PPT-Fifty Years of CMB Anisotropy Experiments (and Theory)

in 15 Minutes Bruce Partridge Haverford College bpartridhaverfordedu A Brief History in 6 epochs Epoch 1 1965 to 1970 Isotropy as one test of the cosmic origin of the CMB Flavor Are we right. & Large scale structure. Tarun Souradeep. I.U.C.A.A. .. Cosmology . IUCAA . VSP program. (. May 18-22, . 2012). Lec. . 2:. Cosmic Content. Perturbed Universe . Simple. … yet, an . exotic. Gaussianities. Antony Lewis. http://cosmologist.info/. Lewis . arXiv:1107.5431. Hanson . & Lewis . arXiv:0908.0963. Lewis, Challinor & Hanson . arXiv:1101.2234. Pearson, Lewis & Regan . arXiv:1201.1010. Bruce Partridge. Haverford College. bpartrid@haverford.edu. Thanks…. Start with thanks:. To funding agencies for supporting CMB research. To ICISE. To the organizers for giving me a chance to relive the early days of CMB science. Shear alignment of olivine crystals. Shear wave splitting. c. a. Olivine Anisotropy: Basic (A-type). [1 0 0] (. a. -axis) parallel to flow direction. (0 1 0) plane parallel to flow plane. Horizontal flow . Scott . Dodelson. Hogan Nguyen. 4/23/2010. 1. FCPA Retreat. Physics Beyond the Standard Model. 4/23/2010. 2. FCPA Retreat. Dark Matter. . Dark Energy. . Inflation. . Neutrino Mass. 4/23/2010. FCPA Retreat. Pankaj Jain . I.I.T. Kanpur. Introduction. Universe is assumed to be homogeneous and isotropic at large distance scales. No preferred position or direction . . Towards the first detection using SPT polarisation. ASA 2016 meeting, . Sydney. 04. 07. 2016. Srinivasan. . Raghunathan. School of Physics. University of Melbourne. In a nutshell . …. . South Pole Telescope – Observes CMB (both T, and P).. Activities funded by NASA proposal: . PI Steve Meyer entire CMB community. Workshops:. The Path to CMBPOL: Upcoming Measurement of CMB Polarization, Chicago July 1-3, 2009. Technology Development for a CMB Probe of Inflation, Boulder, 25-28 August 2008. Alexander . Polnarev. QMUL, School of Physics and Astronomy, London, UK. Tarusa. , 10 September 2015. Talk Overview:. Introduction: . Free electrons + Anisotropy = Polarization. The History of Polarization in Cosmology: . . In order to simulate the performance of an interferometer, 20 by 20 degree sections were extracted from the simulated CMB map. For each array configuration tested a map of . uv. plane coverage was created and then applied to the Fourier transform of the CMB section. The power spectra were then extracted by computing the variance in an annulus with a radius given by the . . In order to simulate the performance of an interferometer, 20 by 20 degree sections were extracted from the simulated CMB map. For each array configuration tested a map of . uv. plane coverage was created and then applied to the Fourier transform of the CMB section. The power spectra were then extracted by computing the variance in an annulus with a radius given by the . Zhuo ChengSupervisors Yi Mao and Jianfeng Zhou1OutlineAn introduction to CMBCOBEInstrumentScientific resultsAnisotropy of CMBWMAPCompare to COBEScientific resultsSummary2The origin of CMB3Before recom From Mays, 2011, Ground and Surface Water Hydrology. Effective conductivity . that represents aggregate effect of flow through a layered system. Effective conductivity is . different. parallel to than perpendicular to the layers. & Aviram . Rosochotsky. 1. The structure of the presentation. A Reminder on the derivation the Planck spectral distribution function.. Detailed exposition of Ford and O’Connell’s derivation of the spectral distribution of a radiation cavity in a moving frame of reference..