中国物理B ›› 2006, Vol. 15 ›› Issue (1): 229-231.doi: 10.1088/1009-1963/15/1/038

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Mass neutrino oscillations in Robertson--Walker space--time

李泽军1, 黄秀菊2, 王永久2   

  1. (1)Department of Physics and Electronics, Hunan University of Arts and Science, Changde 415000, China; (2)Institute of Physics, Hunan Normal University, Changsha 410081, China
  • 收稿日期:2005-03-29 修回日期:2005-09-01 出版日期:2006-01-20 发布日期:2006-01-20
  • 基金资助:
    Project supported by the State Key Development Program for Basic Research of China (Grant No2003CB716300).

Mass neutrino oscillations in Robertson--Walker space--time

Huang Xiu-Ju (黄秀菊)a, Li Ze-Jun (李泽军)b, Wang Yong-Jiu (王永久)a   

  1. a Institute of Physics, Hunan Normal University, Changsha 410081, China; b Department of Physics and Electronics, Hunan University of Arts and Science, Changde 415000, China
  • Received:2005-03-29 Revised:2005-09-01 Online:2006-01-20 Published:2006-01-20
  • Supported by:
    Project supported by the State Key Development Program for Basic Research of China (Grant No2003CB716300).

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摘要： Along the geodesic we calculate the interference phase of the mass neutrinos propagating in the radial direction in Robertson--Walker space--time. Since our universe is expanding, the phase factor Ph is increasing under the condition of the same proper physical distance l. Different values of curvature parameter k in Robertson--Walker metric represent different cosmological models, correspondingly, we obtain the different interference phases.

关键词: interference phase, mass neutrino, Robertson--Walker space--time

Abstract: Along the geodesic we calculate the interference phase of the mass neutrinos propagating in the radial direction in Robertson--Walker space--time. Since our universe is expanding, the phase factor $\varPhi$ is increasing under the condition of the same proper physical distance l. Different values of curvature parameter k in Robertson--Walker metric represent different cosmological models, correspondingly, we obtain the different interference phases.

Key words: interference phase, mass neutrino, Robertson--Walker space--time

中图分类号:  (Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc))

  • 98.80.Es
98.80.Cq (Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)) 14.60.Pq (Neutrino mass and mixing) 14.60.Lm (Ordinary neutrinos)