Soliton foam formation in the early Universe

The formation of composite solitons produced by scalar fields without thermal phase transitions in the early Universe is considered. We present numerical simulations of the formation and evolution of soliton structures at the post-inflationary stage. The realistic initial conditions are obtained thr...

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Main Authors: A.A. Kirillov, B.S. Murygin, V.V. Nikulin
Format: Article
Language:English
Published: Elsevier 2025-01-01
Series:Physics Letters B
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Online Access:http://www.sciencedirect.com/science/article/pii/S0370269324007597
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author A.A. Kirillov
B.S. Murygin
V.V. Nikulin
author_facet A.A. Kirillov
B.S. Murygin
V.V. Nikulin
author_sort A.A. Kirillov
collection DOAJ
description The formation of composite solitons produced by scalar fields without thermal phase transitions in the early Universe is considered. We present numerical simulations of the formation and evolution of soliton structures at the post-inflationary stage. The realistic initial conditions are obtained through the simulation of multiple quantum fluctuations during the inflation epoch. The initial field distributions allow to form local soliton clusters in the early Universe without the need for the thermal production of a soliton network throughout the Universe. We find that in three-dimensional space, the nontrivial composite field structures are formed in the form of <<soliton foam>>, consisting of closed domain walls, domain walls bounded by cosmic strings, and scalar field radiation. The possible cosmological implications of the soliton foam are discussed.
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institution Kabale University
issn 0370-2693
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publishDate 2025-01-01
publisher Elsevier
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series Physics Letters B
spelling doaj-art-f4542e0f3d864609afb9fb1b2ee511302025-01-10T04:37:37ZengElsevierPhysics Letters B0370-26932025-01-01860139201Soliton foam formation in the early UniverseA.A. Kirillov0B.S. Murygin1V.V. Nikulin2National Research Nuclear University MEPhI, Moscow Engineering Physics Institute, Kashirskoe shosse 31, Moscow, 115409, RussiaCorresponding author.; National Research Nuclear University MEPhI, Moscow Engineering Physics Institute, Kashirskoe shosse 31, Moscow, 115409, RussiaNational Research Nuclear University MEPhI, Moscow Engineering Physics Institute, Kashirskoe shosse 31, Moscow, 115409, RussiaThe formation of composite solitons produced by scalar fields without thermal phase transitions in the early Universe is considered. We present numerical simulations of the formation and evolution of soliton structures at the post-inflationary stage. The realistic initial conditions are obtained through the simulation of multiple quantum fluctuations during the inflation epoch. The initial field distributions allow to form local soliton clusters in the early Universe without the need for the thermal production of a soliton network throughout the Universe. We find that in three-dimensional space, the nontrivial composite field structures are formed in the form of <<soliton foam>>, consisting of closed domain walls, domain walls bounded by cosmic strings, and scalar field radiation. The possible cosmological implications of the soliton foam are discussed.http://www.sciencedirect.com/science/article/pii/S0370269324007597SolitonsDomain wallsEarly universe
spellingShingle A.A. Kirillov
B.S. Murygin
V.V. Nikulin
Soliton foam formation in the early Universe
Physics Letters B
Solitons
Domain walls
Early universe
title Soliton foam formation in the early Universe
title_full Soliton foam formation in the early Universe
title_fullStr Soliton foam formation in the early Universe
title_full_unstemmed Soliton foam formation in the early Universe
title_short Soliton foam formation in the early Universe
title_sort soliton foam formation in the early universe
topic Solitons
Domain walls
Early universe
url http://www.sciencedirect.com/science/article/pii/S0370269324007597
work_keys_str_mv AT aakirillov solitonfoamformationintheearlyuniverse
AT bsmurygin solitonfoamformationintheearlyuniverse
AT vvnikulin solitonfoamformationintheearlyuniverse