Looking for a heavy W-ino lightest supersymmetric particle in collider and dark matter experiments

Looking for a heavy W-ino lightest supersymmetric particle in collider and dark matter experiments
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在对撞机和暗物质实验中寻找重W-ino最轻超对称粒子

DOI:
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发表时间:
2007
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影响因子:
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通讯作者:
D. Roy
D. Roy
中科院分区:
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文献类型:
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作者:
U. Chattopadhyay;D. Das;P. Konar;D. Roy

文献摘要

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我们研究了在异常介导的超对称破缺和一些弦模型中获得的最轻超粒子的现象学。威尔金森微波各向异性探测器对暗物质遗迹密度的约束意味着最轻的超粒子质量为 2.0char21{}2.3 TeV。我们在 CLIC 找到了这样一个重型酒杯的可行签名,其最高质心能量为 5 TeV。人们还期望至少对于尖点暗物质晕轮廓来说,来自其在银河系中心的成对湮灭的可行的单色$ensuremath{gamma}$射线信号。
We investigate the phenomenology of a wino lightest superparticle as obtained in anomaly mediated supersymmetry breaking and some string models. The Wilkinson Microwave Anisotropy Probe constraint on the dark matter relic density implies a wino lightest superparticle mass of 2.0char21{}2.3 TeV. We find a viable signature for such a heavy wino at CLIC, operating at its highest center of mass energy of 5 TeV. One also expects a viable monochromatic $ensuremath{gamma}$-ray signal from its pair-annihilation at the galactic center at least for cuspy dark matter halo profiles.