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Is cosmology a solved problem? Bepaling van ΩDM met behulp van gravitatie lenzen gevormd door clusters Is cosmology a solved problem? Abell 2218, een cluster lens waarvan…
PHY306 1 Modern cosmology 2: Type Ia supernovae and Λ Distances at z ~1 Type Ia supernovae SNe Ia and cosmology Results from the Supernova Cosmology Project, the High z…
EE Cep eclipse in 2014 - an international observational campaign The 11-th magnitude star EE Cep is a member of rare class of binary systems in which the eclipses are caused…
RELIC NEUTRINOS: NEUTRINO PROPERTIES FROM COSMOLOGY Sergio Pastor (IFIC) ν RELIC NEUTRINOS: OUTLINE Massive neutrinos Standard neutrinos Extra radiation and Neutrino asymmetries…
ICE/CSIC & IEEC Pizza-Lunch Seminar ICE-IEEC, Bellaterra, 9 Oct 2015 • 1917 Einstein found from his equations of GR a static model of the Universe, by introducing
Martin Bojowald The Pennsylvania State University General relativity determines dynamics and structure of space-time. 1. Background independence. Space-time structure may
ar X iv :0 80 8. 07 46 v1 [ he p- th ] 5 A ug 2 00 8 1 Progress of Theoretical Physics, Vol. 111, No. 4, April 2004 String Gas Cosmology LATEX2ε Version Robert H. Brandenberger∗)…
Has elasticity anything to do with cosmology? Angelo Tartaglia RELGRAV February 17 2011 RELGRAV * “Elastic” continua xμ ξa N+n N N RELGRAV * Geometry and elasticity…
MCMC of the CMB power spectrum, and convergence Zubair and Jen Cosmology 321 ● Random samples of parameter space ● Use CAMB for numerical calculation of Cl ● Calculate…
PROBING THE INHOMOGENEOUS UNIVERSE WITH GW COSMOLOGY Kent Yagi Kyoto University (Montana State Univ. from next April) Amaldi 2011 ＠ Cardiff 7/10 2011 Atsushi Nishizawa…
Observational Test of Halo Model: an empirical approach Mehri Torki Bob Nichol Two types of pairs: both particles in same halo, or particles in different halos ξdm(r) =…
Microsoft PowerPoint - Standard Cosmology II.ppt Red shiftRed shift Hubble lawHubble law Astroparticle Course 2 The full solutions to the Friedmann equations can be quite
4 Friedmann–Robertson–Walker Universe We shall now apply the Einstein equation to the homogeneous and isotropic case, which leads to Friedmann–Robertson–Walker (FRW)…
Ψ-Epistemic Quantum Cosmology Peter W Evans∗1 Sean Gryb†2 and Karim P Y Thébault‡3 1School of Historical and Philosophical Inquiry University of Queensland 2Institute…
Slide 1Ch. 23 - Cosmology Part 2 The Beginning & the End Slide 2 Skip Forward to 1964 Penzias & Wilson discover isotropic emission at λ=7.35 cm. If a blackbody,…
by Tomislav Prokopec A. The Friedmann-Lamatre-Robertson-Walker (FLRW) cosmology 1. The metric tensor We now consider the most general homogeneous space times, the Friedmann-Lematre-Robertson-
Slide 1 An Overview of Modern Cosmology Strings, Gravity and Locality: Slide 2 Physics at the Dawn of the 20 th Century: The Clockwork Universe Newton’s Third Law of Motion…
[ G eV ] tX [ sec ] 3He / D FIRAS 3 FIG. 1: The matter field at z = 99 for various PBH fractions. The PDM density field is represented by the colormap with white points indicating
1 COSMOLOGY Lecturer: Professor Komissarov SS Room: 1019 in Maths Satellite email: SSKomissarov@leedsacuk 2016 Contents Contents 2 1 Introduction 5 2 Euclidean plane 6 21…
Wayne Hu STScI, May 2008 The Cosmology of f (R) Models for Cosmic Acceleration Why Study f (R)? • Cosmic acceleration, like the cosmological constant, can either be viewed…