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Correlation between the symmetry energy slope and the deconfinement phase transition

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arxiv 2311.00125 v2 pith:G3D5PI2I submitted 2023-10-31 hep-ph astro-ph.HEnucl-th

Luiz L. Lopes , Debora P. Menezes , Mateus R. Pelicer This is my paper · ORCID
classification hep-phastro-ph.HEnucl-th
keywords energyslopesymmetryphasestartransitionaffectamount
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abstract

We study how the nuclear symmetry energy slope ($L$) can affect the hadron-quark phase transition and neutron star properties. We show that the main physical quantities as the critical chemical potential and pressure are strongly influenced by the symmetry energy slope. In extreme cases, the total amount of deconfined quarks can reach up to 99$\%$ of the hybrid star mass.

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Cited by 1 Pith paper

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

  1. Impact of the Scalar Isovector $\delta$-meson on the description of nuclear matter and neutron star properties

    nucl-th 2024-12 conditional novelty 5.0 of 10

    Including the delta meson in relativistic mean-field models widens the allowed symmetry energy slope and curvature, changing low-mass neutron star radii while leaving maximum mass nearly fixed.

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