22,854 research outputs found

    Vacuum energy and cosmological evolution

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    An expanding universe is not expected to have a static vacuum energy density. The so-called cosmological constant Λ\Lambda should be an approximation, certainly a good one for a fraction of a Hubble time, but it is most likely a temporary description of a true dynamical vacuum energy variable that is evolving from the inflationary epoch to the present day. We can compare the evolving vacuum energy with a Casimir device where the parallel plates slowly move apart ("expand"). The total vacuum energy density cannot be measured, only the effect associated to the presence of the plates, and then also their increasing separation with time. In the universe there is a nonvanishing spacetime curvature RR as compared to Minkowskian spacetime that is changing with the expansion. The vacuum energy density must change accordingly, and we naturally expect δΛ∼R∼H2\delta\Lambda\sim R\sim H^2. A class of dynamical vacuum models that trace such rate of change can be constructed. They are compatible with the current cosmological data, and conveniently extended can account for the complete cosmic evolution from the inflationary epoch till the present days. These models are very close to the Λ\LambdaCDM model for the late universe, but very different from it at the early times. Traces of the inherent vacuum dynamics could be detectable in our recent past.Comment: Slightly extended discussion, typos corrected and references adde

    The Top-Quark Width in the Light of ZZ-Boson Physics

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    We discuss possible non-standard contributions to the top-quark width, particularly the virtual effects on the standard decay t→W+ bt\rightarrow W^+\,b within the context of the MSSM. We also place a renewed emphasis on the unconventional mode t→H+ bt\rightarrow H^+\,b in the light of recent analyses of ZZ-boson observables. It turns out that in the region of parameter space highlighted by ZZ-boson physics, the charged Higgs mode should exhibite an appreciable branching fraction as compared to the standard decay of the top quark. Remarkably enough, the corresponding quantum effects in this region are also rather large, slowly decoupling, and most likely resolvable in the next generation of experiments at Tevatron and at LHC.Comment: One new figure added, with supplementary comments. 17 pages, LaTeX, 2 figures included via psbox. A postcript version can be obtained from anonymous ftp at ftp://ftp.ifae.es/preprint/ft/uabft372.ps Talk presented at the Workshop on Physics of the Top Quark, Iowa State University, May 199
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