| dc.contributor.author | Rauscher, T. | |
| dc.date.accessioned | 2013-06-20T11:15:47Z | |
| dc.date.available | 2013-06-20T11:15:47Z | |
| dc.date.issued | 2007-03 | |
| dc.identifier.citation | Rauscher , T 2007 , ' Comment on "Heavy element production in inhomogeneous big bang nucleosynthesis" ' , Physical Review D - Particles, Fields, Gravitation and Cosmology , vol. 75 , no. 6 , 068301 . https://doi.org/10.1103/PhysRevD.75.068301 | |
| dc.identifier.issn | 1550-7998 | |
| dc.identifier.other | PURE: 1624312 | |
| dc.identifier.other | PURE UUID: 3eede6f1-0d8a-44dc-87ea-9b71588804ce | |
| dc.identifier.other | WOS: 000245333600110 | |
| dc.identifier.other | Scopus: 33947372582 | |
| dc.identifier.uri | http://hdl.handle.net/2299/10896 | |
| dc.description.abstract | The work of Matsuura et al. [Phys. Rev. D 72, 123505 (2005)] claims that heavy nuclei could have been produced in a combined p- and r-process in very high baryon density regions of an inhomogeneous big bang. However, they do not account for observational constraints and previous studies which show that such high baryon density regions did not significantly contribute to big bang abundances. | en |
| dc.format.extent | 2 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Physical Review D - Particles, Fields, Gravitation and Cosmology | |
| dc.subject | UNIVERSE | |
| dc.title | Comment on "Heavy element production in inhomogeneous big bang nucleosynthesis" | en |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | https://doi.org/10.1103/PhysRevD.75.068301 | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
