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Imprints of Early Universe on Gravitational Waves from First-Order Phase Transition in QCD

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arxiv 1812.09676 v1 pith:C2E7TBFR submitted 2018-12-23 hep-th hep-ph

Meng-Wei Li , Yi Yang , Pei-Hung Yuan This is my paper · ORCID
classification hep-thhep-ph
keywords phasegravitationalspectrumchemicalquarktransitionwavecases
verification ladder T0 review T1 audit T2 compute T3 formal
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We study the gravitational wave spectrum from the confinement-deconfinement phase transi-tion in the holographic QCD models for both light quark and heavy quark. We obtain the gravitationalwave spectrum in the deflagration, detonation and runaway cases for different chemical potentials and duration of the phase transition. We find that the gravitational wave spectrum could be observed by EPTA/IPTA and eLISA for large chemical potential and short duartion of phase transtions.

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Cited by 2 Pith papers

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

  1. Finite temperature QCD crossover at non-zero chemical potential: A Dyson-Schwinger approach

    hep-ph 2025-02 conditional novelty 6.0 of 10

    An analytic Dyson-Schwinger derivation yields Tc(mu_B) for QCD; after fitting one scale to kappa2, the predicted kappa4 agrees with lattice.

  2. Unveiling the Gravitational Universe at \mu-Hz Frequencies

    astro-ph.IM 2019-08 unverdicted novelty 5.0 of 10

    Proposal for a μ-Hz space-based gravitational wave interferometer to observe massive black hole binaries in early inspiral and low-frequency galactic binaries.

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