Built on

S. W. Bruenn, Stellar core collapse: Numerical model and infall epoch, Astrophys. J. Suppl. 58
1985
Earlier work this paper cites.
G. M. Fuller, R. W. Mayle, J. R. Wilson, and D. N. Schramm, Resonant neutrino oscillations and stellar collapse, Astrophys. J. 322
1987
Earlier work this paper cites.
D. Notzold and G. Raffelt, Neutrino Dispersion at Finite Temperature and Density, Nucl. Phys. B 307
1988
Earlier work this paper cites.
J. T. Pantaleone, Dirac neutrinos in dense matter, Phys. Rev. D 46
1992
Earlier work this paper cites.
S. Samuel, Neutrino oscillations in dense neutrino gases, Phys. Rev. D 48
1993
Earlier work this paper cites.
G. Sigl and G. Raffelt, General kinetic description of relativistic mixed neutrinos, Nucl. Phys. B 406
1993
Earlier work this paper cites.
S. Pastor and G. Raffelt, Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background, Phys. Rev. Lett. 89
2002
Earlier work this paper cites.
G. Raffelt, G. Sigl, and L. Stodolsky, NonAbelian Boltzmann equation for mixing and decoherence, Phys. Rev. Lett. 70
2007
Earlier work this paper cites.
S. Hannestad, G. G. Raffelt, G. Sigl, and Y. Y. Y. Wong, Self-induced conversion in dense neutrino gases: Pendulum in flavour space, Phys. Rev. D 74
2007
Earlier work this paper cites.

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2022

Collisional flavor instability in dense neutrino gases

Xiong, Zewei, Johns, Lucas, Wu, Meng-Ru et al.

Understand

Charged-current neutrino processes such as $\nu_e + n \rightleftharpoons p + e^-$ and $\bar\nu_e + p \rightleftharpoons n + e^+$ destroy the flavor coherence among the weak-interaction states of a single neutrino and thus damp its flavor oscillation.

In a dense neutrino gas such as that inside a core-collapse supernova or the black hole accretion disk formed in a compact binary merger, however, these "collision" processes can trigger large flavor conversion in cooperation with the strong neutrino-neutrino refraction.
We show that there exist two types of collisional flavor instability in a homogeneous and isotropic neutrino gas which are identified by the dependence of their real frequencies on the neutrino density $n_\nu$.
The instability transitions from one type to the other and exhibits a resonance-like behavior in the region where the net electron lepton number of the neutrino gas is negligible.

Built on

S. W. Bruenn, Stellar core collapse: Numerical model and infall epoch, Astrophys. J. Suppl. 58
1985
Earlier work this paper cites.
G. M. Fuller, R. W. Mayle, J. R. Wilson, and D. N. Schramm, Resonant neutrino oscillations and stellar collapse, Astrophys. J. 322
1987
Earlier work this paper cites.
D. Notzold and G. Raffelt, Neutrino Dispersion at Finite Temperature and Density, Nucl. Phys. B 307
1988
Earlier work this paper cites.
J. T. Pantaleone, Dirac neutrinos in dense matter, Phys. Rev. D 46
1992
Earlier work this paper cites.
S. Samuel, Neutrino oscillations in dense neutrino gases, Phys. Rev. D 48
1993
Earlier work this paper cites.
G. Sigl and G. Raffelt, General kinetic description of relativistic mixed neutrinos, Nucl. Phys. B 406
1993
Earlier work this paper cites.
S. Pastor and G. Raffelt, Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background, Phys. Rev. Lett. 89
2002
Earlier work this paper cites.
G. Raffelt, G. Sigl, and L. Stodolsky, NonAbelian Boltzmann equation for mixing and decoherence, Phys. Rev. Lett. 70
2007
Earlier work this paper cites.
S. Hannestad, G. G. Raffelt, G. Sigl, and Y. Y. Y. Wong, Self-induced conversion in dense neutrino gases: Pendulum in flavour space, Phys. Rev. D 74
2007
Earlier work this paper cites.