Scalar Radiation in Interaction of Cosmic String with Point Charge

We consider the scalar bremsstrahlung of the spinless relativistic particle, which interacts with infinitely thin cosmic string by linearized gravity. With the iterational scheme, based on the Perturbaion Theory with respect to the Newtonian constant, we compute the radiation amplitude and the emitt...

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Main Author: Pavel Spirin
Format: Article
Language:English
Published: MDPI AG 2021-06-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/7/7/206
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author Pavel Spirin
author_facet Pavel Spirin
author_sort Pavel Spirin
collection DOAJ
description We consider the scalar bremsstrahlung of the spinless relativistic particle, which interacts with infinitely thin cosmic string by linearized gravity. With the iterational scheme, based on the Perturbaion Theory with respect to the Newtonian constant, we compute the radiation amplitude and the emitted energy due to collision. The general phenomenon of mutual cancellation of the leading terms on the local and non-local amplitude, known in the ultrarelativistic regime for several types of collision, also takes place here. Remarkably, this cancellation (destructive interference) is complete, and takes place for any particle’s velocity. We compute the spectral and angular distributions of the emitted waves. Particular attention is paid to the ultrarelativistic case. Due to the radiation emission, a string may lose its energy and decrease the tension; it may affect all field effects, including the vacuum polarization and the Casimir effect, in terms of physical problems with the real cosmic strings.
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spelling doaj.art-7efed482029b4198aa65334411d440122023-11-22T01:18:00ZengMDPI AGUniverse2218-19972021-06-017720610.3390/universe7070206Scalar Radiation in Interaction of Cosmic String with Point ChargePavel Spirin0Physics Department, M.V. Lomonosov Moscow State University, Leninskie Gory 1/2, 119991 Moscow, RussiaWe consider the scalar bremsstrahlung of the spinless relativistic particle, which interacts with infinitely thin cosmic string by linearized gravity. With the iterational scheme, based on the Perturbaion Theory with respect to the Newtonian constant, we compute the radiation amplitude and the emitted energy due to collision. The general phenomenon of mutual cancellation of the leading terms on the local and non-local amplitude, known in the ultrarelativistic regime for several types of collision, also takes place here. Remarkably, this cancellation (destructive interference) is complete, and takes place for any particle’s velocity. We compute the spectral and angular distributions of the emitted waves. Particular attention is paid to the ultrarelativistic case. Due to the radiation emission, a string may lose its energy and decrease the tension; it may affect all field effects, including the vacuum polarization and the Casimir effect, in terms of physical problems with the real cosmic strings.https://www.mdpi.com/2218-1997/7/7/206cosmic stringpoint chargegravitational interactionbremsstrahlungdestructive interferenceperturbation theory
spellingShingle Pavel Spirin
Scalar Radiation in Interaction of Cosmic String with Point Charge
Universe
cosmic string
point charge
gravitational interaction
bremsstrahlung
destructive interference
perturbation theory
title Scalar Radiation in Interaction of Cosmic String with Point Charge
title_full Scalar Radiation in Interaction of Cosmic String with Point Charge
title_fullStr Scalar Radiation in Interaction of Cosmic String with Point Charge
title_full_unstemmed Scalar Radiation in Interaction of Cosmic String with Point Charge
title_short Scalar Radiation in Interaction of Cosmic String with Point Charge
title_sort scalar radiation in interaction of cosmic string with point charge
topic cosmic string
point charge
gravitational interaction
bremsstrahlung
destructive interference
perturbation theory
url https://www.mdpi.com/2218-1997/7/7/206
work_keys_str_mv AT pavelspirin scalarradiationininteractionofcosmicstringwithpointcharge