Heavy dark matter through the Higgs portal

被引:182
|
作者
March-Russell, John [1 ]
West, Stephen M. [1 ,2 ]
Cumberbatch, Daniel [3 ]
Hooper, Dan [4 ]
机构
[1] Univ Oxford, Dept Phys, 1 Kebel Rd, Oxford OX1 3NP, England
[2] Univ Oxford Magdalen Coll, Oxford OX1 4AU, England
[3] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England
[4] Fermilab Natl Accelerator Lab, Ctr Particle Astrophys, Batavia, IL 60510 USA
来源
关键词
cosmology of theories beyond the SM; supersymmetric effective theories;
D O I
10.1088/1126-6708/2008/07/058
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Motivated by Higgs Portal and Hidden Valley models, heavy particle dark matter that communicates with the supersymmetric Standard Model via pure Higgs sector interactions is considered. We show that a thermal relic abundance consistent with the measured density of dark matter is possible for masses up to similar to 30 TeV. For dark matter masses above similar to 1 TeV, non-perturbative Sommerfeld corrections to the annihilation rate are large, and have the potential to greatly affect indirect detection signals. For large dark matter masses, the Higgs-dark-matter-sector couplings are large and we show how such models may be given a UV completion within the context of so-called "Fat-Higgs" models. Higgs Portal dark matter provides an example of an attractive alternative to conventional MSSM neutralino dark matter that may evade discovery at the LHC, while still being within the reach of current and upcoming indirect detection experiments.
引用
收藏
页数:24
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