Chiral effects and Joule heating in hot and dense matter
arXiv:2510.00114 · doi:10.1103/4hch-nm2m
Abstract
Initial states of dense matter with nonzero electron chiral imbalance could potentially give rise to strong magnetic fields through chiral plasma instability. Previous work indicated that unless chiral chemical potential is as large as the electron vector chemical potential, the growth of magnetic fields due to the instability is washed out by chirality flipping rate enabled by electron mass. We re-examine this claim in a broader range of parameters and find that at higher temperatures the hierarchy is reversed supporting a growing magnetic field for an initial electron chiral chemical potential much smaller than the electron vector chemical potential. Further, we identify a qualitatively new effect relevant for magnetized hot and dense medium where chiral magnetic effect (CME) sourced by density fluctuation acts as a powerful source of Joule heating. Remarkably, even modest chiral chemical potentials (keV) in such environment can deposit energy densities set by the QCD scale in a relatively short time of the order of a few milliseconds or seconds. We speculate how this mechanism makes CME-driven Joule heating a potentially critical ingredient in the dynamics of turbulent density fluctuation of supernovae and neutron star mergers.
Matches published version
References in corpus (16)
- The Chiral Magnetic Effect
- Berry Curvature, Triangle Anomalies, and the Chiral Magnetic Effect in Fermi Liquids
- Charge separation induced by P-odd bubbles in QCD matter
- Neutrino-driven winds from neutron star merger remnants
- Gravitational Anomaly and Transport
- Chiral Magnetic Wave
- The Dynamics of Binary Neutron Star Mergers and of GW170817
- General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers
- Turbulent magnetic field amplification in binary neutron star mergers
- The Role of the Electron Mass in Damping Chiral Magnetic Instability in Supernova and Neutron Stars
- Thermal Effects in Binary Neutron Star Mergers
- Anomaly-driven inverse cascade and inhomogeneities in a magnetized chiral plasma in the early Universe
- Equilibration of the chiral asymmetry due to finite electron mass in electron-positron plasma
- Effective Chiral Magnetic Effect from Neutrino Radiation
- Photon radiation in hot nuclear matter by means of chiral anomalies
- Effect of Magnetic Fields on Urca Rates in Neutron Star Mergers