dc.contributor.author |
Sivaram, C |
|
dc.contributor.author |
De Sabbata, V |
|
dc.date.accessioned |
2008-10-16T09:46:42Z |
|
dc.date.available |
2008-10-16T09:46:42Z |
|
dc.date.issued |
1991-02 |
|
dc.identifier.citation |
Astrophysics and Space Science, Vol. 176, No. 1, pp. 141 - 144 |
en |
dc.identifier.issn |
0004-640X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3948 |
|
dc.description.abstract |
The effects of torsion in the early universe on the subsequent evolution are investigated theoretically. The focus is on the simple Einstein-Cartan generalization of conventional big-bang cosmology studied by de Sabbata and Sivaram (1989), but here a massless scalar field with no quartic self-coupling is considered. As in the case with a massive field, a torsion-dominated phase in the early universe leads naturally to negative pressure and inflationary expansion. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.uri |
http://www.springerlink.com/content/t426x2766357l3pp/ |
en |
dc.subject |
Big Bang Cosmology |
en |
dc.subject |
Einstein Equations |
en |
dc.subject |
Space-Time Functions |
en |
dc.subject |
Scalars |
en |
dc.subject |
Spin-Spin Coupling |
en |
dc.subject |
Tensor Analysis |
en |
dc.subject |
Torsion |
en |
dc.title |
Torsion and inflation |
en |
dc.type |
Article |
en |