arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 1104.3572hep-phastro-ph.COastro-ph.HEhep-ex
收藏

XENON100和LHC结果对暗物质模型的意义

Implications of XENON100 and LHC results for Dark Matter models

Marco Farina, Mario Kadastik, Martti Raidal, Duccio Pappadopulo, Joosep Pata, Alessandro Strumia

摘要:

我们执行一个适合最近的氙100数据和研究其影响的暗物质的情况。我们发现非弹性暗物质对DAMA/LIBRA周年调制信号的贡献是不利的。对于标量单重DM模型,我们发现Xenon 100数据不利于它的约束极限。我们研究了CMSSM以及低尺度唯象MSSM,并考虑了最新的Tevatron和LHC数据(1.1/fb)的s粒子和Bs \rightarrow μμ。在EPS 2011会议之后,LHC排除了DM冻结的“希格斯共振”区域,并且Xenon 100不赞成在CMSSM参数空间的“焦点”区域实现的“良好回火”的bino/higgsino。优选区域向更重的sparticle、更高的微调、更高的tan β移动,并且拟合的质量劣化。

英文摘要:

We perform a fit to the recent Xenon100 data and study its implications for Dark Matter scenarios. We find that Inelastic Dark Matter is disfavoured as an explana- tion to the DAMA/LIBRA annual modulation signal. Concerning the scalar singlet DM model, we find that the Xenon100 data disfavors its constrained limit. We study the CMSSM as well as the low scale phenomenological MSSM taking into account latest Tevatron and LHC data (1.1/fb) about sparticles and Bs \rightarrow μμ. After the EPS 2011 conference, LHC excludes the "Higgs-resonance" region of DM freeze-out and Xenon100 disfavors the "well-tempered" bino/higgsino, realized in the "focus-point" region of the CMSSM parameter space. The preferred region shifts to heavier sparticles, higher fine-tuning, higher tan β and the quality of the fit deteriorates.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑