PIRSA:24020064

Video URL

https://pirsa.org/24020064

Gravothermal Evolution of Self-Interacting Dark Matter Halos in the Short Mean Free Path Regime - VIRTUAL

Nasr, S. (2024). Gravothermal Evolution of Self-Interacting Dark Matter Halos in the Short Mean Free Path Regime - VIRTUAL. Perimeter Institute for Theoretical Physics. https://pirsa.org/24020064

Nasr, Sophia. Gravothermal Evolution of Self-Interacting Dark Matter Halos in the Short Mean Free Path Regime - VIRTUAL. Perimeter Institute for Theoretical Physics, Feb. 13, 2024, https://pirsa.org/24020064 

          @misc{ scivideos_PIRSA:24020064,
            doi = {10.48660/24020064},
            url = {https://pirsa.org/24020064},
            author = {Nasr, Sophia},
            keywords = {Cosmology},
            language = {en},
            title = {Gravothermal Evolution of Self-Interacting Dark Matter Halos in the Short Mean Free Path Regime - VIRTUAL},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {feb},
            note = {PIRSA:24020064 see, \url{https://scivideos.org/pirsa/24020064}}
          }

Sophia Nasr York University

Talk numberPIRSA:24020064
DOI10.48660/24020064
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

In this talk, I will discuss my exploration of the gravothermal collapse of isolated self-interacting dark matter (SIDM) halos, driven deep into the core-collapsed regime where interactions are frequent. We investigate how elastic collisions influence the central region of SIDM halos as they undergo core collapse. In our numerical findings, we discover a remarkable universality in the behavior of halos, allowing us to predict their evolution deep in the core-collapsed regime. We develop a semi-analytic method to characterize the core properties of the halo in the latest stages of evolution, which is crucial for making predictions of the mass of potential black holes forming at the heart of these dark matter halos.

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