum field confined to a small cavity, initially at rest, which is suddenly dropped in a static gravitational field. We show that, due to the transition from a Schwarzschild to a Minkowski background, as perceived by a comoving observer, field particles are excited out of the quantum vacuum. The density of the created quanta depends on the proper gravitational acceleration as well as on a parameter <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>α</mi><mo>≃</mo><mn>1</mn><mo>/</mo><mo>Δ</mo><mi>t</mi></mrow></semantics></math></inline-formula>, with <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>Δ</mo><mi>t</mi></mrow></semantics></math></inline-formula> representing the typical time duration of the transition. For the specific acceleration profile considered, the energy spectrum of the created quanta roughly resembles a two-dimensional Planckian distribution, whose equivalent temperature mimics the Hawking-Unruh temperature, with the detector acceleration (or the black hole surface gravity) replaced by the parameter <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>c</mi><mi>α</mi></mrow></semantics></math></inline-formula>. We briefly comment on possible issues related to local Lorentz symmetry.https://www.mdpi.com/2073-8994/13/7/1139accelerationparticle creationquantum fieldsgeneral relativity |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Francesco Sorge |
spellingShingle |
Francesco Sorge Falling from Rest: Particle Creation in a Dropped Cavity Symmetry acceleration particle creation quantum fields general relativity |
author_facet |
Francesco Sorge |
author_sort |
Francesco Sorge |
title |
Falling from Rest: Particle Creation in a Dropped Cavity |
title_short |
Falling from Rest: Particle Creation in a Dropped Cavity |
title_full |
Falling from Rest: Particle Creation in a Dropped Cavity |
title_fullStr |
Falling from Rest: Particle Creation in a Dropped Cavity |
title_full_unstemmed |
Falling from Rest: Particle Creation in a Dropped Cavity |
title_sort |
falling from rest: particle creation in a dropped cavity |
publisher |
MDPI AG |
series |
Symmetry |
issn |
2073-8994 |
publishDate |
2021-06-01 |
description |
We discuss the process of particle creation in the case of a scalar quantum field confined to a small cavity, initially at rest, which is suddenly dropped in a static gravitational field. We show that, due to the transition from a Schwarzschild to a Minkowski background, as perceived by a comoving observer, field particles are excited out of the quantum vacuum. The density of the created quanta depends on the proper gravitational acceleration as well as on a parameter <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>α</mi><mo>≃</mo><mn>1</mn><mo>/</mo><mo>Δ</mo><mi>t</mi></mrow></semantics></math></inline-formula>, with <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>Δ</mo><mi>t</mi></mrow></semantics></math></inline-formula> representing the typical time duration of the transition. For the specific acceleration profile considered, the energy spectrum of the created quanta roughly resembles a two-dimensional Planckian distribution, whose equivalent temperature mimics the Hawking-Unruh temperature, with the detector acceleration (or the black hole surface gravity) replaced by the parameter <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>c</mi><mi>α</mi></mrow></semantics></math></inline-formula>. We briefly comment on possible issues related to local Lorentz symmetry. |
topic |
acceleration particle creation quantum fields general relativity |
url |
https://www.mdpi.com/2073-8994/13/7/1139 |
work_keys_str_mv |
AT francescosorge fallingfromrestparticlecreationinadroppedcavity |
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