One of the most intruiging problems in modern cosmology is that of
dark energy: Why does the expansion of the universe seem to be
accelerating, when standard gravity is attractive? The absence of any
kind of fundamental physical understanding of such seem ingly unnatural
behaviour has led scientists to humorously call the observed universe
preposterous -- a fundamental theory of dark energy is critically
needed.
The current project will explore one specific class of dark energy
candidates, namely those a rising from gravity theories in extra
dimensions. In particular, it will consider Gauss-Bonnet and other
Lovelock gravity theories, which are natural extensions of standard
Einstein gravity in higher dimensions. In four dimensions, these
theories have the potential to describe standard Einstein gravity, now
with naturally incorporated dark energy. Our goal is to determine
whether one or more of these models are physically viable, both at the
classical and quantum level.
The project will be a collaboratio n between members of the theoretical
physics group at the University of Oslo and of the Particle Theory
Group at California Institute of Technology, one of the world's
leading groups in theoretical physics.