PAMELA and ATIC Anomalies in Decaying Gravitino Dark Matter Scenario
PAMELA and ATIC Anomalies in Decaying Gravitino Dark Matter Scenario
复制标题
DOI：
10.1142/9789814293792_0015
复制
发表时间：
2009-03
期刊：
影响因子：
--
通讯作者：
Koji Ishiwata;S. Matsumoto;T. Moroi
中科院分区：
文献类型：
--
作者：
Koji Ishiwata;S. Matsumoto;T. Moroi
受Pamela和ATIC的最新结果的启发，我们研究了引力子暗物质衰变产生的宇宙线电子和正电子。我们计算了宇宙线电子和正电子通量，并讨论了对Pamela和ATIC数据的影响。在本文中，我们将证明在这种情况下可以解释Pamela和ATIC观测到的异常通量。我们还将讨论在这种情况下来自银河系中心的同步辐射通量。
Motivated by the recent results from the PAMELA and ATIC, we study the cosmic-ray electron and positron produced by the decay of gravitino dark matter. We calculate the cosmic-ray electron and positron fluxes and discuss implications to the PAMELA and ATIC data. In this paper, we will show that the observed anomalous fluxes by the PAMELA and ATIC can be explained in such a scenario. We will also discuss the synchrotron radiation flux from the Galactic center in such a scenario.