摘要
We show that the PAMELA anomaly in the positron fraction as well as the ATIC/PPB-BETS excesses in the e- +e+ flux are simultaneously explained in our scenario that a hidden U(1)h gauge boson constitutes dark matter of the Universe and decays into the standardmodel particles through a kinetic mixing with an U(1)b-l gauge boson. Interestingly, the B - L charge assignment suppresses an antiproton flux in consistent with the PAMELA and BESS experiments, while the hierarchy between the B - L symmetry breaking scale and the weak scale naturally leads to the right lifetime of O(1026) seconds.
| 原文 | 英語 |
|---|---|
| 頁(從 - 到) | 553-559 |
| 頁數 | 7 |
| 期刊 | Progress of Theoretical Physics |
| 卷 | 122 |
| 發行號 | 2 |
| DOIs | |
| 出版狀態 | 已發佈 - 2009 8月 |
| 對外發佈 | 是 |
ASJC Scopus subject areas
- 物理與天文學(雜項)
指紋
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