<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Q</mml:mi></mml:math>-ball collisions and their gravitational waves

Sydney Coleman’s Q-ball remains a compelling instance of the formation of localized objects within classical field theory, independently of the quantum evolution. The theoretical possibility of such objects forming and colliding in the early Universe from models such as Affleck-Dine fragmentation, or from a number of mechanisms where they are produced copiously with various sizes and charges to constitute dark matter in the Universe, makes it important to study in detail Q-ball collision phenomenology. In this work, we present certain results from the study of Q-ball collisions and their generation of gravitational waves, using a new general code package for scalar fields coupled to gravity. We then comment on the possibility of future gravitational wave detectors searching for signals of Q-ball collisions. Published by the American Physical Society 2024

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Journal
Physical review. D/Physical review. D.
Published
2024-12-27
DOI
https://doi.org/10.1103/physrevd.110.123037
Citations
1
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.33

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article

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Q</mml:mi></mml:math>-ball collisions and their gravitational waves

Deog Ki Hong, Stephen J. Lonsdale
1 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
0.33
article

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Q</mml:mi></mml:math>-ball collisions and their gravitational waves

Deog Ki Hong, Stephen J. Lonsdale
article en
1 citations

Abstract

Sydney Coleman’s Q-ball remains a compelling instance of the formation of localized objects within classical field theory, independently of the quantum evolution. The theoretical possibility of such objects forming and colliding in the early Universe from models such as Affleck-Dine fragmentation, or from a number of mechanisms where they are produced copiously with various sizes and charges to constitute dark matter in the Universe, makes it important to study in detail Q-ball collision phenomenology. In this work, we present certain results from the study of Q-ball collisions and their generation of gravitational waves, using a new general code package for scalar fields coupled to gravity. We then comment on the possibility of future gravitational wave detectors searching for signals of Q-ball collisions. Published by the American Physical Society 2024

Physical review. D/Physical review. D.Vol. 110(12)
Pusan National University (KR)
Pusan National University
Openalex Percentile: Top 32%
Pulsars and Gravitational Waves Research
0.33
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