Chiral magnetic effect generates magnetar-strength dipoles independently of initial net helicity via localized structures on decade timescales.
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During chiral plasma instability, excess energy from chiral asymmetry heats the plasma with δT ~ μ5²/T instead of fully building the helical magnetic field.
Time-dependent chiral magnetic conductivity modifies particle spectra and energy loss, implying polarized jets in quark-gluon plasma.
citing papers explorer
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Magnetar field dynamics driven by chiral anomalies without magnetic helicity
Chiral magnetic effect generates magnetar-strength dipoles independently of initial net helicity via localized structures on decade timescales.
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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.
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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.