Video URL

https://pirsa.org/24010082

What can we learn from elastic scattering of Cosmological Gravitational Wave Background? - VIRTUAL

König, M. (2024). What can we learn from elastic scattering of Cosmological Gravitational Wave Background? - VIRTUAL. Perimeter Institute for Theoretical Physics. https://pirsa.org/24010082

König, Morgane. What can we learn from elastic scattering of Cosmological Gravitational Wave Background? - VIRTUAL. Perimeter Institute for Theoretical Physics, Jan. 16, 2024, https://pirsa.org/24010082 

          @misc{ scivideos_PIRSA:24010082,
            doi = {10.48660/24010082},
            url = {https://pirsa.org/24010082},
            author = {K{\"o}nig, Morgane},
            keywords = {Cosmology},
            language = {en},
            title = {What can we learn from elastic scattering of Cosmological Gravitational Wave Background? - VIRTUAL},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2024},
            month = {jan},
            note = {PIRSA:24010082 see, \url{https://scivideos.org/pirsa/24010082}}
          }

Morgane König Massachusetts Institute of Technology (MIT)

DOI 10.48660/24010082
Source Repository PIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The current progress in gravitational wave detection opened a new exciting window in cosmology. It is natural to ask ourselves how we can best use this new tool to explore physics beyond the standard model. With this idea in mind, my collaborators and I asked what we could learn from Cosmological Gravitational Wave Backgrounds if they were to be detected to a certain accuracy. By drawing comparison to the cosmic microwave background, we investigate the impact of elastic scattering on any cosmological background. Specifically, we focus on quantifying spectral distortions in the energy density spectrum of CGWB attributed to interaction with beyond-the-standard-model particles. We will also explore the effect that elastic scattering of graviton of Primordial Black holes would have on CGWB in the regime where PBHs account for all the dark matter.

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Zoom link https://pitp.zoom.us/j/98460268383?pwd=RytzWHd5dU1lenRhWG1NYXM3OVJpQT09