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Thermal background can solve the cosmological moduli problem

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arxiv hep-ph/0601067 v4 pith:H3BQBW2H submitted 2006-01-10 hep-ph

Jun'ichi Yokoyama This is my paper
classification hep-ph
keywords modulicosmologicalfieldsproblemthermalbackgroundbosoniccoherent
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It is shown that the coherent field oscillation of moduli fields with weak or TeV scale masses can dissipate its energy efficiently if they have a derivative coupling to standard bosonic fields in a thermal state. This mechanism may provide a new solution to the cosmological moduli problem in some special situations.

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  1. Gravitational Waves from Multiple First-Order Phase Transitions in a Scenario with Early Matter Domination

    hep-ph 2026-07 unverdicted novelty 4.0 of 10

    Early matter domination with time-dependent decay rates produces multiple first-order phase transitions whose gravitational wave signatures encode the transition and reheating temperatures.

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