Cosmological String Solutions by Dimensional Reduction
K. Behrndt, S. Foerste

TL;DR
This paper derives four-dimensional cosmological solutions from five-dimensional black hole configurations within string theory, highlighting the role of a cosmological constant and dilaton potential in shaping cosmological scenarios.
Contribution
It introduces a method to obtain 4D cosmological solutions by reducing 5D black hole and de Sitter solutions in string theory, linking higher-dimensional gravity to cosmology.
Findings
Derived 4D cosmological solutions from 5D black holes
Identified the impact of a 5D cosmological constant on 4D dilaton potential
Discussed cosmological scenarios based on these solutions
Abstract
We obtain cosmological four dimensional solutions of the low energy effective string theory by reducing a five dimensional black hole, and black hole--de Sitter solution of the Einstein gravity down to four dimensions. The appearance of a cosmological constant in the five dimensional Einstein--Hilbert action produces a special dilaton potential in the four dimensional effective string action. Cosmological scenarios implemented by our solutions are discussed. (Talk presented at: ``27th Symposium on the Theory of Elementary Particles'' Wendisch--Rietz, September 7--11, 1993)
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
