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Cosmic string solution to the radio synchrotron background

Research output: Contribution to journalLetterpeer-review

Abstract

We investigate the low-frequency spectral emission from a network of superconducting cosmic string loops in hopes of explaining the observed radio synchrotron background. After considering constraints from a variety of astrophysical and cosmological measurements, we identify a best-fit solution with string tension Gμ≃6.5×10-12 and current I≃2.5×106 GeV. This model yields a convincing fit to the data and may be testable in the near future by spectral distortion (TMS, BISOU) and 21 cm experiments (HERA, SKA, REACH). We also find that soft photon heating protects us against current constraints from global 21 cm experiments. © 2024 authors. Published by the American Physical Society.
Original languageEnglish
JournalPhysical Review D: Particles, Fields, Gravitation and Cosmology
Volume109
Issue number12
DOIs
Publication statusPublished - 4 Jun 2024

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