Detecting dark energy in long baseline neutrino oscillations
文献类型:期刊论文
作者 | Gu PH(顾佩洪); Bi XJ(毕效军)![]() ![]() ![]() ![]() |
刊名 | CHINESE PHYSICS C
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出版日期 | 2008 |
卷号 | 32期号:7页码:530-535 |
关键词 | dark energy neutrino oscillation |
通讯作者 | [Gu Pei-Hong ; Zhang Xin-Min] Chinese Acad Sci, IHEP, Div Theoret Phys, Beijing 100049, Peoples R China ; [Bi Xiao-Jun] Chinese Acad Sci, IHEP, Key Lab Particle Astrophys, Beijing 100049, Peoples R China ; [Feng Bo] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China ; [Feng Bo ; Young Bing-Lin] Univ Tokyo, Grad Sch Sci, Res Ctr Early Universe RESCEU, Tokyo 1130033, Japan ; [Young Bing-Lin] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA |
英文摘要 | In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type of models the scalar field is taken to be quintessence-like and for the other phantom-like. In these models the scalar fields couple to the neutrinos to give rise to spatially varying neutrino masses. We will show that the two types of models predict different behaviors of the spatial variation of the neutrino masses inside the Earth and consequently result in different signals in long baseline neutrino oscillation experiments. |
学科主题 | Physics |
类目[WOS] | Physics, Nuclear ; Physics, Particles & Fields |
研究领域[WOS] | Physics |
原文出处 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000265989400004 |
源URL | [http://ir.ihep.ac.cn/handle/311005/237842] ![]() |
专题 | 高能物理研究所_理论物理室 |
作者单位 | 中国科学院高能物理研究所 |
推荐引用方式 GB/T 7714 | Gu PH,Bi XJ,Zhang XM,et al. Detecting dark energy in long baseline neutrino oscillations[J]. CHINESE PHYSICS C,2008,32(7):530-535. |
APA | 顾佩洪.,毕效军.,张新民.,Gu, PH.,Bi, XJ.,...&Zhang, XM.(2008).Detecting dark energy in long baseline neutrino oscillations.CHINESE PHYSICS C,32(7),530-535. |
MLA | 顾佩洪,et al."Detecting dark energy in long baseline neutrino oscillations".CHINESE PHYSICS C 32.7(2008):530-535. |
入库方式: OAI收割
来源:高能物理研究所
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