PreprintarXiv licencearXiv
Gravitational Waves and Nambu-Goldstone Bosons from Infrared-Finite Cosmic Strings
Abstract
Skyrmion lines and semi-local strings are examples of infrared-finite cosmic strings that arise in theories with spontaneously broken global symmetries. Unlike global U(1) strings, they do not support the long-range Nambu-Goldstone boson (NGB) profile responsible for a logarithmically infrared-divergent string tension. We argue that NGB emission from their low-frequency oscillations is strongly suppressed. Consequently, their gravitational-wave signals may be comparable to those from local strings.
Related
- Impact of cosmic evolution on the gravitational wave spectrum from cosmic strings
- Enhancing Gravitational Waves from Global Strings via a First-Order Phase Transition
- Gravitational Wave Background from Metastable Current-Carrying Cosmic Strings
- Detection of cosmic strings by gravitational wave lensing. Predictions for Einstein Telescope
- Interpretation of Nanohertz Gravitational Waves via Cosmic Strings in Post-BBN Matter and Kination Domination
BibTeX
@misc{fukuda2026gravitational,
title = {{Gravitational Waves and Nambu-Goldstone Bosons from Infrared-Finite Cosmic Strings}},
author = {Hajime Fukuda and Shuailiang Ge and Keisuke Harigaya},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.08254},
eprint = {2610.08254},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.08254},
}
RIS
TY - UNPB
TI - Gravitational Waves and Nambu-Goldstone Bosons from Infrared-Finite Cosmic Strings
AU - Hajime Fukuda
AU - Shuailiang Ge
AU - Keisuke Harigaya
PY - 2026
DA - 2026/10/06
PB - arXiv
DO - 10.48550/arxiv.2610.08254
UR - https://arxiv.org/abs/2610.08254
AB - Skyrmion lines and semi-local strings are examples of infrared-finite cosmic strings that arise in theories with spontaneously broken global symmetries. Unlike global U(1) strings, they do not support the long-range Nambu-Goldstone boson (NGB) profile responsible for a logarithmically infrared-divergent string tension. We argue that NGB emission from their low-frequency oscillations is strongly suppressed. Consequently, their gravitational-wave signals may be comparable to those from local strings.
ER -