Please use this identifier to cite or link to this item:
https://olympias.lib.uoi.gr/jspui/handle/123456789/16198Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Nesseris, S. | en |
| dc.contributor.author | Perivolaropoulos, L. | en |
| dc.date.accessioned | 2015-11-24T18:28:53Z | - |
| dc.date.available | 2015-11-24T18:28:53Z | - |
| dc.identifier.issn | 1550-7998 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16198 | - |
| dc.rights | Default Licence | - |
| dc.subject | high-redshift supernovae | en |
| dc.subject | equation-of-state | en |
| dc.subject | hubble-space-telescope | en |
| dc.subject | dark energy density | en |
| dc.subject | cosmological constant | en |
| dc.subject | accelerating universe | en |
| dc.subject | constraints | en |
| dc.subject | models | en |
| dc.subject | quintom | en |
| dc.subject | omega(lambda) | en |
| dc.title | Evolving Newton's constant, extended gravity theories, and SnIa data analysis | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.primary | Doi 10.1103/Physrevd.73.103511 | - |
| heal.identifier.secondary | <Go to ISI>://000237951100021 | - |
| heal.identifier.secondary | http://prd.aps.org/abstract/PRD/v73/i10/e103511 | - |
| heal.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 2006 | - |
| heal.abstract | If Newton's constant G evolves on cosmological timescales as predicted by extended gravity theories then Type Ia supernovae (SnIa) cannot be treated as standard candles. The magnitude-redshift datasets however can still be useful. They can be used to simultaneously fit for both H(z) and G(z) (so that local G(z) constraints are also satisfied) in the context of appropriate parametrizations. Here we demonstrate how this analysis can be done by applying it to the Gold SnIa dataset. We compare the derived effective equation of state parameter w(z) at best fit with the corresponding result obtained by neglecting the evolution G(z). We show that even though the results clearly differ from each other, in both cases the best fit w(z) crosses the phantom divide w=-1. We then attempt to reconstruct a scalar-tensor theory that predicts the derived best fit forms of H(z) and G(z). Since the best fit G(z) fixes the scalar-tensor potential evolution F(z), there is no ambiguity in the reconstruction and the potential U(z) can be derived uniquely. The particular reconstructed scalar-tensor theory, however, involves a change of sign of the kinetic term Phi'(z)(2) as in the minimally coupled case. | en |
| heal.journalName | Physical Review D | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| perivolaropoulos-2006-Evolving Newton's constant, extended gravity theories, and SnIa data analysis.pdf | 229.22 kB | Adobe PDF | View/Open |
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