PPT-CMB Decadal Study: What We Did

Author : debby-jeon | Published Date : 2018-09-21

Activities funded by NASA proposal PI Steve Meyer entire CMB community Workshops The Path to CMBPOL Upcoming Measurement of CMB Polarization Chicago July 13 2009

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CMB Decadal Study: What We Did: Transcript

Activities funded by NASA proposal PI Steve Meyer entire CMB community Workshops The Path to CMBPOL Upcoming Measurement of CMB Polarization Chicago July 13 2009 Technology Development for a CMB Probe of Inflation Boulder 2528 August 2008. & 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. a prospect from galaxy evolution. Cosmic Microwave Background Radiation and Its Foreground Interstellar Components, Tokyo. , . 17. th. February, 2010. Tsutomu T. TAKEUCHI. Institute for Advanced Research, Nagoya University, Japan. The value of . reionization. fraction derived from CMB polarization measurements has decreased steadily since WMAP2003 (WMAP2005, WMAP2007, WMAP2011, and Planck 2015). The final word from Planck is not out yet , and whenever it is out, it will surely not be “a 100-sigma measurement” of . Uro. š. . Seljak. UC Berkeley/LBNL. Dec 18. 2014. Goals and methods. Goals: testing Lambda CDM model . . and its e. xtensions . Testing inflation. Methods: redshift distance relation (SN, BAO…) . & Large scale structure. Tarun Souradeep. I.U.C.A.A. .. Cosmology . IUCAA . VSP program. (. May 18-22, . 2012). Lec. . . 4:. Current frontiers. Mildly Perturbed universe at z=1100. Present universe at z=0. Antony Lewis. http://cosmologist.info/. Lewis . arXiv:1204.5018. see also . Creminelli. . et al . astro-ph. /0405428, . arXiv:1109.1822, . Bartolo. et al arXiv:1109.2043. Lewis . arXiv:1107.5431. Lewis. Two-Way . Land/Atmosphere/Ocean . I. nteractions. Yongkang Xue. 1. , F. De Sales, Z. Zhang, Y. Wang, . Y. Liu. , H.-Y. Ma. , L. Marx, M. Ek, R. Yang, J.-W. Lee. 1. University of California, Los Angels . and Large-Scale Structure. 1. Cora Dvorkin. IAS (Princeton) Harvard (Hubble fellow) . COSMO 2014. August 2014, Chicago. Outline. Dark Matter overview.. Effect of . WIMP Dark Matter . Gaussianity. measurement. Dr. . Rajib. . Saha. Assistant Professor. Physics Department. IISER Bhopal. INDO-UK Scientific Seminar: Confronting particle cosmology with PLANCK and LHC . IUCAA, August 11, 2011. &. Primordial Gravitational Waves. Jun-Qing Xia. Key Laboratory of Particle Astrophysics, IHEP. Planck Member. CHEP, PKU, April 3, 2014. BICEP2. . Paper (arXiv:1403.3985). 2. Tensor Modes Detection by BICEP2. A community-driven initiative to harmonize data practices, research priorities and infrastructure for 2025. Carol B. Meyer. Foundation for Earth Science. September 23, 2013. Overview. 1. About . ESIP. 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 .

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