106 research outputs found
Matter Contributions to the Expansion Rate of the Universe
We consider the effect of various particles on the cosmic expansion rate
relative to that of the graviton. Effectively massless fermions, gauge bosons
and conformally coupled scalars make only minuscule contributions due to local
conformal invariance. Minimally coupled scalars can give much stronger
contributions, but they are still sub-dominant to those of gravitons on account
of global conformal invariance. Unless effectively massless scalar particles
with very particular couplings exist, the leading effect on the expansion rate
is furnished solely by the graviton. An upper bound on the mass of such scalar
particles is obtained.Comment: 14 pages, plain TeX, 7 Postscript files, uses psfig.st
Quantum Gravity Slows Inflation
We consider the quantum gravitational back-reaction on an initially
inflating, homogeneous and isotropic universe whose topology is . Although there is no secular effect at one loop, an explicit calculation
shows that two-loop processes act to slow the rate of expansion by an amount
which becomes non-perturbatively large at late times. By exploiting Feynman's
tree theorem we show that all higher loops act in the same sense.Comment: 19 pages, plain TeX, 1 Postscript file, uses psfig.sty, revised June
1996 for publication in Nuclear Physics
Pair creation and axial anomaly in light-cone
The 1+1 dimensional massive Dirac equation is solved exactly in light-cone
coordinates for and , in the presence of an arbitrary
dependent electric field. Our solution resolves the ambiguity at . We
also obtain the one loop rate for pair production for a positive electric
field, compute the expectation values of the vector and axial vector currents,
and recover the well known anomaly in the divergence of the latter.
A final intriguing result is that the theory seems to exhibit a phase
transition in the limit of infinite .Comment: 33 pages, 2 figures, LaTeX 2 epsilon, revised for publicatio
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