Parameters in a class of leptophilic dark matter models from PAMELA, ATIC and FERMI | |
Bi XJ(毕效军)![]() ![]() | |
2009 | |
发表期刊 | PHYSICS LETTERS B (IF:4.807[JCR-2016],4.327[5-Year]) |
卷号 | 678期号:2页码:#REF! |
通讯作者 | He, XG (reprint author), Natl Taiwan Univ, Dept Phys, Ctr Theoret Sci, Taipei, Taiwan. |
文章类型 | Article |
摘要 | In this work we study a class of leptophilic dark matter models, where the dark matter interacts with the standard model particles via the U(1)L(i)-L(j) gauge boson, to explain the e(+/-) excess in cosmic rays observed by ATIC and PAMELA experiments, and more recently by Fermi experiment. There are three types of U(1)L(i)-L(j) models: (a) U(1)(Le-L mu) (b) U(1)(Le-L tau) and (c) U(1)(Le-L tau). Although ATIC or Fermi data are consistent with PAMELA data separately, ATIC and Fermi data do not agree with each other. We therefore aim to identify which of the three models can explain which data set better. We find that models (a) and (b) can give correct dark matter relic density and explain the ATIC and PAMELA data simultaneously recur to the Breit-Wigner enhancement. Whereas model (c) with a larger Z' mass can explain Fermi and PAMELA data simultaneously. In all cases the model parameters are restricted to narrow regions. Future improved data will decide which set of data is correct and also help to decide the correct dark matter model. (C) 2009 Elsevier B.V. All rights reserved. |
学科领域 | Physics |
DOI | 10.1016/j.physletb.2009.06.009 |
收录类别 | SCI ; INSPIREHEP ; ADS |
WOS类目 | Physics, Multidisciplinary |
WOS记录号 | WOS:000268210600003 |
ADS Bibcode | 2009PhLB..678..168B |
ADS URL | https://ui.adsabs.harvard.edu/abs/2009PhLB..678..168B |
ADS引文 | https://ui.adsabs.harvard.edu/abs/2009PhLB..678..168B/citations |
INSPIRE ID | 814462 |
INSPIRE URL | https://inspirehep.net/literature/814462 |
引用统计 | 正在获取...
被引频次:88 [INSPIRE]
被引频次:90 [ADS]
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文献类型 | 期刊论文 |
条目标识符 | https://ir.ihep.ac.cn/handle/311005/226644 |
专题 | 粒子天体物理中心 |
推荐引用方式 GB/T 7714 | Bi XJ,Yuan Q,Bi, XJ,et al. Parameters in a class of leptophilic dark matter models from PAMELA, ATIC and FERMI[J]. PHYSICS LETTERS B,2009,678(2):#REF!. |
APA | 毕效军,袁强,Bi, XJ,He, XG,&Yuan, Q.(2009).Parameters in a class of leptophilic dark matter models from PAMELA, ATIC and FERMI.PHYSICS LETTERS B,678(2),#REF!. |
MLA | 毕效军,et al."Parameters in a class of leptophilic dark matter models from PAMELA, ATIC and FERMI".PHYSICS LETTERS B 678.2(2009):#REF!. |
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