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Title: Electron-muon heat conduction in neutron star cores via the exchange of transverse plasmons

Abstract

We calculate the thermal conductivity of electrons and muons {kappa}{sub e{mu}} produced due to electromagnetic interactions of charged particles in neutron star cores and show that these interactions are dominated by the exchange of transverse plasmons (via the Landau damping of these plasmons in nonsuperconducting matter and via a specific plasma screening in the presence of proton superconductivity). For normal protons, the Landau damping strongly reduces {kappa}{sub e{mu}} and makes it temperature independent. Proton superconductivity suppresses the reduction and restores the Fermi-liquid behavior {kappa}{sub e{mu}}{proportional_to}T{sup -1}. Comparing with the thermal conductivity of neutrons {kappa}{sub n}, we obtain {kappa}{sub e{mu}} > or approx. {kappa}{sub n} for T > or approx. 2x10{sup 9} K in normal matter and for any T in superconducting matter with proton critical temperatures T{sub cp} > or approx. 3x10{sup 9} K. The results are described by simple analytic formulae.

Authors:
;  [1]
  1. Ioffe Physico-Technical Institute, Politekhnicheskaya 26, 194021 St. Petersburg (Russian Federation)
Publication Date:
OSTI Identifier:
20935247
Resource Type:
Journal Article
Resource Relation:
Journal Name: Physical Review. D, Particles Fields; Journal Volume: 75; Journal Issue: 10; Other Information: DOI: 10.1103/PhysRevD.75.103004; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; CHARGED PARTICLES; CRITICAL TEMPERATURE; ELECTROMAGNETIC INTERACTIONS; ELECTRONS; FERMI GAS; LANDAU DAMPING; MATTER; MUONS; NEUTRON STARS; NEUTRONS; PLASMA; PLASMONS; PROTONS; SUPERCONDUCTIVITY; THERMAL CONDUCTION; THERMAL CONDUCTIVITY

Citation Formats

Shternin, P. S., and Yakovlev, D. G.. Electron-muon heat conduction in neutron star cores via the exchange of transverse plasmons. United States: N. p., 2007. Web. doi:10.1103/PHYSREVD.75.103004.
Shternin, P. S., & Yakovlev, D. G.. Electron-muon heat conduction in neutron star cores via the exchange of transverse plasmons. United States. doi:10.1103/PHYSREVD.75.103004.
Shternin, P. S., and Yakovlev, D. G.. Tue . "Electron-muon heat conduction in neutron star cores via the exchange of transverse plasmons". United States. doi:10.1103/PHYSREVD.75.103004.
@article{osti_20935247,
title = {Electron-muon heat conduction in neutron star cores via the exchange of transverse plasmons},
author = {Shternin, P. S. and Yakovlev, D. G.},
abstractNote = {We calculate the thermal conductivity of electrons and muons {kappa}{sub e{mu}} produced due to electromagnetic interactions of charged particles in neutron star cores and show that these interactions are dominated by the exchange of transverse plasmons (via the Landau damping of these plasmons in nonsuperconducting matter and via a specific plasma screening in the presence of proton superconductivity). For normal protons, the Landau damping strongly reduces {kappa}{sub e{mu}} and makes it temperature independent. Proton superconductivity suppresses the reduction and restores the Fermi-liquid behavior {kappa}{sub e{mu}}{proportional_to}T{sup -1}. Comparing with the thermal conductivity of neutrons {kappa}{sub n}, we obtain {kappa}{sub e{mu}} > or approx. {kappa}{sub n} for T > or approx. 2x10{sup 9} K in normal matter and for any T in superconducting matter with proton critical temperatures T{sub cp} > or approx. 3x10{sup 9} K. The results are described by simple analytic formulae.},
doi = {10.1103/PHYSREVD.75.103004},
journal = {Physical Review. D, Particles Fields},
number = 10,
volume = 75,
place = {United States},
year = {Tue May 15 00:00:00 EDT 2007},
month = {Tue May 15 00:00:00 EDT 2007}
}
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