Dark matter production at the LHC from black hole remnants1

被引:6
|
作者
Nayak G.C. [1 ]
机构
[1] Department of Physics, University of Arizona, Tucson
关键词
Black Hole; Dark Matter; Large Hadron Collider; Nucleus Letter; Dark Matter Candidate;
D O I
10.1134/S1547477111040121
中图分类号
学科分类号
摘要
We study dark matter production at CERN LHC from black hole remnants (BHR). We find that the typical mass of these BHR at the LHC is ~5-10 TeV which is heavier than other dark matter candidates, such as axion, axino, neutralino, etc. We propose the detection of this dark matter via single jet production in the process pp → jet + BHR (dark matter) at CERN LHC. We find that for zero impact parameter partonic collisions, the monojet cross section is not negligible in comparison to the standard model background and is much higher than the other dark matter scenarios studied so far. We also find that dσ/dpT of jet production in this process increases as pT increases, whereas in all other dark matter scenarios the dσ/dpT decreases at CERN LHC. This may provide a useful signature for dark matter detection at the LHC. However, we find that when the impact parameter dependent effect of inelasticity is included, the monojet cross section from the above process becomes much smaller than the standard model background and may not be detectable at the LHC. © 2011 Pleiades Publishing, Ltd.
引用
收藏
页码:337 / 341
页数:4
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