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The evolution of vacuum states and phase transitions in 2HDM during cooling of Universe

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arxiv 0911.2383 v2 pith:4UPRTF2E submitted 2009-11-12 hep-ph

I.F. Ginzburg , I.P. Ivanov , K.A. Kanishev This is my paper · ORCID
classification hep-ph
keywords differentevolutioncoolingduringmodelparametersphasethermal
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We consider the evolution of the ground state in the Two Higgs Doublet Model during cooling down of the Universe after the Big Bang. Different regions in the space of free parameters of this model correspond to different sequences of thermal phase transitions. We discuss different paths of thermal evolution and corresponding evolution of physical properties of the system for different modern values of the parameters.

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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. Electroweak Baryogenesis: Advances in Sphaleron Rate Calculations and Implications of Thermal Phase Transitions

    hep-ph 2026-07 conditional novelty 5.0 of 10

    Sphaleron rates can be computed gauge-invariantly in 3D thermal EFT, yielding a new baryon-washout criterion x = lambda3/g3^2 that replaces v_c/T_c > 1 for electroweak baryogenesis.

  2. Goofy is the new Normal

    hep-ph 2025-04 conditional novelty 5.0 of 10

    Goofy transformations define new renormalization-group-stable parameter relations in the two-Higgs-doublet model that are not ordinary symmetries.

  3. BSM: Extended Scalar Sectors

    hep-ph 2025-07 unverdicted novelty 1.0 of 10

    An updated review chapter on extended scalar sectors, their constraints, dark matter and CP violation links, and future collider searches.

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