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Bubble wall velocity and gravitational wave in the minimal left-right symmetric model

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arxiv 2405.01949 v2 pith:U6D5ONFB submitted 2024-05-03 gr-qc astro-ph.COhep-ph

classification gr-qcastro-ph.COhep-ph
keywords velocitywallfirstfoundgravitationalorderphasetransition
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abstract

The bubble wall velocity in the first order phase transition plays an important role in determining both the amplitude and the pivot frequency of stochastic gravitational wave background. In the framework of the minimal left-right symmetric model, we study the wall velocity when the first order phase transition can occur. The wall velocity can be determined by matching the distribution functions in the free particle approximation and the local thermal equilibrium approximation. It is found that the wall velocity can be determined in the range $ 0.2 < v_w < 0.5 $ for the parameter space with the first order phase transition. It is also found that for the case when the wall velocity is close to the speed of sound, the peak amplitude of gravitational wave spectrum can be larger than that in the runaway case. Moreover, It is also found that there exists an approximate power law between the wall velocity and pressure difference between broken and symmetry phases, and the power index is equal to 0.41 or so.

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Forward citations

Cited by 6 Pith papers

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

  1. Multi-step Strong First-Order Electroweak Phase Transitions in the Inverted Type-I 2HDM: Parameter Space, Gravitational Waves, and Collider Phenomenology

    hep-ph 2025-06 conditional novelty 7.0 of 10

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  2. Bubble wall dynamics from nonequilibrium quantum field theory

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  4. Loop-Level Lepton Flavor Violation and Diphoton Signals in the Minimal Left-Right Symmetric Model

    hep-ph 2025-12 conditional novelty 6.0 of 10

    Recasting axion limits onto the one-loop H3 couplings of the minimal left-right symmetric model excludes the right-handed scale up to 2×10^9 GeV and could eventually probe 6×10^11 GeV.

  5. Electroweak Phase Transition and Bubble Wall Velocity in Local Thermal Equilibrium

    hep-ph 2025-04 conditional novelty 6.0 of 10

    Bubble wall velocities in local thermal equilibrium are computed for three BSM models and found to be nearly universal when expressed via the critical temperature and supercooling, with only deflagration solutions.

  6. The Bubble Wall Velocity in Local Thermal Equilibrium and Energy Budget with Full Effective Potential

    hep-ph 2025-05 conditional novelty 5.0 of 10

    Using the full one-loop effective potential with the LTE approximation, the authors find that for xSM deflagration, bag-model gravitational wave peak predictions can differ by up to 48% in frequency and 90% in amplitu...

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