362 research outputs found
Can the cosmological constant undergo abrupt changes?
The existence of a simple spherically symmetric and static solution of the
Einstein equations in the presence of a cosmological constant vanishing outside
a definite value of the radial distance is investigated. A particular
succession of field configurations, which are solutions of the Einstein
equations in the presence of the considered cosmological term and auxiliary
external sources, is constructed. Then, it is shown that the associated
succession of external sources tend to zero in the sense of the generalized
functions. The type of weak solution that is found becomes the deSitter
homogeneous space-time for the interior region, and the Schwartzschild space in
the outside zone.Comment: 10 pages, 1 figur
Exploring effects of strong interactions in enhancing masses of dynamical origin
A previous study of the dynamical generation of masses in massless QCD is
considered from another viewpoint. The quark mass is assumed to have a
dynamical origin and is substituted by a scalar field without self-interaction.
The potential for the new field background is evaluated up to two loops.
Expressing the running coupling in terms of the scale parameter , the
potential minimum is chosen to fix when .
The second derivative of the potential predicts a scalar field mass of 126.76
. This number is close to the value 114 which, preliminary data
taken at CERN, suggested to be associated with the Higgs particle. However, the
simplifying assumptions limit the validity of the calculations done, as
indicated by the large value of obtained.
However, supporting statements about the possibility of improving the scheme
come from the necessary inclusion of weak and scalar field couplings and mass
counterterms in the renormalization procedure, in common with the seemingly
needed consideration of the massive W and Z fields, if the real conditions of
the SM model are intended to be approached.Comment: 10 pages, 4 figures, a numerical error was corrected as well as the
values of the estimated parameters which it determined. The discussion and
arguments were also improve
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