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Strange quark mass turns magnetic domain walls into multi-winding flux tubes

Strange quark mass turns magnetic domain walls into multi-winding flux tubes
Strange quark mass turns magnetic domain walls into multi-winding flux tubes
Dense quark matter is expected to behave as a type-II superconductor at strong coupling. It was previously shown that if the strange quark mass ms is neglected, magnetic domain walls in the so-called 2SC phase are the energetically preferred magnetic defects in a certain parameter region. Computing the flux tube profiles and associated free energies within a Ginzburg–Landau approach, we find a cascade of multi-winding flux tubes as 'remnants' of the domain wall when ms is increased. These flux tubes exhibit an unconventional ring-like structure of the magnetic field. We show that flux tubes with winding numbers larger than one survive for values of ms up to about 20% of the quark chemical potential. This makes them unlikely to play a significant role in compact stars, but they may appear in the QCD phase diagram in the presence of an external magnetic field.
0954-3899
Evans, Geraint W.
d2dec11a-277e-4afa-95cd-b086bf164afa
Schmitt, Andreas
1765159f-255f-45e7-94ea-58c1c883d65f
Evans, Geraint W.
d2dec11a-277e-4afa-95cd-b086bf164afa
Schmitt, Andreas
1765159f-255f-45e7-94ea-58c1c883d65f

Evans, Geraint W. and Schmitt, Andreas (2021) Strange quark mass turns magnetic domain walls into multi-winding flux tubes. Journal of Physics G: Nuclear and Particle Physics, 24, [035002]. (doi:10.1088/1361-6471/abcb9d).

Record type: Article

Abstract

Dense quark matter is expected to behave as a type-II superconductor at strong coupling. It was previously shown that if the strange quark mass ms is neglected, magnetic domain walls in the so-called 2SC phase are the energetically preferred magnetic defects in a certain parameter region. Computing the flux tube profiles and associated free energies within a Ginzburg–Landau approach, we find a cascade of multi-winding flux tubes as 'remnants' of the domain wall when ms is increased. These flux tubes exhibit an unconventional ring-like structure of the magnetic field. We show that flux tubes with winding numbers larger than one survive for values of ms up to about 20% of the quark chemical potential. This makes them unlikely to play a significant role in compact stars, but they may appear in the QCD phase diagram in the presence of an external magnetic field.

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More information

Accepted/In Press date: 18 November 2020
e-pub ahead of print date: 21 January 2021
Published date: 26 January 2021

Identifiers

Local EPrints ID: 478038
URI: http://eprints.soton.ac.uk/id/eprint/478038
ISSN: 0954-3899
PURE UUID: 05370b56-06a6-4e42-9cac-55b0443a3409
ORCID for Geraint W. Evans: ORCID iD orcid.org/0000-0001-6106-4567
ORCID for Andreas Schmitt: ORCID iD orcid.org/0000-0003-2858-4450

Catalogue record

Date deposited: 21 Jun 2023 16:34
Last modified: 17 Mar 2024 03:40

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