Determination of dark matter properties at high-energy colliders

被引：180

作者：

Baltz, Edward A. ^{[1
]}

Battaglia, Marco

Peskin, Michael E.

Wizansky, Tommer

机构：

[1] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94309 USA

[2] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[3] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA

[4] Stanford Univ, Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA

来源：

PHYSICAL REVIEW D | 2006年 / 74卷 / 10期

关键词：

MUON MAGNETIC-MOMENT; GAMMA-RAYS; E(+)E(-) ANNIHILATION; NUCLEAR RECOIL; SUPERSYMMETRY; HALOS; CONSTRAINTS; BREAKING; PARTICLE; PHYSICS;

D O I：

10.1103/PhysRevD.74.103521

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

If the cosmic dark matter consists of weakly-interacting massive particles, these particles should be produced in reactions at the next generation of high-energy accelerators. Measurements at these accelerators can then be used to determine the microscopic properties of the dark matter. From this, we can predict the cosmic density, the annihilation cross sections, and the cross sections relevant to direct detection. In this paper, we present studies in supersymmetry models with neutralino dark matter that give quantitative estimates of the accuracy that can be expected. We show that these are well matched to the requirements of anticipated astrophysical observations of dark matter. The capabilities of the proposed International Linear Collider (ILC) are expected to play a particularly important role in this study.

引用

页数：57

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