Physics of synchronized neutrino oscillations caused by self-interactions

Institute for Nuclear Research of the Academy of Sciences of Russia,60th October Anniversary Prospect 7a, Moscow 117312, Russia(February 5, 2002)In the early universe or in some regions of supernovae, the neutrino refractive index is dominated bythe neutrinosthemselves. Several previous studieshave found numerically that these self-interactionshave the effect of coupling different neutrino modes in such a way as to synchronize the flavoroscillations which otherwise would depend on the energy of a given mode. We provide a simpleexplanation for this baffling phenomenon in analogy to a system of magnetic dipoles which arecoupled by their self-interactions to form one large magnetic dipole which then precesses coherentlyin a weak external magnetic field. In this picture the synchronized neutrino oscillations are perfectlyanalogous to the weak-field Zeeman effect in atoms.PACS number(s): 14.60.Pq,I. INTRODUCTION

[1]  S. Petcov,et al.  Cosmological bounds on neutrino degeneracy improved by flavor oscillations , 2002, hep-ph/0201287.

[2]  P. Fishbane,et al.  Neutrino oscillations in matter of varying density , 2001, hep-ph/0101013.

[3]  N. Bell,et al.  Synchronisation and MSW sharpening of neutrinos propagating in a flavour blind medium , 2000, hep-ph/0011068.

[4]  S. Hannestad,et al.  On the Chaoticity of active-sterile neutrino oscillations in the early universe , 2000, hep-ph/0012194.

[5]  J. Pantaleone,et al.  Stability of incoherence in an isotropic gas of oscillating neutrinos , 1998 .

[6]  Samuel Bimodal coherence in dense self-interacting neutrino gases. , 1996, Physical review. D, Particles and fields.

[7]  Samuel,et al.  Neutrino oscillations in the early Universe with nonequilibrium neutrino distributions. , 1995, Physical review. D, Particles and fields.

[8]  Samuel,et al.  Self-maintained coherent oscillations in dense neutrino gases. , 1995, Physical review. D, Particles and fields.

[9]  Mckellar,et al.  Oscillating neutrinos in the early Universe. , 1994, Physical review. D, Particles and fields.

[10]  Samuel,et al.  Nonlinear neutrino oscillations in the expanding Universe. , 1994, Physical review. D, Particles and fields.

[11]  V. Kostelecký,et al.  Neutrino oscillations in the early Universe with an inverted neutrino-mass hierarchy , 1993, hep-ph/9610399.

[12]  J. Pantaleone,et al.  Neutrino oscillations in the early universe , 1993 .

[13]  Samuel,et al.  Neutrino oscillations in dense neutrino gases. , 1993, Physical review. D, Particles and fields.

[14]  G. Raffelt,et al.  General kinetic description of relativistic mixed neutrinos , 1993 .

[15]  J. Pantaleone Neutrino oscillations at high densities , 1992 .

[16]  Stodolsky Treatment of neutrino oscillations in a thermal environment. , 1987, Physical review. D, Particles and fields.

[17]  W. Hampel,et al.  Matter effects for solar neutrino oscillations , 1986 .

[18]  V. Tsarev,et al.  Buildup of Neutrino Oscillations in the Earth , 1986 .