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We study solutions of the Wheeler-DeWitt equation corresponding to an S-modular invariant N=1 supergravity model and a closed homogeneous and isotropic Friedmann-Robertson-Walker spacetime. The issues of inflation and of the cosmological constant problem are addressed with the help of the relevant wave functions. We find that topological type inflation is consistent from the quantum mechanical point of view and that a solution for the cosmological constant problem along the lines of the strong CP problem naturally arises.
Latex, 23 pages, 1 figure. Revised version to appear in Classical and Quantum Gravity
High Energy Physics - Theory, High Energy Physics - Theory (hep-th), Wheeler-De Witt equation, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Quantization of the gravitational field, inflation, strong CP problem, General Relativity and Quantum Cosmology, Relativistic cosmology, modular invariant supergravity, Friedmann-Robertson-Walker spacetime
High Energy Physics - Theory, High Energy Physics - Theory (hep-th), Wheeler-De Witt equation, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Quantization of the gravitational field, inflation, strong CP problem, General Relativity and Quantum Cosmology, Relativistic cosmology, modular invariant supergravity, Friedmann-Robertson-Walker spacetime
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 12 | |
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influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |