Towards the Standard Cosmological Model. Andrei Linde. Cosmology: A general outlook ... String Cosmology and the Gravitino Mass. Kallosh, A.L. 2004. VAdS. uplifting ...
Probing the Reheating with Astrophysical Observations J r me Martin Institut d Astrophysique de Paris (IAP) [In collaboration with K. Jedamzik & M. Lemoine, arXiv ...
Eden in Paris 05. The Quintessence Field during Inflation. J r me Martin ... Eden in Paris 05. Quintessence ... Eden in Paris 05. Quantum effects. The ...
Title: INFLU NCIAS DA EXPANS O DO UNIVERSO NA EVOLU O DO SISTEMA SOLAR Author: Usuario InfoWay Last modified by: nelson Created Date: 6/17/1995 11:31:02 PM
... Copeland, Liddle, Lyth, Stewart, Wands and Dine, Randall, Thomas Moduli Problem Several extra scalar fields - needs to make them heavy (Dine) Scalar fields ...
The Maier-Leibnitz-Laboratory for Nuclear and Particle Physics of LMU ... Plot by Ryan Winkler (Yale) - (p,t) reactions. using 25 MeV protons. 3-5 angles. MLL ...
Andrei Linde Lecture 1 Plan of the lectures: Inflation: a general outlook Basic inflationary models (new inflation, chaotic inflation, hybrid inflation) Creation of ...
William R. Salaneck Prof. of surface physics and chemistry, LiU ... Intercalation materials for batteries. Hybrid interfaces in solar cell applications ...
Dunkle Energie. Ein kosmisches Raetsel. Dark Energy. a cosmic ... Uzan,Vangioni. 10/06. variation of Li- abundance. Time variation of coupling constants ...
Gauge invariance: SU(2) invariance at each vertex. becomes SU(2) ... Schur's duality. is the irrep of the permutation group. Example: =#standard tableaux ...
advertisement: see talk by Andy Mennim on Monday! primordial perturbations from scalar fields ... Lyth & Rodriguez (2005) non-Gaussianity from curvaton decay ...
ii) equation of state wh(today) -1. B) Time variation of fundamental 'constants' ... Range : size of the Universe horizon. Strength : weaker than gravity ...
( M : reduced Planck-mass , H : Hubble parameter ) Ob=?b/?c. fraction in baryons ... picture of the big bang. Otot=1. WMAP 2006. Polarization. Dark Energy. Om ...
fire , air, water, soil ! Dark Energy. dominates the Universe. Energy - density in the Universe ... Jordan,... Standard Model of. electroweak interactions : ...
... phase modulator, one needs an interferometer, which is now available in VUV ... a proposal for installation of the interferometer in the UV/VUV beamline ...
Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006 ... Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006. The zoo plot in ( 2, 1) plane ...
Remote regions are strikingly different from. what we observe here. ... Shortest man: Gul Mohammed, 0.56 m Guinness Book. Tallest man: Robert Wadlow, 2.72 m of Records ...
Galileo Galilei Physics Dept., Padova ... Effects on the inflationary observables from the so ... A possibility is to try to resum these potentially large ...
Old view: Theory prior = delta function of THE correct one and only theory ... DUNE-WL (50% sky, gals @z = 0.1-1.1, 35/min2 ) Planck1yr. es=0.02 0.07-0.06 ...
... of a non zero Jeans length. Oscillating behavior of the dark fluid perturbations below the Jeans length ... Defining an effective Jeans length , we obtain ...
Since GWs propagate freely after being generate, they keep the information on their source. Detection of GWs could open a window into new physics (parity symmetry ...
Institute for Theory and Computation, Harvard-Smithsonian Center for ... Prelude. In this poster, I discuss how back-reaction of large amplitude inhomogeneities ...