We review the various methods to search for dark matter particles based on the resultsfrom the recent symposium at Marina Del Rey [1]. At present, the most promisingmethods are: (a) Direct searches with earth-bound detectors made of Ge, Xe, Ar, etc. (b)Search for Gamma Rays from dark matter annihilation in the local galaxy. We note thereis progress on (a) to date, the expectation for the current generation of detectors CDMSII, Edelweiss H, ZEPLIN H, WARP etc. and hopes for future one ton detectors. In thecase of (b) the detection of Dark Matter Gamma Rays will depend on the clumping ofDark Matter in the Galaxy and Backgrounds. We will discuss this. We also discuss verybriefly warm dark matter.
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机译：我们审查了各种方法，以根据玛丽娜Del Rey [1]的最近研讨会来搜索暗物质颗粒。目前，最有前景的方法是：（a）与GE，XE，AR等的接地检测器直接搜索（b）从局部星系中的暗物质湮灭搜索伽马光线。我们注意到（a）迄今为止的进展情况，对当前一代探测器Cdmsii，Edelweiss H，Zeplin H，Warp等的期望，并希望未来一吨探测器。在（b）的咬合中，暗物质伽马射线的检测将取决于星系和背景中的陆地群。我们会讨论这一点。我们还讨论了非常温暖的暗物质。
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