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Non-Linear Fuzzy Dark Matter Modelling with Extended LPT Alex Laguë, Renée Hložek, George Stein, and Dick Bond Fuzzy Dark Matter FDM ✤ Ultra-light boson: ✤ Scale-dependent…
New signals in dark matter detectors Joachim Kopp based on work done in collaboration with Roni Harnik and Pedro Machado arXiv:12026073 Kaffeepalaver @ MPIK November 08 2012…
M.Battaglieri - INFN GEBDX - Light Dark Matter search in a Beam Dump eXperiment1 M.Battaglieri INFN-GE Italy BDX Light Dark Matter search in a Beam Dump eXperiment M.Battaglieri…
Constraining Inert Dark Matter by Rγγ and WMAP data Maria Krawczyk Dorota Soko lowska Pawe l Swaczyna Bogumi la Świeżewska Univeristy of Warsaw Faculty of Physics Hoża…
Mon Not R Astron Soc 000 1– 14 0000 Printed 8 November 2018 MN LATEX style file v22 Dark Matter Halo Growth II: Diffuse Accretion and its Environmental Dependence Onsi…
How cold is cold dark matter? Mark Wilkinson with Matt Walker, Justin Read, Walter Dehnen, Gerry Gilmore,Ugur Ural, David Cole, David Maurin, etc. Friday, 6 August 2010 Dark…
1 Class 23 : Dark Matter Halos n This class l Dark matter halos the “skeleton” of a galaxy l Halo over-density factor ΔV l Applications of Virial Theorem…
Gravitational Lensing and the Dark Energy Future Prospects Wayne Hu SLAC August 2002 1 05 0 -05 06 065 07 -1 ΩDE w -09 -1 -11 06 065 07 ΩDE w Outline • Standard model…
Mon. Not. R. Astron. Soc. 000, 1–25 2020 Printed 9 July 2020 MN LATEX style file v2.2 A dark matter profile to model diverse feedback-induced core sizes of ΛCDM haloes…
Blue: background uncertainty Background + DMA signal describe EGRET data! Blue: WIMP mass uncertainty Wim de Boer, Karlsruhe HEP2008, Chile, Jan. 8, 2008 * Analysis of EGRET…
Paolo Gondolo University of Utah Dark Matter Particle Candidates Evidence for cold dark matter 376±02 pJm3 ordinary matter 1 to 4 pJm3 neutrinos 201±2 pJm3 cold…
Energy of Black Holes Dark Matter Dark Energy Remo Ruffini ICRANet ICRA and Università di Roma “La Sapienza” Thursday 20 October 2005 “Geometry and the Universe”…
1 Check better resolution by Retained Melt Surface (RMS) Experiment Retained Melt Surface trace of retained melt (=isolated liquid) Movie File AA’ Choose more accurate
LUX: A Liquid Xenon Dark Matter Detector Masahiro Morii Harvard University August 24, 2010 * LUX Dark Matter Detector New Physics — Where? * From the labs — Unexplained…
Το μυστήριο της σκοτεινής ύλης Μετάφραση: Χ Στογιάννος ΕΚΦΕ Αλίμου 2018 1 ΠΕΡΙΕΧΟΜΕΝΑ 4 10 11 11 14 16…
8/3/2019 Adam Lidz- Warm Dark Matter, the Temperature of the IGM, and the Ly- Forest 1/32Warm Dark Matter, the Temperatureof the IGM, and the Ly-ForestAdam Lidz (CfA)DM_MCFP:…
Dark Matter and Dark Energy from the solution of the strong CP problem Roberto Mainini, L. Colombo & S.A. Bonometto Universita’ di Milano Bicocca Mainini & Bonometto…
Theory Overview Hitoshi Murayama IPMU Berkeley APSJPS meeting 0nbb seminar Oct 11, 2009, Waikoloa Hilton Hitoshi Murayama, APSJPS 0νββ seminar Waikoloa 2009 There are…
Primordial Black Holes Alexandre Arbey IP2I UCBL Many thanks to J. Au�nger, J.-F. Coupechoux and J. Silk! JOGLy 2 Lyon � October 17th, 2019 Introduction Primordial black…
1 DARK MATTER LHC – ATLAS SEASON 2 Dan Levin, University of Michigan on behalf of the ATLAS Collabora 1. Direct detec+on : èNuclear recoil from DM par χχ recoil against…