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Zakopane May 2012 Gamma-rays Neutrinos Production Propagation Detection of Hard & soft e+ p, DZ0, W ProductionProduction Hard & soft e+ p, DZ0, W Decay rate ρ
Dark Matter Superfluidity & Galactic DynamicsJune 12, 2018 Dark Matter Distribution N-body simulations reveal universal density profile: Navarro, Frenk, White ’96
Dark matter, baryogenesis and neutrinos Mikhail Shaposhnikov ISAPP 2011: The dark side of the Universe Heidelberg, 13 and 14 July 2011 – p. 1 Outline 1 Introduction: “No…
Dark Energy in the Universe Scott Dodelson March 25, 2003 Overview Evidence for Dark Energy • Age: Hubble constant + globular clusters • Distance vs. redshift: Type Ia…
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…
CMB as a dark energy probe Carlo Baccigalupi Outline Fighting against a cosmological constant Parametrizing cosmic acceleration The CMB role in the current dark energy bounds…
PowerPoint Presentation Dr Caroline Edwards Birkbeck, University of London [email protected] Dark City: London After the Apocalypse London’s apocalyptic tradition…
linderteachin1.PDFand ⇒ Dark energy ~70% The horizon is 95% cloudy! Revolutions in PhysicsRevolutions in Physics STScI Expansion history t(a) DistanceDistance--redshift
Week 1 A Brief History of Dark Matter Joel Primack University of California, Santa Cruz A Brief History of Dark Matter 1980 - Most astronomers are convinced that dark matter
1. Control system Automatic street light control system using PI controller Aroosa Sheher Sidra Ali Mrayam 2. Dark detector circuitusing LDR LED : Parts list of dark detector:…
PowerPoint PresentationDARK MATTER AND ITS PARTICLE PROPERTIES Jonathan Feng, UC Irvine Dark Matter in Southern California (DaMaSC 2) Keck Institute for Space Studies, Caltech
Conservation of Information: Reverse engineering dark social systemsTitle Conservation of Information: Reverse engineering dark social systems Permalink https://escholarship.org/uc/item/38475290
arXiv:1307.7152 Bremsstrahlung emission bremss and from DM annihilations in halop e+ Indirect Detection: basics Bremsstrahlung emission • Bremss (and related uncertainties)
1 NIGHTSCAPE The 2015 Annual Report Edition 2 3 CHAPTERS Australia ÖsterreichAustria Canada 4 República de ChileChile Česká Republika Czech Republic 中国China4 India…
Models of coupled dark matter to dark energy Alkistis Pourtsidou Department of Physics Astronomy, Bologna University, Italy Work in collaboration with Ed Copeland and Costas…
Βιογραφικό Σημείωμα Προσωπικές Πληροφορίες Όνομα Ιωάννης Ντζούφρας Ημερομηνία γέννησης 14 Φεβρουαρίου…
Looking for SUSY Dark Matter with ATLAS The Story of a Lonely Lepton Nadia Davidson Supervisor: Elisabetta Barberio The Standard Model In high agreement with experimental…
Have neutrinos to do with Dark Energy ? Why neutrinos may play a role Mass scales : Dark Energy density : ρ ~ ( 2×10 -3 eV )- 4. Neutrino mass : eV or below. Cosmological…
The Accelerating Universe,Inflation, & the Dark Energy Ta-Pei Cheng Univ of Missouri - St. Louis Material based on the book “Relativity, Gravitation & Cosmology:…
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…