Please use this identifier to cite or link to this item:
http://hdl.handle.net/11189/6441| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Carloni, S | en_US |
| dc.contributor.author | Dunsby, PKS | en_US |
| dc.contributor.author | Solomons, D | en_US |
| dc.date.accessioned | 2018-07-11T09:26:04Z | - |
| dc.date.available | 2018-07-11T09:26:04Z | - |
| dc.date.issued | 2006 | - |
| dc.identifier.citation | Carloni, S., Dunsby, P.K.S. and Solomons, D. 2006. Bounce conditions in f (R) cosmologies. Classical and Quantum Gravity, 23(6): 1913-1922 | en_US |
| dc.identifier.issn | 0264-9381 | - |
| dc.identifier.uri | https://doi.org/10.1088/0264-9381/23/6/006 | - |
| dc.identifier.uri | http://hdl.handle.net/11189/6441 | - |
| dc.description.abstract | We investigate the conditions for a bounce to occur in Friedmann–Robertson–Walker cosmologies for the class of fourth-order gravity theories. The general bounce criterion is determined and constraints on the parameters of three specific models are given in order to obtain bounce solutions. Furthermore, unlike the case of general relativity, a bounce appears to be possible in open and flat cosmologies. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | IOP Publishing | en_US |
| dc.relation.ispartof | Classical and Quantum Gravity | en_US |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/3.0/za/ | - |
| dc.subject | Friedmann–Robertson– Walker cosmologie | en_US |
| dc.subject | Fourth-order gravity theories | en_US |
| dc.subject | Bounce | en_US |
| dc.title | Bounce conditions in f (R) cosmologies. | en_US |
| dc.type.patent | Article | en_US |
| Appears in Collections: | Appsc - Journal Articles (DHET subsidised) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Bounce conditions in f(R) cosmologies.pdf | Main article | 159.35 kB | Adobe PDF | View/Open |
Page view(s)
80
Last Week
0
0
Last month
2
2
checked on Sep 4, 2026
Download(s)
32
checked on Sep 4, 2026
Google ScholarTM
Check
This item is licensed under a Creative Commons License