Eternal binaries

Fuente: arXiv
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Autori principali: Redondo-Yuste, Jaime, Cardoso, Vitor, Macedo, Caio F. B., van de Meent, Maarten
Natura: Preprint
Pubblicazione: 2023
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author Redondo-Yuste, Jaime
Cardoso, Vitor
Macedo, Caio F. B.
van de Meent, Maarten
author_facet Redondo-Yuste, Jaime
Cardoso, Vitor
Macedo, Caio F. B.
van de Meent, Maarten
contents The two-body problem is extensively studied in open systems and asymptotically flat spacetimes. However, there are many systems where radiation is trapped: they range from radiating charges in cavities to low-energy excitations of massive degrees of freedom, to anti-de Sitter spacetimes. Here, we study the problem of motion of a pointlike particle orbiting a massive compact object inside a cavity. We first show that - assuming circular motion - there are initial conditions for which the self-force vanishes and the binary is eternal. We then consider the evolution of the system under radiation reaction in a toy model which we argue captures the essentials of orbiting particles. We show that eternal circular binaries may exist. We also show that the presence of cavity modes leads to chaos in regimes of strong coupling or when the system is initialized close enough to a resonance. Our results have implications for physics in anti-de Sitter spacetimes and possibly for binaries evolving within dark matter haloes, if it consists on massive fundamental fields.
format Preprint
id arxiv_https___arxiv_org_abs_2304_02039
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Eternal binaries
Redondo-Yuste, Jaime
Cardoso, Vitor
Macedo, Caio F. B.
van de Meent, Maarten
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
High Energy Physics - Theory
The two-body problem is extensively studied in open systems and asymptotically flat spacetimes. However, there are many systems where radiation is trapped: they range from radiating charges in cavities to low-energy excitations of massive degrees of freedom, to anti-de Sitter spacetimes. Here, we study the problem of motion of a pointlike particle orbiting a massive compact object inside a cavity. We first show that - assuming circular motion - there are initial conditions for which the self-force vanishes and the binary is eternal. We then consider the evolution of the system under radiation reaction in a toy model which we argue captures the essentials of orbiting particles. We show that eternal circular binaries may exist. We also show that the presence of cavity modes leads to chaos in regimes of strong coupling or when the system is initialized close enough to a resonance. Our results have implications for physics in anti-de Sitter spacetimes and possibly for binaries evolving within dark matter haloes, if it consists on massive fundamental fields.
title Eternal binaries
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2304.02039