During chiral plasma instability, excess energy from chiral asymmetry heats the plasma with δT ~ μ5²/T instead of fully building the helical magnetic field.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
fields
hep-ph 2years
2026 2verdicts
UNVERDICTED 2roles
background 2polarities
background 2representative citing papers
Time-dependent chiral magnetic conductivity modifies particle spectra and energy loss, implying polarized jets in quark-gluon plasma.
citing papers explorer
-
Plasma heating during the chiral plasma instability
During chiral plasma instability, excess energy from chiral asymmetry heats the plasma with δT ~ μ5²/T instead of fully building the helical magnetic field.
-
Quark and gluon production in the presence of the time-varying chiral magnetic current
Time-dependent chiral magnetic conductivity modifies particle spectra and energy loss, implying polarized jets in quark-gluon plasma.