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The Mitchell Conference on Collider, Dark Matter, and Neutrino Physics 2025

13–16 May 2025
Mitchell Institute, Texas A&M University
America/Chicago timezone

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Session

Tuesday Afternoon Session 2

13 May 2025, 15:40
Hawking Auditorium (Mitchell Institute, Texas A&M University)

Hawking Auditorium

Mitchell Institute, Texas A&M University

Conveners

Tuesday Afternoon Session 2: Tuesday Afternoon Session 2

  • Isabelle Goldstein (Texas A&M University)

Presentation materials

There are no materials yet.

  1. 17. CMB Constraints on Non-Minimally Coupled Ultralight Dark Matter
    Prof. Kimberly Boddy (University of Texas at Austin)
    13/05/2025, 15:40
  2. 14. Structure Formation in Dark Matter with Warm White Noise
    Mustafa Amin, Mustafa Amin (Rice University)
    13/05/2025, 16:03
  3. 15. Observational Signatures of Cosmological Stasis
    Brooks Thomas
    13/05/2025, 16:26

    Cosmological stasis is a phenomenon wherein the abundances of multiple cosmological energy components with different equations of state remain constant for an extended period despite the expansion of the universe. In this talk, I discuss the possible observational implications of this phenomenon. These include characteristic imprints in the stochastic gravitational-wave background and an...

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  4. 49. TBD
    Savvas Koushiappas, Savvas Koushiappas (Brown University)
    13/05/2025, 16:49
  5. 16. Evaporating Primordial Black Holes: Reformation and Isocurvature Perturbations
    Dr TaeHun Kim (KIAS)
    13/05/2025, 17:12

    Primordial black holes (PBHs) lighter than 10^9 g are expected to have fully evaporated before the big bang nucleosynthesis, leaving their past abundances unconstrained by observations. Depending on their initial abundance, these PBHs could have temporarily dominated the Universe or remained as a subdominant component. In this talk, I explore the cosmological implications of such light mass...

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