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On the nature of the electroweak phase transition

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arxiv hep-ph/9212248 v4 pith:6YYGMR6G submitted 1992-12-10 hep-ph hep-th

classification hep-phhep-th
keywords contributionsdiscusselectroweaknaturephasetransitionapproachesapproximations
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abstract

We discuss the finite-temperature effective potential of the Standard Model, $\veff$, with emphasis on the resummation of the most important infrared contributions. We compute the one-loop scalar and vector boson self-energies in the zero-momentum limit. By solving the corresponding set of gap equations, with the inclusion of subleading contributions, we find a non-vanishing magnetic mass for the $SU(2)$ gauge bosons. We comment on its possible implications for the nature of the electroweak phase transition. We also discuss the range of validity of our approximations and compare this with other approaches.

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Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 108 citations worldwide. Full citation record

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    In the inverted Type-I 2HDM, one-step and two-step strong first-order electroweak phase transitions live in largely separate parameter regions, and LISA-detectable gravitational wave signals come predominantly from th...

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  3. Cosmological phase transitions from the functional measure

    hep-ph 2025-02 conditional novelty 6.0 of 10

    In the minimal modified functional measure model, a logarithmic scalar-potential correction can make the electroweak transition strongly first order, and future gravitational-wave observatories could probe the Higgs t...

  4. Primordial Gravitational Waves from Phase Transitions during Reheating

    astro-ph.CO 2025-06 conditional novelty 5.0 of 10

    Phase transitions happening during reheating can produce gravitational-wave signals that are delayed, prolonged, and shifted in amplitude and frequency by orders of magnitude compared with standard cosmology.

  5. Gauge-independent Gravitational Waves from Cogenesis in a $B-L$ Conserving Universe

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    In a B-L conserving SM extension with U(1)_x dark sector, CP-violating Yukawas generate opposite lepton asymmetries in visible and hidden sectors that sphalerons convert to baryon asymmetry, with gauge-independent bub...

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