Vacuum decay by p-branes production In Print
[Proceedings of the 6th Internationa Symposium on
Frontiers in Fundamental and Computatioanl Physics,
26-29 September 2004, Udine - ITALY]
general relativity, quantum gravity, quantum mechanics, de
Sitter spacetime, anti de-Sitter spacetime, Israel junction
conditions, relativistic shells, WKB (semiclassical) approximation,
N-dimensional generalization.
Project goals:
to generalize to the N-dimensional case
some results about vacuum decay that where obtained by Coleman
and de Luccia in 4-dimensions (and reproduced using general
relativistic shells).
Project results:
in this proceedings we summarize the problem
and show that the generalization is possible; the full computation
can be found elsewhere.
Short Description.
The system under consideration is constituted by a relativistic
shell (described using Israel's junction conditions) which
separates two regions with the de Sitter and/or anti de Sitter
geometries. With at hand the effective momentum of the system,
in the WKB approximation it is possible to compute the transition
coefficient associated with the process of nucleation of a
de Sitter/anti-de Sitter bubble inside a de Sitter/anti-de
Sitter spacetime with different cosmological constant. The
bubble then expands and fill the whole "universe"
, realizing the transitio between what we call "two different
vacua".