Why do we observe a small but nonzero cosmological constant?
| dc.contributor.author | Padmanabhan, T. | |
| dc.date.accessioned | 2012-03-03T15:02:30Z | |
| dc.date.available | 2012-03-03T15:02:30Z | |
| dc.date.issued | 2002-08-16 | |
| dc.identifier.uri | http://hdl.handle.net/11007/204 | |
| dc.language.iso | en | en_US |
| dc.publisher | IOP Publishing | en_US |
| dc.relation.ispartofseries | Classical and Quantum Gravity;Vol. 19, 2002 | |
| dc.subject | Cosmology | en_US |
| dc.subject | Nonzero | en_US |
| dc.title | Why do we observe a small but nonzero cosmological constant? | en_US |
| dc.type | Article | en_US |