Concentrated Dark Matter and PBHs Scott Watson ( Syracuse University - PowerPoint PPT Presentation

Mar 01, 2024 •108 likes •436 views

Concentrated Dark Matter and PBHs Scott Watson ( Syracuse University ) Based on: Concentrated Dark Matter PRD 97 arXiv: 1711.04773 with J. Dror (Berkeley), E. Kuflik (Hebrew University), and B. Melcher (Syracuse) Primordial Black

Concentrated Dark Matter and PBHs Scott Watson ( Syracuse University ) Based on: “Concentrated Dark Matter” — PRD 97 arXiv: 1711.04773   with J. Dror (Berkeley), E. Kuflik (Hebrew University), and B. Melcher (Syracuse) “Primordial Black Holes and Co-Decaying Dark Matter” — arXiv: 1902.04082   with J. Georg (Rensselaer Polytech. Inst.) and B. Melcher (Syracuse)
What happens at The end of Inflation?   Gravitationally coupled hidden sectors are a   natural consequence of inflationary model building. Image courtesy F . Quevedo
Plan for this talk: Part One: Concentrated Dark Matter Weakly coupled to Standard Model, naturally leads to departure from a radiation dominated universe Observables? Part Two: Primordial Black Holes as Dark Matter Weakly coupled to Standard Model. Can they be all or part of the dark matter?

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Concentrated Dark Matter and PBHs Scott Watson ( Syracuse University - PowerPoint PPT Presentation

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Concentrated Dark Matter and PBHs Scott Watson ( Syracuse University - PowerPoint PPT Presentation

Concentrated Dark Matter and PBHs Scott Watson ( Syracuse University ) Based on: Concentrated Dark Matter PRD 97 arXiv: 1711.04773 with J. Dror (Berkeley), E. Kuflik (Hebrew University), and B. Melcher (Syracuse) Primordial Black

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