Classical mode conversion description of neutrino oscillations in dense magnetized plasmas

R Bingham; LO Silva; Robert Alan Cairns; VB Semikoz; VN Oraevsky

doi:10.1063/1.1625937

Classical mode conversion description of neutrino oscillations in dense magnetized plasmas

R Bingham, LO Silva, Robert Alan Cairns, VB Semikoz, VN Oraevsky

Applied Mathematics

Research output: Contribution to journal › Article › peer-review

Abstract

Neutrino oscillations in dense magnetized plasmas, similar to those found in supernovas, are described. The adopted model is similar to the classical mode conversion problems examined in fluid dynamics and plasma physics. This approach allows for the derivation of analytical results for the neutrino conversion probability for different combinations of background density profile and magnetic field profile. (C) 2003 American Institute of Physics.

Original language	English
Pages (from-to)	4903-4906
Number of pages	4
Journal	Physics of Plasmas
Volume	10
Issue number	12
DOIs	https://doi.org/10.1063/1.1625937
Publication status	Published - Dec 2003

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EARLY UNIVERSE
FIELD

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10.1063/1.1625937

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title = "Classical mode conversion description of neutrino oscillations in dense magnetized plasmas",

abstract = "Neutrino oscillations in dense magnetized plasmas, similar to those found in supernovas, are described. The adopted model is similar to the classical mode conversion problems examined in fluid dynamics and plasma physics. This approach allows for the derivation of analytical results for the neutrino conversion probability for different combinations of background density profile and magnetic field profile. (C) 2003 American Institute of Physics.",

keywords = "EARLY UNIVERSE, FIELD",

author = "R Bingham and LO Silva and Cairns, {Robert Alan} and VB Semikoz and VN Oraevsky",

year = "2003",

month = dec,

doi = "10.1063/1.1625937",

language = "English",

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publisher = "American Institute of Physics",

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AU - Bingham, R

AU - Silva, LO

AU - Cairns, Robert Alan

AU - Semikoz, VB

AU - Oraevsky, VN

PY - 2003/12

Y1 - 2003/12

N2 - Neutrino oscillations in dense magnetized plasmas, similar to those found in supernovas, are described. The adopted model is similar to the classical mode conversion problems examined in fluid dynamics and plasma physics. This approach allows for the derivation of analytical results for the neutrino conversion probability for different combinations of background density profile and magnetic field profile. (C) 2003 American Institute of Physics.

AB - Neutrino oscillations in dense magnetized plasmas, similar to those found in supernovas, are described. The adopted model is similar to the classical mode conversion problems examined in fluid dynamics and plasma physics. This approach allows for the derivation of analytical results for the neutrino conversion probability for different combinations of background density profile and magnetic field profile. (C) 2003 American Institute of Physics.

KW - EARLY UNIVERSE

KW - FIELD

U2 - 10.1063/1.1625937

DO - 10.1063/1.1625937

M3 - Article

SN - 1070-664X

VL - 10

SP - 4903

EP - 4906

JO - Physics of Plasmas

JF - Physics of Plasmas

IS - 12

ER -

Classical mode conversion description of neutrino oscillations in dense magnetized plasmas

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