PIRSA:24040098

Video URL

https://pirsa.org/24040098

Primordial Black Holes from Axion Domain Walls

Dunsky, D. (2024). Primordial Black Holes from Axion Domain Walls. Perimeter Institute for Theoretical Physics. https://pirsa.org/24040098

Dunsky, David. Primordial Black Holes from Axion Domain Walls. Perimeter Institute for Theoretical Physics, Apr. 16, 2024, https://pirsa.org/24040098 

          @misc{ scivideos_PIRSA:24040098,
            doi = {10.48660/24040098},
            url = {https://pirsa.org/24040098},
            author = {Dunsky, David},
            keywords = {Particle Physics},
            language = {en},
            title = {Primordial Black Holes from Axion Domain Walls},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {apr},
            note = {PIRSA:24040098 see, \url{https://scivideos.org/pirsa/24040098}}
          }

David Dunsky New York University (NYU)

Talk numberPIRSA:24040098
DOI10.48660/24040098
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Besides providing a possible explanation to the strong CP problem and dark matter, the QCD axion possesses a rich cosmology. For example, if PQ breaking occurs after inflation, then axion cosmic strings form. Near the QCD phase transition, every axion string become attached to a domain wall which pull on the strings and cause the string-wall network to decay. While every string becomes attached to a domain wall, it is possible, though rare, to form an enclosed domain wall that is not attached to any axion string. These enclosed domain walls collapse under their own self tension, compressing a large amount of energy into a small volume and thereby potentially forming a primordial black hole. In this talk, I will discuss the abundance of enclosed domain walls, their dynamics of collapse, the efficiency of black hole formation, and their relic abundance. For sufficiently large axion decay constants, there may be an observable gravitational lensing signal at future lensing telescopes, especially in models with axion-like-particles.

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