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Strong-field magnetohydrodynamics for neutron stars
ID Vardhan, Shreya (Author), ID Grozdanov, Sašo (Author), ID Leutheusser, Samuel (Author), ID Liu, Hong (Author)

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Abstract
We present a formulation of magnetohydrodynamics which can be used to describe the evolution of strong magnetic fields in neutron star interiors. Our approach is based on viewing magnetohydrodynamics as a theory with a one-form global symmetry and developing an effective field theory for the hydrodynamic modes associated with this symmetry. In the regime where the local velocity and temperature variations can be neglected, we derive the most general constitutive relation consistent with symmetry constraints for the electric field in the presence of a strong magnetic field. This constitutive relation not only reproduces the phenomena of Ohmic decay, ambipolar diffusion, and Hall drift derived in a phenomenological model by Goldreich and Reisenegger, but also reveals terms in the evolution of the magnetic field which cannot easily be seen from such microscopic models. This formulation gives predictions for diffusion behaviors of small perturbations around a constant background magnetic field, and for the two-point correlation functions among various components of the electric and magnetic fields.

Language:English
Keywords:magnetohydrodynamics, magnetic field, neutron stars, effective field theory, diffusion
Work type:Article
Typology:1.01 - Original Scientific Article
Organization:FMF - Faculty of Mathematics and Physics
Publication status:Published
Publication version:Version of Record
Year:2024
Number of pages:Str. L042050-1-L042050-12
Numbering:Vol. 6, iss. 4
PID:20.500.12556/RUL-165227 This link opens in a new window
UDC:537
ISSN on article:2643-1564
DOI:10.1103/PhysRevResearch.6.L042050 This link opens in a new window
COBISS.SI-ID:216651779 This link opens in a new window
Publication date in RUL:27.11.2024
Views:443
Downloads:140
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Record is a part of a journal

Title:Physical review research
Publisher:American Phyisical Society
ISSN:2643-1564
COBISS.SI-ID:32822823 This link opens in a new window

Licences

License:CC BY 4.0, Creative Commons Attribution 4.0 International
Link:http://creativecommons.org/licenses/by/4.0/
Description:This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.

Secondary language

Language:Slovenian
Keywords:magnetohidrodinamika, magnetno polje, nevtronske zvezde, efektivna teorija polja, difuzija

Projects

Funder:UKRI - UK Research and Innovation
Project number:ST/T00388X/1
Name:From quantum chaos to collective transport in plasmas

Funder:ARIS - Slovenian Research and Innovation Agency
Project number:P1-0402-2019
Name:Matematična fizika

Funder:ARIS - Slovenian Research and Innovation Agency
Project number:N1-0245-2021
Name:Kvantni kaos v relativističnih plazmah

Funder:Other - Other funder or multiple funders
Funding programme:US Department of Energy
Project number:DE-SC0012567

Funder:Other - Other funder or multiple funders
Funding programme:US Department of Energy
Project number:DE-SC0020360

Funder:Other - Other funder or multiple funders
Funding programme:Natural Sciences and Engineering Research Council of Canada

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