PPT-Probing Dark Matter with the CMB

Author : alexa-scheidler | Published Date : 2016-09-19

and LargeScale Structure 1 Cora Dvorkin IAS Princeton Harvard Hubble fellow COSMO 2014 August 2014 Chicago Outline Dark Matter overview Effect of WIMP Dark Matter

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Probing Dark Matter with the CMB: Transcript


and LargeScale Structure 1 Cora Dvorkin IAS Princeton Harvard Hubble fellow COSMO 2014 August 2014 Chicago Outline Dark Matter overview Effect of WIMP Dark Matter . Microwave . Background. and Its Polarization . A New . & Ultimate Tool . for Cosmology and Particle Physics. Naoshi. . Sugiyama. Nagoya University. Taup2007@Sendai. Cosmic Microwave Background. 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. & 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. Paul McMillan. Surveys For All, 1st February 2016 . Why do we care?. On the biggest scales, the ΛCDM model works. Why do we care?. On the scale of individual galaxies, agreement is less obvious.. Things are more complicated, we have to consider the baryons. 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).. Cody . Carr. , Minh Nguyen. December 9. th. , 2014.. Agenda. Motivations (Cosmic & Atomic scales). Dark Matter categories. The Dark Matter Zoo. Neutrinos. Neutralinos. Kaluza. -Klein particles. Summary. Guo. 《. 现代宇宙学. 》. 2017.5.27. O. utline. §. Background. M. odern cosmology. Cosmic Microwave Background (CMB) radiation. §. . CMB . anisotropy theory. §. CMB . experiments. §. Cosmological . National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . SCIENCE. . PEOPLE TECHNOLOGY. Scientists Discover Galaxy that is 99.99 Percent Dark Matter. Dr. Simona . Murgia. (UC, Irvine). Dr. Will Dawson (Lawrence Livermore National Laboratory). Carolyn Slivinski (STScI). Facilitator: Dr. Emma Marcucci (STScI). Science Briefing. October . 5. , 2017. Sahil. Singla. . (Carnegie Mellon University). Joint . Work (. Partly) With . ANUPAM GUPTA . and . VISWANATH NAGARAJAN. (2. nd. Feb, 2018). Combinatorial Optimization. Given a . Finite . Universe. Uri Zwick. Tel Aviv University. Started: . April . 2015. Last update: . January 12, 2017. Hashing with open addressing. “Uniform probing”. Insert key . in the first free position among.  . (Sometimes) assumed to be a . Carisa Petris, Don Liu . Issue . 7. , 2017. A presentation to:. Meeting name. Date. Table of Contents. 01. Background. 02. Types. of studies. 03. Key results. 04. Tables (Risk of Bias/Forest Plots). Perimeter Explorations 01. CERN HST2019 . Uniform Circular Motion. Predict. Observe. Explain. How are . mass. and . speed. connected in circular motion?. mass. speed. Uniform Circular Motion. Objective: .

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