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弱相互作用大质量粒子的衰落？模型、搜索及限制的综述

The waning of the WIMP? A review of models, searches, and constraints.

作者信息

Arcadi Giorgio, Dutra Maíra, Ghosh Pradipta, Lindner Manfred, Mambrini Yann, Pierre Mathias, Profumo Stefano, Queiroz Farinaldo S

机构信息

1Max Planck Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.

2Laboratoire de Physique Théorique, CNRS, Univ. Paris-Sud, Université Paris-Saclay, 91405 Orsay, France.

出版信息

Eur Phys J C Part Fields. 2018;78(3):203. doi: 10.1140/epjc/s10052-018-5662-y. Epub 2018 Mar 10.

DOI:10.1140/epjc/s10052-018-5662-y
PMID:31258403
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6560773/
Abstract

Weakly Interacting Massive Particles (WIMPs) are among the best-motivated dark matter candidates. No conclusive signal, despite an extensive search program that combines, often in a complementary way, direct, indirect, and collider probes, has been detected so far. This situation might change in near future due to the advent of one/multi-TON Direct Detection experiments. We thus, find it timely to provide a review of the WIMP paradigm with focus on a few models which can be probed at best by these facilities. Collider and Indirect Detection, nevertheless, will not be neglected when they represent a complementary probe.

摘要

弱相互作用大质量粒子（WIMPs）是最有说服力的暗物质候选者之一。尽管开展了广泛的搜索计划，该计划常常以互补的方式将直接探测、间接探测和对撞机探测结合起来，但迄今为止尚未检测到确凿的信号。由于单/多吨级直接探测实验的出现，这种情况在不久的将来可能会改变。因此，我们认为适时对WIMP范式进行综述，重点关注一些这些设施最能探测到的模型。不过，当对撞机探测和间接探测代表一种互补性探测手段时，也不会被忽视。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4232/6560773/8a71bb64e7d2/10052_2018_5662_Fig21_HTML.jpg
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