PPT-CMB Polarization generated by cosmological gravitational waves
Author : donetrand | Published Date : 2020-07-02
Alexander Polnarev QMUL School of Physics and Astronomy London UK Tarusa 10 September 2015 Talk Overview Introduction Free electrons Anisotropy Polarization
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CMB Polarization generated by cosmological gravitational waves: Transcript
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 . MBAF Certified Mortgage Banker Society. The Certified Mortgage Banker (CMB) Designation is the industry standard of professional success. It symbolizes respect, credibility, ethics, and achievement within real estate finance. . Microwave . Background. and Its Polarization . A New . & Ultimate Tool . for Cosmology and Particle Physics. Naoshi. . Sugiyama. Nagoya University. Taup2007@Sendai. Cosmic Microwave Background. 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. 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 . some history. (based on D. . Kennefick’s. work). Historical tidbits. 1776: Laplace suggests four mechanisms that could explain secular perturbations of Moon-Earth orbit. One the explanations was a non-instantaneous propagation of gravity, affecting the binary system (abandoned because its speed would be too large to be measurable to explain the effect). . (& Gravitons ?). -. Vishal. . Kasliwal. Classical Electromagnetism. Vacuum. Maxwell Field Equations. Light!!. Electromagnetic waves. Quantum Electromagnetism. Hamiltonian of Quantized. Field. where. & 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. 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 . &. 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. Gravitational Waves. Prediction. General Relativity – 1915. Gravity is not the pulling force envisioned by Kepler or Newton. Space warps around massive objects. Accelerating massive objects could radiate distortions like the wake of a boat. 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. . 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 . Jamie Bock . (Caltech/JPL). PhysPAG. Meeting, . HEAD . @ . Chicago. . 19 August 2014. 2. Testing Inflation with CMB Polarization. Key Inflationary Observables. . First Definitive CMB Result. Nearly scale-invariant fluctuations. gravitational. . waves. by. Laser-plasma . interaction. . Hedvika . Kadlecová. . a. , . S. Weber . a. , G. Korn. a . a. . Institute of Physics, v.v.i. ASCR, Na Slovance 1999, Prague, Czech Republic;.
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