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Ethan Siegel1,2, Mark Hertzberg3, JNF2 1University of Wisconsin, 2University of Florida, 3MIT Cosmic Cartography 4 December 2007 M = 5× 1014 M • Weak Field General
FERMI dark matter dwarf galaxies and dark satellites of the Milky Way Savvas M Koushiappas Saturday June 1 13 Many thanks to Alex Geringer-Sameth Saturday June 1 13 χ χ…
Tbilisi 2011 - p. 147 Parallel Worlds: from Dark Matter to Dark Gravity Zurab Berezhiani Università di L’Aquila and LNGS Gran Sasso, Italy Recent Advances in Quantum Field…
Winter conferences: cosmology • CMB • clusters • dark energy • dark matter Jean-Marc Le Goff séminaire SPP 7 avril 2014 CMB 2 PolarBear: lensed B…
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…
ar X iv :1 31 0. 26 95 v1 [ as tro -p h. H E] 1 0 O ct 2 01 3 Indirect Detection of Dark Matter with γ rays Stefan Funk ∗ ∗Kavli Institute for Particle Astrophysics…
PowerPoint Presentationisotropic gamma-ray background “The gamma-ray sky” - Minneapolis, October 10, 2013 Plan of my talk What is the isotropic γ-ray background
Antiproton and Electron Measurements and Dark Matter Searches Piergiorgio Picozza INFN and University of Rome Tor Vergata 8th International Workshop on Identification of…
photo by Art Rosch Missing Satellite Problem and Dark Matter Models Collaborators: James Bullock Louis Strigari Manoj Kaplinghat Center for Cosmology UC Irvine Properties…
5 Dark matter and dark energy the Universe revealed Our place Courtesy: NASA How much matter • Add up all we can see – ~ 1 atom per 10 m-3 • Ω = 1 – ~ 1 atom m-3…
Search for dark matter and transient variations in using fibre-linked optical atomic clocksSearch for dark matter and transient variations in α using fibre-linked optical
Neutralino Dark Matter in Light Higgs Boson Scenario (LHS) The scenario is consistent with particle physics experiments Particle mass b → sγ Bs →μ+μ- cosmological…
Dark Matter Direct Dark Matter Search CRESST JJochum Kepler Center for Astro and Particle Physics Dark Matter distance to center = Dark Matter halo in galaxy Keplers‘s…
Direct Dark Matter Search Dark Matter in the Universe Ω = 023 • non-baryonic • not neutrinos physics beyond the standard model thermal relics from Big Bang weakly…
Lecture fifteen: Friday 21st March ΛCDM Universe contd Longair chap 13 16 1 ONLY predicts dark matter distribution NGC 4216 2 dissipation how goes gas collapse in a dark…
Ultra-light Cold Dark Matter from α− attractors @ Post-Planck Cosmology 2017 Swagat Saurav Mishra SRF CSIR Inter University Centre for Astronomy and Astrophysics —————–…
Nuclear structure for ββ decay and dark matter searches Javier Menéndez JSPS Fellow The University of Tokyo International Workshop on Double Beta Decay and Underground…
DARK MATTER AND THE WEAK SCALE Graciela Gelmini - UCLA INPAC- Berkeley-May 4, 2007 Graciela Gelmini-UCLA . Physics beyond the SM is required by Dark Matter, and expected…
The case for a sterile neutrino as warm dark matter Hey! Λ CDM do you have a small scale problem? WDM: Sterile neutrinos come to the rescue!! Any sightings of (El) ν s…
to Massive Vector Bosons Master of Physics Abstract In this thesis the width of the gravitino under radiative loop decays G → Z0ν and G → W+l− in R-parity