Living with Lambda
| dc.contributor.author | Sahni, Varun | |
| dc.date.accessioned | 2012-03-12T11:17:26Z | |
| dc.date.available | 2012-03-12T11:17:26Z | |
| dc.date.issued | 2000-10-24 | |
| dc.description.abstract | This talk presents a brief overview of recent results pertaining to the cosmological con- stant ‘ ’. I summarize the observational situation focussing on observations of high redshift Type Ia supernovae which suggest > 0. Observations of small angular anisotropies in the cosmic mi- crowave background complement Type Ia supernovae observations and both CMB and Sn can be combined to place strong constraints on the value of . The presence of a small -term increases the age of the universe and slows down the formation of large scale structure. I also review recent the- oretical attempts to generate a small -term at the current epoch and a model independent approach for determining the cosmic equation of state. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/1275 | |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | IUCAA Preprint;39/00 | |
| dc.subject | Cosmology | en_US |
| dc.subject | Supernovae | en_US |
| dc.subject | Cosmological constant | en_US |
| dc.subject | Vacuum fluctuations | en_US |
| dc.title | Living with Lambda | en_US |
| dc.type | Preprint | en_US |