Radiation Field on Superspace

dc.creatorGonzalez-Diaz, P. F.
dc.date1994-03-18
dc.date.accessioned2026-07-07T03:30:17Z
dc.date.available2026-07-07T03:30:17Z
dc.descriptionWe study the dynamics of multiwormhole configurations within the framework of the Euclidean Polyakov approach to string theory, incorporating a modification to the Hamiltonian which makes it impossible to interpret the Coleman Alpha parameters of the effective interactions as a quantum field on superspace, reducible to an infinite tower of fields on space-time. We obtain a Planckian probability measure for the Alphas that allows $\frac{1}{2}α^{2}$ to be interpreted as the energy of the quanta of a radiation field on superspace whose values may still fix the coupling constants.
dc.description13, IMAFF-RC-01-94#
dc.identifierhttps://arxiv.org/abs/gr-qc/9403037
dc.identifierhttp://arxiv.org/abs/gr-qc/9403037
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35486
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRadiation Field on Superspace
dc.typetext

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