1-loop quantum cosmology: the normalisability of the Hartle-Hawking wavefunction and the probability of inflation

Details 1-loop quantum cosmology: the normalisability of the Hartle-Hawking wavefunction and the probability of inflation 1-loop quantum cosmology: the normalisability of the Hartle-Hawking wavefunction and the probability of inflation

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cqgra...7l.181b&link_type=abstract

Class. Quantum Grav., Volume 7, Issue 8, pp. L181-L186 (1990).

Mathematics

Probability

50

Scientific paper

The Hartle-Hawking wavefunction of the Universe is computed in the 1-loop approximation and the general algorithm for the probability of inflation is obtained. Its normalisability is shown to be determined by the anomalous scaling of the theory on the closed Euclidean gravitational instanton. The mechanism of peaking the inflation probability due to 1-loop corrections is proposed for the inflaton scalar field with non-minimal gravitational coupling.

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