Gravitino Dark Matter

被引:0
作者
Buchmueller, Wilfried [1 ]
机构
[1] Deutsch Elektronen Synchrotron DESY, D-22607 Hamburg, Germany
来源
SUSY09: THE 17TH INTERNATIONAL CONFERENCE ON SUPERSYMMETRY AND THE UNIFICATION OF FUNDAMENTAL INTERACTIONS | 2009年 / 1200卷
关键词
supergravity; dark matter; leptogenesis; cosmic rays; SUPERSYMMETRY; LEPTOGENESIS; ENERGIES;
D O I
暂无
中图分类号
O59 [应用物理学];
学科分类号
摘要
Gravitino dark matter, together with thermal leptogenesis, implies an upper bound on the masses of superparticles In the case of broken R-parity the constraints from primordial nucleosynthesis are naturally satisfied and decaying gravitinos lead to characteristic signatures in high energy cosmic rays Electron and positron fluxes from gravitino decays cannot explain both, the PAMELA positron fraction and the electron + positron flux recently measured by Fermi LAT The observed fluxes require astrophysical sources The measured antiproton flux allows for a sizable contribution of decaying gravitinos to the gamma-ray spectrum, in particular a line at an energy below 300 GeV
引用
收藏
页码:155 / 164
页数:10
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