'Weakly interacting massive particles' diaporamas de présentation

THE DARK UNIVERSE

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The Milky Way

The Milky Way. Our home galaxy, full of stars, gas and mysterious dark matter We decompose it into a disk and a halo and a few other parts. Second Exam Results. Mean: 53.7 + 20 pt curve = 73.9 Standard deviation: 10.4 Maximum: 76 raw, 92 curved ; Minimum: 36 raw, 56 curved.

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The PAMELA experiment: looking for antiparticles in Cosmic Rays

Firenze, 25 February 2009. The PAMELA experiment: looking for antiparticles in Cosmic Rays. Oscar Adriani University of Florence and INFN Florence. Outline. The PAMELA experiment: short review Results on cosmic-ray antimatter abundance: Antiprotons Positrons Other results:

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Stefano Scopel

Review of dark matter searches and comments on CMO DM search. Stefano Scopel. International Workshop on Double Beta Decay Search, SNU, Seoul, October 15-17 2009. Daejeon, 24-26 september 2009.

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ASTROPARTICLES IN THE LHC ERA

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Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe

Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe . Unseen Influences. Dark Matter: An undetected form of mass that emits little or no light but whose existence we infer from its gravitational influence

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Galaxies and the Universe

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Th e Bi g Bang

Th e Bi g Bang. D r . Mike MacCallum Long Beach City College mmaccallu m @lbcc.edu. Astrono m y Pictur e o f th e D a y. http://apod.na s a.gov/apod/. ?. Astronome r o f th e W eek. Alan H. Guth. ?.

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Reionization

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The Extreme Universe of Gamma-ray Astronomy

The Extreme Universe of Gamma-ray Astronomy. Professor Lynn Cominsky Department of Physics and Astronomy Sonoma State University. What are Gamma rays?. Why study gamma rays?. Universe as seen by eye is peaceful. The Gamma-ray Sky.

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SPU-22: The Unity of Science from the Big Bang to the Brontosaurus and Beyond

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Chapter 16

Chapter 16 . Dark Matter And The Fate Of The Universe. The Case for Dark Matter. Rotation Curve for the Solar System (This is what we expect to see from the laws of Gravity applied to all the visible mass). Rotation Curve for the Milky Way Galaxy (unexpected).

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Galaxies

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Vibration Analysis of a Cryocooler for CDMS

Vibration Analysis of a Cryocooler for CDMS. Lauren Coutant SULI, summer 2007. What is CDMS?. Cryogenic Dark Matter Search (CDMS) It is known that dark matter exists [1] Best theory: it is Weakly Interacting Massive Particles (WIMPs) [2] CDMS is a direct detection experiment

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Particle Physics and Telescopes

Particle Physics and Telescopes. November 18, 2002. Dark Matter Particle Physics Telescopes. Announcements. Final Exam will be held in Ruby Diamond Auditorium NOTE THIS!!! not UPL Dec. 11, 2002 10am-noon Lenoid shower tonight 4am-sunrise

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Our best fit for all our parameters: What is all that dark matter?

What is the Dark Matter?. Standard Model Particles and Hot Dark Matter. Could It Be Standard Model Particles?. Our best fit for all our parameters: What is all that dark matter? If it is standard model particles, it must be stable Only stable particles are:

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Evidence and Motivation Dual-phase Noble Liquid Detectors Initial Work

Evidence and Motivation Dual-phase Noble Liquid Detectors Initial Work. Evidence for Dark Matter . Astronomical Evidence Galaxy Cluster masses Galaxy rotation curves Gravitational lensing Cosmological Evidence Cosmic Microwave Background (CMB).

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Dark Matter in Cosmology

Dark Matter in Cosmology. Alessandro Palma Dottorato in Fisica XXII ciclo Corso di Cosmologia Prof. A. Melchiorri. Outlook. Why does Cosmology need Dark Matter (DM)? gravitational data from Galaxies and Clusters structure formation in the Universe lensing DM: observed relic density

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Origins : Dark Matter & Dark Energy

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