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Exploring the High-Energy Universe Rene A. Ong Dept. of Statistics Seminar UCLA Physics Astronomy March 11, 2003 Outline • Introduction – Exploring the universe with…
Bouncing universe in the presence of an extended Chaplygin gas A Salehi* Department of Physics Lorestan University Khoramabad Iran Received 25 December 2015 published 21…
PowerPoint PresentationAtomic Structure and the Fine structure constant α Niels Bohr Erwin Schrödinger Wolfgang Pauli Paul Dirac Lecture Notes Fundamental Constants
Slide 1Why did the Universe Inflate? Slide 2 Proceedings of the Nuffield Workshop, Cambridge, 1982 Slide 3 Old Inflation Scenario Time Space Bubble Nucleation Bubble Collision…
1 Modeling the Universe Chapter 11 HawleyHolcomb Adapted from Dr Dennis Papadopoulos UMCP Spectral Lines - Doppler obs em em z λ λ λ − = 1 em obs z λ λ + = Doppler…
1 Dark Energy, Expansion History of the Universe, and SNAP Dr. Eric Linder, LBL KITP New Cosmology 110502 11 Dark Energy, Dark Energy, Expansion History of the Universe,…
ISAPP 2011 MPIK Heidelberg “The Dark Side of the Universe” Dark Matter phenomenology Thomas Schwetz-Mangold 13 July 2011 T Schwetz 1 Introduction What is the Universe…
Ch 11 - Structure of the Universe 18 - Structure of the Universe Extragalactic Distance Scale Cepheids MV=-3.35logΠ-2.13+2.13(B-V) Π=period (days) Novae MV(max)=-9.96-2.31log(Δm/day)first…
Scalar perturbations in f(R)-cosmology in the late universeJan Novak Jan Novak Department of theoretical physics at Charles University, Prague, Czech republic 11.August 2014
The Inflating Universe Max Tegmark, MIT Max Tegmark Dept. of Physics, MIT [email protected] Bright Horizons Cruise May 13, 2011 Smorga sbord THE COSMIC SMÖRGÅSBORD Galaxy…
AS 4022 Cosmology Lecture 7 Dynamics of the Universe Solutions to the Friedmann Equation for Rt AS 4022 Cosmology Hubble Parameter Evolution -- Hz € H 2 ≡ ˙ R R …
Planck evidence for a closed Universe and a possible crisis for cosmology Eleonora Di Valentino1 Alessandro Melchiorri2 Joseph Silk3456 The recent Planck Legacy 2018 release…
Nemanja Kaloper, UC Davis Forget immortality: the universe will collapse Nemanja Kaloper, UC Davis Λ What is vacuum energy? Consider full matter QFT coupled to semiclassical…
Dark Energy Dark Matter Ordinary Matter 5% Ordinary Matter 25% Dark Matter 70% Dark Energy Dark Energy and the Preposterous Universe Sean Carroll, University of Chicago Our…
Formation and growth of galaxies in the young Universe: progress challenges Simon White Max Planck Institute for Astrophysics Obergurgl. April 2014 Ly α forest spectra and…
Atmospheric CO2 reaches 400 PPM AST101 Lecture 28 The End of the Universe Most Recent Numbers H0 = 67.8 ± 0.8 km/s/Mpc Ω = 0.9995 ± 0.0034 (universe is flat) Age of the…
hera The Structure of the Proton and HERA 1 M.Klein HERA & p Structure 12.5.2009 Max Klein (H1 and ATLAS) 1989 – before HERA The first years Some of today’s results…
Lecture Notes Fundamental Constants 2015 W Ubachs Atomic Structure and the Fine structure constant α Niels Bohr Erwin Schrödinger Wolfgang Pauli Paul Dirac Lecture Notes…
From Einstein to Schücking: Mach’s Principle and Relativistic Cosmology David E Rowe Mainz University On Solving Einstein’s Gravitational Field Equations Einstein’s…
Hans Urs von Balthasar God From his book, Cosmic Liturgy, The Universe according to Maximus the Confessor. Translated by Brian E. Daley, S.J., Ed. A Communio Book Ignatius…