dc.contributor.author |
de Sabbata, V |
|
dc.contributor.author |
Sivaram, C |
|
dc.date.accessioned |
2008-09-22T11:44:39Z |
|
dc.date.available |
2008-09-22T11:44:39Z |
|
dc.date.issued |
1990-03 |
|
dc.identifier.citation |
Astrophysics and Space Science, Vol. 165, No. 1, pp. 51 - 55 |
en |
dc.identifier.issn |
0004-640X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3759 |
|
dc.description.abstract |
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. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.uri |
http://www.springerlink.com/content/k5l845n17x765t36/ |
en |
dc.subject |
Computational Astrophysics |
en |
dc.subject |
Cosmology |
en |
dc.subject |
Plancks Constant |
en |
dc.subject |
Rotating Matter |
en |
dc.subject |
Torsion |
en |
dc.subject |
Universe |
en |
dc.subject |
Einstein Equations |
en |
dc.subject |
Gravitational Effects |
en |
dc.subject |
Relativity |
en |
dc.subject |
Spin Dynamics |
en |
dc.title |
Torsion and the cosmological constant problem |
en |
dc.type |
Article |
en |