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How generic is cosmic string formation in SUSY GUTs

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arxiv hep-ph/0308134 v1 pith:IFFMDJ42 submitted 2003-08-12 hep-ph astro-phgr-qchep-th

classification hep-phastro-phgr-qchep-th
keywords cosmicformationstringgaugeinflationbreakingformgroups
verification ladder T0 review T1 audit T2 compute T3 formal

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We study cosmic string formation within supersymmetric grand unified theories. We consider gauge groups having a rank between 4 and 8. We examine all possible spontaneous symmetry breaking patterns from the GUT down to the standard model gauge group. Assuming standard hybrid inflation, we select all the models which can solve the GUT monopole problem, lead to baryogenesis after inflation and are consistent with proton lifetime measurements. We conclude that in all acceptable spontaneous symmetry breaking schemes, cosmic string formation is unavoidable. The strings which form at the end of inflation have a mass which is proportional to the inflationary scale. Sometimes, a second network of strings form at a lower scale. Models based on gauge groups which have rank greater than 6 can lead to more than one inflationary era; they all end by cosmic string formation.

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Cited by 10 Pith papers

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

  1. Metastable cosmic strings are broken at the start

    hep-ph 2026-01 conditional novelty 7.0 of 10

    Metastable cosmic-string networks are typically broken within a Hubble time of formation by finite-temperature effects or by pre-existing monopoles, so matching NANOGrav requires m_M^2/μ ≳ 10^3.

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    hep-ph 2025-01 conditional novelty 7.0 of 10

    A general deformation function maps gravitational wave spectra from phase transitions during inflation into today's spectrum; for GUT-scale transitions the peak can appear near 10 Hz or mHz.

  3. Stochastic Gravitational Wave Background from Chiral Superconducting Cosmic Strings

    astro-ph.CO 2024-12 conditional novelty 6.0 of 10

    Superconducting cosmic string loops emit vector radiation whose strength is fitted in this paper; including this channel suppresses the predicted gravitational wave background for strong coupling and can make the spec...

  4. Probing the gravitational wave background from cosmic strings with LISA

    astro-ph.CO 2019-09 conditional novelty 6.0 of 10

    LISA is projected to probe cosmic string tensions G mu down to about 1e-17 and to measure spectral features from early-universe physics.

  5. Cosmic string gravitational wave backgrounds at LISA: II. Reconstruction of conventional signals over astrophysical foregrounds

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    When realistic astrophysical foregrounds are included, LISA can reconstruct the cosmic-string tension to 10% precision only for Gμ ≳ 10^{-11}, 10^5 times larger than foreground-free forecasts.

  6. Gravitational waves from cosmic strings with friction: analytical approximations and parameter space

    astro-ph.CO 2026-05 unverdicted novelty 5.0 of 10

    Analytical approximations for the ultra-high-frequency GW peak sourced by friction-era cosmic string loops, with expanded observable parameter space.

  7. Cosmological History of Flavour Deconstruction Models: Constraints from Monopole Production

    hep-ph 2026-05 unverdicted novelty 5.0 of 10

    Flavour deconstruction models with semi-simple gauge groups generically produce light monopoles that require low-scale reheating after inflation to satisfy cosmological and astrophysical bounds.

  8. Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison

    astro-ph.CO 2025-08 unverdicted novelty 5.0 of 10

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  9. Gravitational waves from metastable cosmic strings in the delayed scaling scenario

    astro-ph.CO 2025-01 conditional novelty 5.0 of 10

    Metastable cosmic strings with delayed scaling can explain the PTA gravitational wave background with tension up to Gmu ~ 3e-5 while evading LVK bounds, producing a plateau and an f^-1/3 tail detectable by future inte...

  10. Science Case for the Einstein Telescope

    astro-ph.CO 2019-12 unverdicted novelty 3.0 of 10

    The Einstein Telescope will enable gravitational-wave observations up to cosmological distances, opening avenues for discoveries in astrophysics, cosmology, and fundamental physics.

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