'Wmap data' presentation slideshows

5-year Results from WMAP with a Glimpse Ahead

486 views • 39 slides

AY202a Galaxies & Dynamics Lecture 18: Galaxy Clusters & Cosmology

508 views • 37 slides

IPv6 Background Radiation

IPv6 Background Radiation. Geoff Huston George Michaelson APNIC R&D. Radiation Detection. The Holmdel Horn Antenna, at Bell Labs, on which Penzias and Wilson discovered the cosmic microwave background radiation.

486 views • 36 slides

LHC, NUOVA FISICA E MATERIA OSCURA

448 views • 35 slides

Weighing neutrinos with Cosmology

419 views • 30 slides

Supersymmetric B-L Extended Standard Model with Right-Handed Neutrino Dark Matter

Supersymmetric B-L Extended Standard Model with Right-Handed Neutrino Dark Matter. Nobuchika Okada. University of Alabama Tuscaloosa, AL. In collaboration with Zachary M. Burell (U. of Alabama). Paper in preparation. Miami 2010 @ Fort Lauderdale, Dec. 14-19, 2010.

416 views • 26 slides

Astrometry and the expansion of the universe

Astrometry and the expansion of the universe. Michael Soffel & Sergei Klioner TU Dresden. Fundamental object for astrometry: metric tensor g. ??. IAU -2000 Resolutions: BCRS (t, x ) with metric tensor. BCRS-metric is asymptotically flat; ignores cosmological effects,

390 views • 25 slides

Significant effects of second KK particles on LKP dark matter physics

Collaborated with Mitsuru Kakizaki (ICRR) Shigeki Matsumoto (ICRR) Yoshio Sato (Saitama U.). Significant effects of second KK particles on LKP dark matter physics. Masato Senami (ICRR, University of Tokyo) senami@icrr.u-tokyo.ac.jp. hep-ph/0502059. Kaluza-Klein dark matter.

336 views • 22 slides

Limits on non-Gaussianities from WMAP 3yr data

Paolo Creminelli (ICTP, Trieste). Limits on non-Gaussianities from WMAP 3yr data. astro-ph/0610600 with L. Senatore, M. Zaldarriaga and M. Tegmark. Is there any correlation among modes?. OUTLINE. Standard slow roll inflation predicts very small NG: NG < 10 -6

337 views • 21 slides

Limits on non-Gaussianities from WMAP 3yr data

Paolo Creminelli (ICTP, Trieste). Limits on non-Gaussianities from WMAP 3yr data. astro-ph/0610600 with L. Senatore, M. Zaldarriaga and M. Tegmark. Is there any correlation among modes?. OUTLINE. Standard slow roll inflation predicts very small NG: NG < 10 -6

217 views • 21 slides

Modern cosmology 4: The cosmic microwave background

Modern cosmology 4: The cosmic microwave background. Expectations Experiments: from COBE to Planck COBE ground-based experiments WMAP Planck Analysis Results. Analysis of WMAP data: the power spectrum. Resolution and sky coverage

256 views • 14 slides

Congresso del Dipartimento di Fisica Highlights in Physics 2005

137 views • 1 slides