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Is there a monopole problem?

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arxiv hep-ph/9507230 v2 pith:IK66HMBS submitted 1995-07-05 hep-ph astro-ph

Gia Dvali , Alejandra Melfo , Goran Senjanovic This is my paper · ORCID
classification hep-phastro-ph
keywords highmonopolesparametersrangetemperaturethereavoidingbehavior
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We investigate the high temperature behavior of SU(5) in its minimal version. We show that there exists a range of parameters of the Higgs potential for which the symmetry remains broken at high temperature, thus avoiding the phase transition that gives rise to the overproduction of monopoles . We also show that in such scenario the thermal production of monopoles can be suppressed in a wide range of parameters, keeping their number density below the cosmological limits.

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Cited by 3 Pith papers

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

  1. 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.

  2. Simulations of Magnetic Monopole Collisions

    hep-th 2025-02 conditional novelty 5.0 of 10

    Numerical field-theory simulations reproduce the predicted right-angle, 60-degree, and 45-degree scattering of BPS magnetic monopoles and show tetrahedral and cubic intermediate states.

  3. C-parity, magnetic monopoles and higher frequency gravitational waves

    hep-ph 2025-02 conditional novelty 4.0 of 10

    The C-string-wall network from SO(10) breaking with unbroken C-parity produces a gravitational wave background peaking between 100 Hz and 100 kHz for intermediate breaking scales around 10^10 to 10^12 GeV.

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