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.
北京工业大学高能组

STOCHASTIC APPROACH TO INFLATION AND PRIMORDIAL BLACK HOLES FORMATION.

by Dr Diego Cruces (ICC, Barcelona U)

Asia/Shanghai
zoom id:819 5644 5168 passcode:700793 (线上)

zoom id:819 5644 5168 passcode:700793

线上

北京市朝阳区平乐园100号
Description
Abstract: The stochastic approach to inflation (as it is usually formulated) is based upon the separate universe approach. While for the case of slow-roll, the separate universe approach is enough to obtain cosmological observables, in other cases that are relevant for primordial black hole formation, like in ultra-slow-rolling and/or constant-rolling backgrounds, this is not the case. In this seminar, I will define an improved version of the stochastic approach to inflation which is valid for any inflationary regime, by doing so, I will show that the linear perturbation theory power spectrum coincides with the one calculated by the use of the stochastic approach, contrary to what is claimed in recent literature.