Thermal/quantum effects and induced superstring cosmologies
| dc.creator | Catelin-Jullien, Tristan | |
| dc.creator | Kounnas, Costas | |
| dc.creator | Partouche, Herve | |
| dc.creator | Toumbas, Nicolaos | |
| dc.date | 2007-10-22 | |
| dc.date | 2009-04-02 | |
| dc.date.accessioned | 2026-07-07T12:58:44Z | |
| dc.date.available | 2026-07-07T12:58:44Z | |
| dc.description | We consider classical superstring theories on flat four dimensional space-times, and where N=4 or N=2 supersymmetry is spontaneously broken. We obtain the thermal and quantum corrections at the string one-loop level and show that the back-reaction on the space-time metric induces a cosmological evolution. We concentrate on heterotic string models obtained by compactification on a T^6 torus and on T^6/Z_2 orbifolds. The temperature T and the supersymmetry breaking scale M are generated via the Scherk-Schwarz mechanism on the Euclidean time cycle and on an internal spatial cycle respectively. The effective field theory corresponds to a no-scale supergravity, where the corresponding no-scale modulus controls the Susy-breaking scale. The classical flatness of this modulus is lifted by an effective thermal potential, given by the free energy. The gravitational field equations admit solutions where M, T and the inverse scale factor 1/a of the universe remain proportional. In particular the ratio M/T is fixed during the time evolution. The induced cosmology is governed by a Friedmann-Hubble equation involving an effective radiation term ~1/a^4 and an effective curvature term ~1/a^2, whose coefficients are functions of the complex structure ratio M/T. | |
| dc.description | v4: 57 pages, 9 figures, modified discussion on Wilson lines | |
| dc.identifier | https://arxiv.org/abs/0710.3895 | |
| dc.identifier | http://arxiv.org/abs/0710.3895 | |
| dc.identifier | Nucl.Phys.B797:137-178,2008 | |
| dc.identifier | doi:10.1016/j.nuclphysb.2007.12.030 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/225342 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Thermal/quantum effects and induced superstring cosmologies | |
| dc.type | text |