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arxiv 2202.09205 v2 pith:HONDOFI4 submitted 2022-02-18 astro-ph.HE hep-phnucl-th

Chiral plasma instability and inverse cascade from nonequilibrium left-handed neutrinos in core-collapse supernovae

classification astro-ph.HE hep-phnucl-th
keywords chiralmagneticneutrinoscurrentfieldsupernovaecascadecore-collapse
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We show that the backreaction of left-handed neutrinos out of equilibrium on the matter sector induces an electric current proportional to a magnetic field even without a chiral imbalance for electrons in core-collapse supernovae. We derive the transport coefficient of this effect based on the recently formulated chiral radiation transport theory for neutrinos. This chiral electric current generates a strong magnetic field via the so-called chiral plasma instability, which could provide a new mechanism for the strong and stable magnetic field of magnetars. We also numerically study the physical origin of the inverse cascade of the magnetic energy in the magnetohydrodynamics including this current. Our results indicate that incorporating the chiral effects of neutrinos would drastically modify the hydrodynamic evolutions of supernovae, which may also be relevant to the explosion dynamics.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Magnetar field dynamics driven by chiral anomalies without magnetic helicity

    astro-ph.HE 2026-05 unverdicted novelty 5.0

    Chiral magnetic effect generates magnetar-strength dipoles independently of initial net helicity via localized structures on decade timescales.

  2. Plasma heating during the chiral plasma instability

    hep-ph 2026-05 unverdicted novelty 5.0

    During chiral plasma instability, excess energy from chiral asymmetry heats the plasma with δT ~ μ5²/T instead of fully building the helical magnetic field.