Energy density and spatial curvature in general relativity

Theodore Frankel, Gregory J. Galloway

Research output: Contribution to journalArticle

14 Scopus citations

Abstract

Positive energy density tends to limit the size of space. This effect is studied within several contexts. We obtain sufficient conditions (which involve the energy density in a crucial way) for the compactness of spatial hypersurfaces in space-time. We then obtain some results concerning static or, more generally, stationary space-times. The Schwarzchild solution puts an upper bound on the size of a static spherically symmetric fluid with density bounded from below. We derive a result of roughly the same nature which, however, requires no symmetry and allows for rotation. Also, we show that static or rotating universes with Λ=0 require that the density along some spatial geodesic must fall off rapidly with distance from a point.

Original languageEnglish (US)
Pages (from-to)813-817
Number of pages5
JournalJournal of Mathematical Physics
Volume22
Issue number4
StatePublished - Dec 1 1980

ASJC Scopus subject areas

  • Statistical and Nonlinear Physics
  • Mathematical Physics

Fingerprint Dive into the research topics of 'Energy density and spatial curvature in general relativity'. Together they form a unique fingerprint.

  • Cite this