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 : ...
Dunkle Energie. Ein kosmisches Raetsel. Dark Energy. a cosmic ... Uzan,Vangioni. 10/06. variation of Li- abundance. Time variation of coupling constants ...
Observation of (molecular absorption lines. in the light of quasars ) ... Different couplings of cosmon to proton and neutron. Differential acceleration ...
ii) equation of state wh(today) -1. B) Time variation of fundamental 'constants' ... Cosmon mediates new long-range interaction. Range : size of the Universe ...
Quintessence and solution of cosmological constant problem should be related ! ... How can quintessence be distinguished from a. cosmological constant ? ...
Orbits and velocities of stars and galaxies measurement of gravitational potential ... stars , galaxies, clusters. One primordial fluctuation spectrum describes ...
New long - range interaction. cosmon mass changes with time ! for ... ii) equation of state wh(today) -1. B) Time variation of fundamental 'constants' ...
quintessence. fifth force. violation of equivalence principle. time ... Quintessence and time variation of fundamental constants. Strong, electromagnetic, weak ...