Elementary Particles, Volume 92N. Cabibbo, Società italiana di fisica |
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Page 167
... constant can given a pseudo - Newtonian interpretation as a Klein - Gordon modification the Poisson equation [ 63 ] : 13 ) = - = For the time being , let us set 0. ( I will discuss the case of a non- ishing cosmological constant in sect ...
... constant can given a pseudo - Newtonian interpretation as a Klein - Gordon modification the Poisson equation [ 63 ] : 13 ) = - = For the time being , let us set 0. ( I will discuss the case of a non- ishing cosmological constant in sect ...
Page 186
... constant ( 4 > 0 ) . solution is - ( 2.72 ) Ꭱ R = R , exp [ Ht ] , with constant Hubble parameter ( 2.73 ) H = ( 1/3 ) . = There are analogous solutions for k +1 and k = -1 with Rx cosh and Roc sinh Ht , respectively . The scale factor ...
... constant ( 4 > 0 ) . solution is - ( 2.72 ) Ꭱ R = R , exp [ Ht ] , with constant Hubble parameter ( 2.73 ) H = ( 1/3 ) . = There are analogous solutions for k +1 and k = -1 with Rx cosh and Roc sinh Ht , respectively . The scale factor ...
Page 189
... constant is probably vanishingly small after inflation , which implies ( in the absence of a osmological constant today ) that 2,1 to a very high degree of accuracy . However , in view of our lack of knowledge of the true dynamics of ...
... constant is probably vanishingly small after inflation , which implies ( in the absence of a osmological constant today ) that 2,1 to a very high degree of accuracy . However , in view of our lack of knowledge of the true dynamics of ...
Contents
Leptonic processes | 22 |
Measurements of the W and Z masses at the SPS collider | 39 |
the spectator model | 50 |
Copyright | |
41 other sections not shown
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amplitude Astron Astrophys baryonic bosons calculations cD galaxies chiral cold-DM collapse component constant constraint continuum correlation corresponding cosmological cosmological constant coupling dark matter decay Dirac discuss disk dynamics edited effective electron energy equation factor fermions field finite fluctuations function gauge group gauge theory gluons gravitino gravity halos Higgs horizon Hubble implies interactions invariance Jeans mass Lagrangian lattice lepton lepton number Lett limit luminosity Majorana massless matrix multiplet N-body simulations neutrino masses node Nucl observed parameter particle physics particles perturbation photon Phys physical possible preon primordial problem quantum quark R. D. PECCEI radiation radius red-shift renormalizable renormalization result rich clusters scalar scale sect simulations spectrum spin spinor structure SU₂ superclusters superfields supergravity superspace supersymmetry symmetry transformation U₁ Universe vector velocity virial W-bosons Weyl Yang-Mills ZEL'DOVICH