Built on

L. Wolfenstein, “Neutrino Oscillations In Matter,” Phys. Rev. D 17
1985
Earlier work this paper cites.
R. F. Sawyer, “Neutrino oscillations in inhomogeneous matter,” Phys. Rev. D 42
1990
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.
Y. Z. Qian and G. M. Fuller, “Neutrino-neutrino scattering and matter enhanced neutrino flavor transformation in Supernovae,” Phys. Rev. D 51
1995
Earlier work this paper cites.
S. Samuel, “Bimodal coherence in dense selfinteracting neutrino gases,” Phys. Rev. D 53
1996
Earlier work this paper cites.
R. F. Sawyer, “Speed-up of neutrino transformations in a supernova environment,” Phys. Rev. D 72
2005
Earlier work this paper cites.
P. Strack and A. Burrows, “Generalized Boltzmann formalism for oscillating neutrinos,” Phys. Rev. D 71
2005
Earlier work this paper cites.
H. Duan, G. M. Fuller, J. Carlson and Y. -Z. Qian, “Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the Supernova Environment. 1. Correlated Neutrino Trajectories,” Phys. Rev. D 74
2006
Earlier work this paper cites.

Similar

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
Cited alongside, same era.
H. Duan, G. M. Fuller and Y. -Z. Qian, “A Simple Picture for Neutrino Flavor Transformation in Supernovae,” Phys. Rev. D 76
Original
2007
Cited alongside, same era.
A. Esteban-Pretel, S. Pastor, R. Tomàs, G. G. Raffelt and G. Sigl, “Decoherence in supernova neutrino transformations suppressed by deleptonization,” Phys. Rev. D 76
Original
2007
Cited alongside, same era.
G. G. Raffelt and G. Sigl, “Self-induced decoherence in dense neutrino gases,” Phys. Rev. D 75
2007
Cited alongside, same era.
G. G. Raffelt and A. Y. .Smirnov, “Self-induced spectral splits in supernova neutrino fluxes,” Phys. Rev. D 76
Original

Then

J. F. Cherry, J. Carlson, A. Friedland, G. M. Fuller and A. Vlasenko, “Neutrino scattering and flavor transformation in supernovae,” Phys. Rev. Lett. 108
Original
2012
Later among the works it cites.
S. Sarikas, I. Tamborra, G. Raffelt, L. Hudepohl and H. -T. Janka, “Supernova neutrino halo and the suppression of self-induced flavor conversion,” Phys. Rev. D 85
Original
2012
Later among the works it cites.
G. Raffelt, S. Sarikas and D. d. S. Seixas, “Axial symmetry breaking in self-induced flavor conversion of supernova neutrino fluxes,” Phys. Rev. Lett. 111
Original
2013
Later among the works it cites.
G. Raffelt and D. d. S. Seixas, “Neutrino flavor pendulum in both mass hierarchies,” Phys. Rev. D 88
Original
2013
Later among the works it cites.
H. Duan, “Flavor Oscillation Modes In Dense Neutrino Media,” Phys. Rev. D 88

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2014

Damping the neutrino flavor pendulum by breaking homogeneity

Mangano, Gianpiero, Mirizzi, Alessandro, Saviano, Ninetta

Understand

The most general case of self-induced neutrino flavor evolution is described by a set of kinetic equations for a dense neutrino gas evolving both in space and time.

Solutions of these equations have been typically worked out assuming that either the time (in the core-collapse supernova environment) or space (in the early universe) homogeneity in the initial conditions is preserved through the evolution.
In these cases one can gauge away the homogeneous variable and reduce the dimensionality of the problem.
In this paper we investigate if small deviations from an initial postulated homogeneity can be amplified by the interacting neutrino gas, leading to a new flavor instability.

Built on

L. Wolfenstein, “Neutrino Oscillations In Matter,” Phys. Rev. D 17
1985
Earlier work this paper cites.
R. F. Sawyer, “Neutrino oscillations in inhomogeneous matter,” Phys. Rev. D 42
1990
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.
Y. Z. Qian and G. M. Fuller, “Neutrino-neutrino scattering and matter enhanced neutrino flavor transformation in Supernovae,” Phys. Rev. D 51
1995
Earlier work this paper cites.
S. Samuel, “Bimodal coherence in dense selfinteracting neutrino gases,” Phys. Rev. D 53
1996
Earlier work this paper cites.
R. F. Sawyer, “Speed-up of neutrino transformations in a supernova environment,” Phys. Rev. D 72
2005
Earlier work this paper cites.
P. Strack and A. Burrows, “Generalized Boltzmann formalism for oscillating neutrinos,” Phys. Rev. D 71
2005
Earlier work this paper cites.
H. Duan, G. M. Fuller, J. Carlson and Y. -Z. Qian, “Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the Supernova Environment. 1. Correlated Neutrino Trajectories,” Phys. Rev. D 74
2006
Earlier work this paper cites.