Torsion and the cosmological constant problem

Details Torsion and the cosmological constant problem Torsion and the cosmological constant problem

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165...51d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 1, March 1990, p. 51-55.

Statistics

Computation

17

Computational Astrophysics, Cosmology, Plancks Constant, Rotating Matter, Torsion, Universe, Einstein Equations, Gravitational Effects, Relativity, Spin Dynamics

Scientific paper

A promising possibility which has yet to be considered with a view to furthering understanding of the cosmological constant problem is the use of torsion in a framework such as that of Einstein-Cartan theory: as would be natural in considering the gravitational contributions of particles with spin. It is presently shown that the recently suggested energy-dependent torsion-coupling constant can make the spin contributions of matter sources sufficiently large to cancel the cosmological constant term at all stages of the early universe, from the Plank epoch onward.

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