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  • Letter

Vector interactions inhibit quark-hadron mixed phases in neutron stars

G. Lugones1 and A. G. Grunfeld2,3

  • 1Universidade Federal do ABC, Centro de Ciências Naturais e Humanas, Avenida dos Estados 5001- Bangú, CEP 09210-580, Santo André, SP, Brazil
  • 2CONICET, Godoy Cruz 2290, Buenos Aires, Argentina
  • 3Departamento de Física, Comisión Nacional de Energía Atómica, Avenida Libertador 8250, (1429) Buenos Aires, Argentina

Phys. Rev. D 104, L101301 – Published 17 November, 2021

DOI: https://doi.org/10.1103/PhysRevD.104.L101301

Abstract

We investigate the surface tension σ and the curvature energy γ of quark matter drops in the MIT bag model with vector interactions. Finite size corrections to the density of states are implemented by using the multiple reflection expansion (MRE) formalism. We find that σ and γ are strongly enhanced by new terms arising from vector interactions. With respect to the noninteracting case they are increased by a large factor, which can be as high as ∼10 when the vector coupling constant g varies within the range used in the literature. This behavior may have major consequences for the hadron-quark mixed phase speculated to exist at neutron star (NS) interiors, which may be totally suppressed or have its extension substantially reduced.

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