Dark Radiation & Superheavy Dark Matter from Black Hole - PowerPoint PPT Presentation

May 17, 2023 •318 likes •996 views

Dark Radiation & Superheavy Dark Matter from Black Hole Domination Sam McDermott Utah, Aug 7 2019 1905.01301 (with Dan Hooper and Gordan Krnjaic) (+ongoing) Basic Question: can a population of black holes that evaporate early have an

Dark Radiation & Superheavy Dark Matter from Black Hole Domination Sam McDermott Utah, Aug 7 2019 1905.01301 (with Dan Hooper and Gordan Krnjaic) (+ongoing…)
Basic Question: can a population of black holes that evaporate early have an observable impact on the universe?

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Dark Radiation & Superheavy Dark Matter from Black Hole - PowerPoint PPT Presentation

Dark Radiation & Superheavy Dark Matter from Black Hole Domination Sam McDermott Utah, Aug 7 2019 1905.01301 (with Dan Hooper and Gordan Krnjaic) (+ongoing) Basic Question: can a population of black holes that evaporate early have an

Beyond Dark Matter and Dark Energy Sean Carroll Beyond Dark Matter and Dark Energy Sean Carroll,

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Credit: ESO/G Credit: ESA/Hubble DARK MATTER Dark Matter 10 x Luminous Matter Dark Matter

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Dark Radiation & Superheavy Dark Matter from Black Hole - PowerPoint PPT Presentation

Dark Radiation & Superheavy Dark Matter from Black Hole Domination Sam McDermott Utah, Aug 7 2019 1905.01301 (with Dan Hooper and Gordan Krnjaic) (+ongoing) Basic Question: can a population of black holes that evaporate early have an

Beyond Dark Matter and Dark Energy Sean Carroll Beyond Dark Matter and Dark Energy Sean Carroll,

Doomsday Dark Matter Doomsday Dark Matter or Some stones are better left unturned Doomsday

Credit: ESO/G Credit: ESA/Hubble DARK MATTER Dark Matter 10 x Luminous Matter Dark Matter

Black Hole Thermodynamics Robert M. Wald I. Black Holes; Event Horizons and Killing Horizons II.

Black hole X-ray binaries V: Formation and evolution of black hole binaries Thomas J. Maccarone

Neutrinos and Dark Matter Alejandro Ibarra Technische Universitt Mnchen Neutrino 2014

Dark Stars, Dark Matter and Black Holes Chris Kouvaris Solvay Inst. Brussels, 5 April 2019 Why

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Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe 22.1 Unseen Influences in the

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Searching for the Dark Matter Wind: a Novel Approach to Dark Matter Detection Jocelyn Monroe, MIT

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Chapter 20: Phenomena Phenomena: Below is a list of stable isotopes of different elements.

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Radiation Transfer Status Time dependent radiation transport implemented in Athena++, roughly

Window Options Keeping cool in summer, warm in winter, comfortable all the time,... and saving

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DARK MATTER IN DSPH Paolo Salucci (& G. Gilmore) SISSA (Oxford) Outline of the Review Dark