Self-acceleration in scalar-bimetric theories
Texte intégral
Figure
Documents relatifs
Indeed, in Planck Collaboration V (2020), the probability density of the polarised spectra at low multipoles was modelled with a polynomial function adjusted on simulations in
In section IV A we illustrate the existence of the GMFP and the properties of the RG flow near the GMFP in specific truncations where scalar matter fields are coupled nonminimally
We think of scalar curvature as a Riemannin incarnation of mean cur- vature (1) and we search for constraints on global geometric invariants of n-spaces X with Sc(X) > 0 that
(5.1) dominates and σ SI is of the same order of magnitude as in the non-composite case. By comparing with Fig. 1, one remarks that the correct relic density can be reproduced by m η
In the dark dark town there is a dark dark street.. In the dark dark street there is a dark
Write how the field φ(x) transforms under the action of an element of the Poincar´ e group.. Show that it is reducible and do the reduction in terms of irreducible
which admits a is of course a necessary condition for an asymptotic condition in time and a scattering theory with a particle interpretation on the space
One of us (Cantor [6]) has shown that the solvability of the Lichnerowicz-York equation for asymptotically flat maximal slices is equivalent to the given metric