Abstract
Necessary conditions are proposed for the admissibility of singular classical solutions with 3 + 1-dimensional Poincaŕe invariance to five-dimensional gravity coupled to scalars. Finite temperature considerations and examples from AdS/CFT support the conjecture that the scalar potential must remain bounded above for a solution to be physical. Having imposed some restrictions on naked singularities allows us to comment on a recent proposal for solving the cosmological constant problem.
Original language | English (US) |
---|---|
Pages (from-to) | 679-745 |
Number of pages | 67 |
Journal | Advances in Theoretical and Mathematical Physics |
Volume | 4 |
Issue number | 3 |
DOIs | |
State | Published - May 2000 |
All Science Journal Classification (ASJC) codes
- General Mathematics
- General Physics and Astronomy