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Charge Screening at First Order Phase Transitions and Hadron - Quark Mixed Phase

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arxiv nucl-th/0208067 v2 pith:ETPFHTT7 submitted 2002-08-29 nucl-th astro-phcond-mat

D. N. Voskresensky (Yukawa ITP , Kyoto , GSI , Darmstadt , MEPhI , Moscow) , M. Yasuhira (Yukawa ITP & Kyoto Univ. , Kyoto)
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T. Tatsumi (Kyoto Univ.
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classification nucl-thastro-phcond-mat
keywords phasemixedchargeelectricfirsthadronorderphases
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abstract

Possibility of structured mixed phases at first order phase transitions in neutron stars is re-examined by taking into account charge screening and surface effects. Transition from the hadron $npe$ phase to the quark phase is studied. Two possibilities, the mixed phase and two separate phases given by the double-tangent (Maxwell) construction are considered. Inhomogeneous profiles of the electric potential and their contribution to the energy are analytically calculated. The electric field configurations determine the droplet size and the geometry of structures.

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Cited by 4 Pith papers

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

  1. Distinct Signatures of the Nature of Phase Transition in Binary Neutron Star Mergers

    astro-ph.HE 2025-03 unverdicted novelty 6.0 of 10

    Simulations with a tunable phase-transition parameter in neutron-star equations of state produce unique post-merger gravitational-wave peaks and link Δp to the prompt-collapse mass threshold, with Δp ≲ 0.04 implied fo...

  2. Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    Using full general relativity, the authors compute f-mode oscillation frequencies for neutron stars with hyperons, delta baryons, and quark-matter cores, and find composition-dependent shifts in universal asteroseismo...

  3. Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?

    nucl-th 2024-12 conditional novelty 6.0 of 10

    Hybrid stars with color-superconducting quark matter can reproduce the mass and spin of pulsar J0952-0607, whereas the hadronic-only model cannot, and the revised Kepler-frequency relation tightens radius bounds.

  4. Phase transitions in neutron stars and their links to gravitational waves

    astro-ph.HE 2019-07 unverdicted novelty 2.0 of 10

    Review of neutron star dense matter, hadron-quark phase transitions, and potential g-mode signatures in gravitational waves from multimessenger observations.

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