Neutrino propagation in an electron background with an inhomogeneous magnetic field

被引:4
作者
Nieves, Jose F. [1 ]
Sahu, Sarira [2 ,3 ]
机构
[1] Univ Puerto Rico, Dept Phys, Lab Theoret Phys, San Juan, PR 00936 USA
[2] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, A Postal 70-543, Mexico City 04510, DF, Mexico
[3] RIKEN, Astrophys Big Bang Lab, 2-1 Hirosawa, Wako, Saitama 3510198, Japan
来源
EUROPEAN PHYSICAL JOURNAL C | 2018年 / 78卷 / 07期
基金
日本学术振兴会;
关键词
ELECTROMAGNETIC-FIELDS; OSCILLATIONS; MATTER;
D O I
10.1140/epjc/s10052-018-6030-7
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study the electromagnetic coupling of a neutrino that propagates in a two-stream electron background medium. Specifically, we calculate the electromagnetic vertex function for a medium that consists of a normal electron background plus another electron stream background that is moving with a velocity four-vector v(mu) relative to the normal background. The results can be used as the basis for studying the neutrino electromagnetic properties and various processes in such a medium. As an application, we calculate the neutrino dispersion relation in the presence of an external magnetic field (B), focused in the case in which B is inhomogeneous, keeping only the terms of the lowest order in 1/m(W)(2) and linear in the B and its gradient. We show that the dispersion relation contains additional anisotropic terms involving the derivatives of B, such as the gradient of (k) over cap . (v x B), which involve the stream background velocity, and a term of the form (k) over cap . (del x B) that can be present in the absence of the stream background, in addition to a term of the form (k) over cap . v and the well known term (k) over cap . B that arises in the constant B case. The derivative-dependent terms are even under a CP transformation. As a result, in contrast to the latter two just mentioned, they depend on the sum of the particle and antiparticle densities and therefore can be non-zero in a CP-symmetric medium in which the particle and antiparticle densities are equal.
引用
收藏
页数:17
相关论文
共 39 条
  • [1] Pure quantum states of a neutrino with rotating spin in dense magnetized matter
    Arbuzova, E. V.
    Lobanov, A. E.
    Murchikova, E. M.
    [J]. PHYSICAL REVIEW D, 2010, 81 (04):
  • [2] Neutrino propagation in matter with general interactions
    Bergmann, S
    Grossman, Y
    Nardi, E
    [J]. PHYSICAL REVIEW D, 1999, 60 (09):
  • [3] COMPUTATIONS ON ANOMALOUS RESISTANCE
    BORIS, JP
    DAWSON, JM
    ORENS, JH
    ROBERTS, KV
    [J]. PHYSICAL REVIEW LETTERS, 1970, 25 (11) : 706 - &
  • [4] Nonlinear Development of Streaming Instabilities in Strongly Magnetized Plasma
    Che, H.
    Drake, J. F.
    Swisdak, M.
    Yoon, P. H.
    [J]. PHYSICAL REVIEW LETTERS, 2009, 102 (14)
  • [5] ELECTROMAGNETIC PROPERTIES OF NEUTRINOS IN A BACKGROUND OF ELECTRONS
    DOLIVO, JC
    NIEVES, JF
    PAL, PB
    [J]. PHYSICAL REVIEW D, 1989, 40 (11): : 3679 - 3687
  • [6] FINITE-TEMPERATURE CORRECTIONS TO THE EFFECTIVE POTENTIAL OF NEUTRINOS IN A MEDIUM
    DOLIVO, JC
    NIEVES, JF
    TORRES, M
    [J]. PHYSICAL REVIEW D, 1992, 46 (03): : 1172 - 1179
  • [7] Formation of electron holes and particle energization during magnetic reconnection
    Drake, JF
    Swisdak, M
    Cattell, C
    Shay, MA
    Rogers, BN
    Zeiler, A
    [J]. SCIENCE, 2003, 299 (5608) : 873 - 877
  • [8] Neutrino processes in strong magnetic fields and implications for supernova dynamics
    Duan, HY
    Qian, YZ
    [J]. PHYSICAL REVIEW D, 2004, 69 (12):
  • [9] Dvornikov M, 2014, JCAP, V1405
  • [10] Neutrino self-energy and dispersion in a medium with a magnetic field
    Erdas, A
    Kim, CW
    Lee, TH
    [J]. PHYSICAL REVIEW D, 1998, 58 (08)