Metastable strings at PTAs: classical stability analysis

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autores principales: Blasi, Simone, Grandjean, Maxime, Mariotti, Alberto
Formato: Preprint
Publicado: 2026
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866914528531316736
author Blasi, Simone
Grandjean, Maxime
Mariotti, Alberto
author_facet Blasi, Simone
Grandjean, Maxime
Mariotti, Alberto
contents Metastable strings can arise from a two-step symmetry breaking chain of the type $SU(2) \to U(1) \to 1$.They can decay through quantum tunneling by nucleating a monopole-antimonopole pair, and are prominent candidates for explaining the gravitational wave background detected at Pulsar Timing Arrays (PTAs).We investigate the classical stability of the strings arising in this commonly-considered setup, which serves as a fundamental input for discussing their possible decay channels. We identify the regions of parameter space in which the strings are either classically stable or unstable. Our results show that classical instabilities can impact the parameter space relevant for PTAs. We also discuss the possible fate of the string network in the regions of classical instability.
format Preprint
id arxiv_https___arxiv_org_abs_2605_03003
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Metastable strings at PTAs: classical stability analysis
Blasi, Simone
Grandjean, Maxime
Mariotti, Alberto
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
Metastable strings can arise from a two-step symmetry breaking chain of the type $SU(2) \to U(1) \to 1$.They can decay through quantum tunneling by nucleating a monopole-antimonopole pair, and are prominent candidates for explaining the gravitational wave background detected at Pulsar Timing Arrays (PTAs).We investigate the classical stability of the strings arising in this commonly-considered setup, which serves as a fundamental input for discussing their possible decay channels. We identify the regions of parameter space in which the strings are either classically stable or unstable. Our results show that classical instabilities can impact the parameter space relevant for PTAs. We also discuss the possible fate of the string network in the regions of classical instability.
title Metastable strings at PTAs: classical stability analysis
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2605.03003