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Phase Boundary of Nuclear Matter in Magnetic Field

Phase Boundary of Nuclear Matter in Magnetic Field

来源:Arxiv_logoArxiv
英文摘要

Nuclear matter with a strong magnetic field is prevalent inside neutron stars and heavy-ion collisions. In a sufficiently large magnetic field the ground state is either a chiral soliton lattice (CSL), an array of solitons of the neutral pion field, or a domain-wall Skyrmion phase in which Skyrmions emerge inside the chiral solitons. In the region of large chemical potential and a magnetic field lower than its critical value for CSL, a Skyrmion crystal is expected to take up the ground state based on the chiral perturbation theory at the next leading order. We determine the phase boundary between such a Skyrmion crystal and the QCD vacuum. There was a conjecture that a magnetic field deforms the Skyrmion into a pancake shape whose boundary is a superconducting ring of charged pions. In contrast, through the exact Skyrmion solution, we find that the pancake conjecture holds approximately in a strong magnetic field, but fails for a weak one. We also validate that a Skyrmion would shrink to null without the Skyrme term, although Derrick's scaling law is modified by a background magnetic field, and the stability at the leading order is not ruled out in theory.

Yuki Amari、Muneto Nitta、Zebin Qiu

物理学

Yuki Amari,Muneto Nitta,Zebin Qiu.Phase Boundary of Nuclear Matter in Magnetic Field[EB/OL].(2025-04-11)[2025-05-03].https://arxiv.org/abs/2504.08379.点此复制

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