1. IE browser is NOT supported anymore. Please use Chrome, Firefox or Edge instead.
2. If you are a new user, please register to get an IHEP SSO account through https://login.ihep.ac.cn/registlight.jsp Any questions, please email us at helpdesk@ihep.ac.cn or call 88236855.
3. If you need to create a conference in the "Conferences, Workshops and Events" zone, please email us at helpdesk@ihep.ac.cn.
4. The max file size allowed for upload is 100 Mb.
Particle Astrophysics Theory

The Self-Organized Criticality of Dark Matter in the Early Universe

by Prof. 明杰 金 (荆楚理工学院)

Asia/Shanghai
Description

报告人简介:

金明杰博士,本科毕业于兰州大学,硕士毕业于浙江大学,博士毕业于中国科学院高能物理研究所,之后在北京师范大学做博士后研究,现就职于荆楚理工学院。研究方向是高能粒子物理和暗物质唯象理论。

 

报告摘要:

In this talk, we propose a new mechanism for dark matter freeze-out that results in the self-organized criticality in dark matter production, wherein the final relic abundance is independent of initial inputs, in analogy to scale invariance in other realms of non-equilibrium physics. The dynamic of self-organized is triggered through a semi-annihilation process χϕ→ϕϕ in the premise of the instability of dark partner ϕ, where χ is the dark matter candidate. The relic abundance can be analytically ascertained when the dark partner is slightly heavier than the dark matter, which permits a substantially heavy dark matter mass without violating unitarity bounds. We demonstrate that this process provides a bridge between the freeze-in and freeze-out mechanisms, and that the intricate dynamics of self-organized criticality can be actualized in a thermal dark sector bath.