Thermodynamic Stability of a Multi-Bubble Cosmological Model

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dc.creatorHorwitz, G.
dc.creatorFonarev, O.
dc.date1994-10-20
dc.date.accessioned2026-07-07T03:30:30Z
dc.date.available2026-07-07T03:30:30Z
dc.descriptionMultibubble solutions for a cosmological model which lead to thermal inflationary states due to a semi-classical tunneling of gravity are calculated.
dc.descriptiontalk at Seventh Marcel Grossman Meeting, Stanford, July 1994, 6p, one figure is included
dc.identifierhttps://arxiv.org/abs/gr-qc/9410028
dc.identifierhttp://arxiv.org/abs/gr-qc/9410028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35551
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThermodynamic Stability of a Multi-Bubble Cosmological Model
dc.typetext

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