.png){kind=icon}
返回
Higher spin dark matter
.png){kind=icon}
OA
AI
DOI：10.1016/j.physletb.2021.136436.png)
.png){kind=icon}
.png){kind=icon}
分享.png){kind=icon}
收藏
摘要
En 中文
Little is known about dark matter beyond the fact that it does not interact with the standard model or itself, or else does so incredibly weakly. A natural candidate, given the history of no-go theorems against their interactions, are higher spin fields. Here we develop the scenario of higher spin (spin s > 2) dark matter. We show that the gravitational production of superheavy bosonic higher spin fields during inflation can provide all the dark matter we observe today. We consider the observable signatures, and find a potential characteristic signature of bosonic higher spin dark matter in directional direct detection; we find that there are distinct spin-dependent contributions to the double differential recoil rate, which complement the oscillatory imprint of higher spin fields in the cosmic microwave background. We consider the extension to higher spin fermions and supersymmetric higher spins. (C) 2021 The Author(s). Published by Elsevier B.V.
Keyword:
MASSLESS GAUGE SUPERFIELDS
EQUATIONS
FIELDS
AI总结
对已上传原文的论文进行重点信息的提取，主要内容包括：简要概述、研究摘要、背景介绍、关键亮点、图文解析、展望与总结。
期刊
IF:
4.5
论文数:
3.2W
被引数:
7.3W
机构
引用论文
.png){kind=icon}
New Perspective for Heat Transfer Evaluation During Film Condensation Inside Tubes管内膜状凝结传热评价的新视角
OAAI
OAAI分享收藏AN ANALYTICAL MODEL FOR DETERMINING THE PER CAPITA INDEX OF SPORTS PLACES AND SPACES一种用于确定体育场所和空间人均指数的分析模型OAAI
OAAI分享收藏分享收藏
查看更多内容