Designer bubble walls in a holographic Weyl semi-metal with magnetic field
Designer bubble walls in a holographic Weyl semi-metal with magnetic field
We study bubble walls in the holographic D3/probe D7 system that is dual to strongly coupled quark dynamics. We work to construct holographic descriptions of bubble wall junctions where we can tune the bubble wall height and pressure difference in a theory at zero temperature and density. We study the system in the presence of a background axial vector field b that induces a Weyl semi-metal, massless phase and a background magnetic field B which favours mass generation. We find a first order transition line in the mass-B plane, at fixed b, ending at a critical point. We present some preliminary solutions of PDEs that describe the motion of one dimensional bubble walls in this theory, with a stationary initial condition - large pressure differences accelerate the wall to the speed of light whilst when the pressure difference is small the wall slumps to an interpolating solution. We also take the first steps to include temperature and see evidence of thermal drag slowing the wall motion. Slump configurations at finite temperature show some signs of a back pressure wave against the wall motion.
hep-th
Evans, Nick
33dfbb52-64dd-4c1f-9cd1-074faf2be4b3
Fan, Wanxiang
26ec2421-45f6-4181-8d21-dc8aea1f8992
Evans, Nick
33dfbb52-64dd-4c1f-9cd1-074faf2be4b3
Fan, Wanxiang
26ec2421-45f6-4181-8d21-dc8aea1f8992
[Unknown type: UNSPECIFIED]
Abstract
We study bubble walls in the holographic D3/probe D7 system that is dual to strongly coupled quark dynamics. We work to construct holographic descriptions of bubble wall junctions where we can tune the bubble wall height and pressure difference in a theory at zero temperature and density. We study the system in the presence of a background axial vector field b that induces a Weyl semi-metal, massless phase and a background magnetic field B which favours mass generation. We find a first order transition line in the mass-B plane, at fixed b, ending at a critical point. We present some preliminary solutions of PDEs that describe the motion of one dimensional bubble walls in this theory, with a stationary initial condition - large pressure differences accelerate the wall to the speed of light whilst when the pressure difference is small the wall slumps to an interpolating solution. We also take the first steps to include temperature and see evidence of thermal drag slowing the wall motion. Slump configurations at finite temperature show some signs of a back pressure wave against the wall motion.
Text
2408.10835v1
- Author's Original
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Accepted/In Press date: 20 August 2024
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27 pages, 15 figures
Keywords:
hep-th
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Local EPrints ID: 497260
URI: http://eprints.soton.ac.uk/id/eprint/497260
PURE UUID: 44fa52dd-261b-4d89-8bfa-e935c3b1b127
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Date deposited: 16 Jan 2025 17:56
Last modified: 16 Jan 2025 17:56
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Author:
Wanxiang Fan
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