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Cosmic Strings

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arxiv 1506.04039 v2 pith:4PAP2INZ submitted 2015-06-12 astro-ph.CO hep-phhep-th

Tanmay Vachaspati , Levon Pogosian , Daniele Steer This is my paper
classification astro-ph.COhep-phhep-th
keywords cosmicstringsarticlebriefcosmologicalevolutionintroductionmain
verification ladder T0 review T1 audit T2 compute T3 formal
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This article, written for Scolarpedia, provides a brief introduction into the subject of cosmic strings, together with a review of their main properties, cosmological evolution and observational signatures.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run

    gr-qc 2025-08 accept novelty 4.0 of 10

    No gravitational-wave background is detected in O1-O4a data; the new CBC-spectrum limit Ω_GW(25 Hz) = 2.0×10^-9 (95%) is 1.7x tighter and remains roughly 2-3x above the GWTC-4-predicted astrophysical background of 0.9×10^-9.

  2. Interpreting the KM3-230213A PeV Neutrino Event via Vector Dark Matter Decay and Its Multi-Messenger Signatures

    hep-ph 2025-07 conditional novelty 4.0 of 10

    A U(1)_X vector dark matter model explains the KM3-230213A PeV neutrino via DM decay and predicts a cosmic string gravitational wave background consistent with PTA observations, but with several parameters fitted to the data.

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