Topology change and nuclear symmetry energy in compact-star matter

Xiang-Hai Liu, Yong-Liang Ma, and Mannque Rho
Phys. Rev. C 99, 055808 – Published 10 May 2019

Abstract

We show that the cusplike structure in the nuclear symmetry energy, a consequence of topology change, visible in the skyrmion lattice description of dense matter, is extremely robust. It is present in the Skyrme model—with the pion field only—and is left unscathed by massive degrees of freedom such as the vector mesons ρ and ω and also the scalar meson introduced as a dilaton. It leads to the emergence of parity-doubling at the skyrmion–half-skyrmion transition and impacts on the nuclear symmetry energy “wilderness” landscape, weeding out roughly half of the wilderness. It is shown that a pseudoconformal sound velocity arises at a precocious density at which the cusp is formed. It is suggested that the topology change, being robust, could impact on the tidal deformability observed in gravity waves

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  • Received 7 January 2019

DOI:https://doi.org/10.1103/PhysRevC.99.055808

©2019 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Xiang-Hai Liu1, Yong-Liang Ma2,*, and Mannque Rho3,†

  • 1College of Physics, Jilin University, Changchun, 130012, China
  • 2Center for Theoretical Physics and College of Physics, Jilin University, Changchun, 130012, China
  • 3Institut de Physique Théorique, CEA Saclay, 91191 Gif-sur-Yvette Cédex, France

  • *yongliangma@jlu.edu.cn
  • mannque.rho@cea.fr

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Issue

Vol. 99, Iss. 5 — May 2019

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