English

Cosmological Constant in Low Energy $d = 4$ String Leads to Naked Singularity

High Energy Physics - Theory 2010-11-19 v2 General Relativity and Quantum Cosmology

Abstract

In the sigma model approach, the β\beta-function equations for non critical strings contain a term which acts like a tree level cosmological constant, Λ\Lambda. We analyse the static, spherically symmetric solutions to these equations in d=4d = 4 space time and show that the curvature scalar seen by the strings is singular if Λ0\Lambda \ne 0. This singularity is naked. Requiring its absence in our universe imposes the constraint Λ<10120| \Lambda | < 10^{- 120} in natural units. {}From another point of view, our analysis implies that low energy d=4d = 4 non critical strings lead to naked singularities.

Keywords

Cite

@article{arxiv.hep-th/9402009,
  title  = {Cosmological Constant in Low Energy $d = 4$ String Leads to Naked Singularity},
  author = {S. Kalyana Rama},
  journal= {arXiv preprint arXiv:hep-th/9402009},
  year   = {2010}
}

Comments

13 pages, preprint TCD-1-94. Revised version: a note and some references added; a few minor changes in the text