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Cosmology, cohomology and compactification

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C G Torre

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LETTER TO THE EDITOR

Ashtekar and Samuel have shown that Bianchi cosmological models with compact spatial sections must be of Bianchi class A. Motivated by general results on the symmetry reduction of variational principles, we show how to extend the Ashtekar–Samuel results to the setting of weakly locally homogeneous spaces as defined, e.g., by Singer and Thurston. In particular, it is shown that any m-dimensional homogeneous space G/K admitting a G-invariant volume form will allow a compact discrete quotient only if the Lie algebra cohomology of G relative to K is non-vanishing at degree m.


PACS

98.80.-k Cosmology

04.60.Kz Lower dimensional models; minisuperspace models

02.20.Sv Lie algebras of Lie groups

04.20.Gz Spacetime topology, causal structure, spinor structure

MSC

22E60 Lie algebras of Lie groups (For the algebraic theory of Lie algebras, see 17Bxx)

17B56 Cohomology of Lie (super)algebras

57T15 Homology and cohomology of homogeneous spaces of Lie groups

83F05 Cosmology

Subjects

Mathematical physics

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 11 (7 June 2004)

Received 23 February 2004

Published 24 April 2004



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