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Cosmology with a TeV mass GUT Higgs
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abstract
The most natural way to break the GUT gauge symmetry is with a Higgs field whose vacuum expectation value is of order $10^{16}\,\mbox{GeV}$ but whose mass is of order $10^2$ to $10^3\,\mbox{GeV}$. This can lead to a cosmological history radically different from what is usually assumed to have occurred between the standard inflationary and nucleosynthesis epochs, which may solve the gravitino and Polonyi/moduli problems in a natural way.
Forward citations
Cited by 2 Pith papers
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Phase Transitions and Gravitational Wave Production at the End of Thermal Inflation
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What happens when supercooling is terminated by curvature flipping of the effective potential?
Supercooling terminated by curvature flipping still proceeds by bubble nucleation and expansion, not by smooth phase mixing, according to 3D lattice simulations.
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