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停止共湮灭带的范围。

The extent of the stop coannihilation strip.

作者信息

Ellis John, Olive Keith A, Zheng Jiaming

机构信息

Theoretical Particle Physics and Cosmology Group, Department of Physics, King's College London, London, WC2R 2LS UK ; Theory Division, CERN, 1211  Geneva 23, Switzerland.

School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA ; William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA.

出版信息

Eur Phys J C Part Fields. 2014;74(7):2947. doi: 10.1140/epjc/s10052-014-2947-7. Epub 2014 Jul 9.

Abstract

Many supersymmetric models such as the constrained minimal supersymmetric extension of the Standard Model (CMSSM) feature a strip in parameter space where the lightest neutralino [Formula: see text] is identified as the lightest supersymmetric particle, the lighter stop squark [Formula: see text] is the next-to-lightest supersymmetric particle (NLSP), and the relic [Formula: see text] cold dark matter density is brought into the range allowed by astrophysics and cosmology by coannihilation with the lighter stop squark [Formula: see text] NLSP. We calculate the stop coannihilation strip in the CMSSM, incorporating Sommerfeld enhancement effects, and we explore the relevant phenomenological constraints and phenomenological signatures. In particular, we show that the [Formula: see text] may weigh several TeV, and its lifetime may be in the nanosecond range, features that are more general than the specific CMSSM scenarios that we study in this paper.

摘要

许多超对称模型,如标准模型的约束最小超对称扩展(CMSSM),在参数空间中有一个条带区域,其中最轻的中性伴随子[公式:见正文]被认定为最轻的超对称粒子,较轻的顶夸克超对称伙伴[公式:见正文]是次最轻的超对称粒子(NLSP),并且遗迹[公式:见正文]冷暗物质密度通过与较轻的顶夸克超对称伙伴[公式:见正文]NLSP的共湮灭被带入天体物理学和宇宙学所允许的范围。我们在CMSSM中计算顶夸克超对称伙伴共湮灭条带,纳入索末菲增强效应,并探索相关的现象学约束和现象学特征。特别是,我们表明[公式:见正文]可能重达数太电子伏特,其寿命可能在纳秒范围内,这些特征比我们在本文中研究的特定CMSSM情景更具普遍性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17c4/4370881/b7030caa6c62/10052_2014_2947_Fig2_HTML.jpg

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