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| HAL : hal-00007531, version 2 |
| arXiv : gr-qc/0507065 |
| Fiche détaillée |  Récupérer au format |
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| Versions disponibles : | v1 (15-07-2005) | v2 (15-08-2005) |
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| Negative Energies and a Constantly Accelerating Flat Universe |
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| Frederic Henry-Couannier1André Tilquin1Anne Ealet1Charling Tao1 |
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| (14/07/2005) |
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| It has been shown that in the context of General Relativity (GR) enriched with a new set of discrete symmetry reversal conjugate metrics, negative energy states can be rehabilitated while avoiding the well-known instability issues. We review here some cosmological implications of the model and confront them with the supernovae and CMB data. The predicted flat universe constantly accelerated expansion phase is found to be in rather good agreement with the most recent cosmological data. |
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| 1 : | CPPM - Centre de Physique des Particules de Marseille |
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| Domaine | : | Physique/Relativité Générale et Cosmologie Quantique Physique/Astrophysique/Cosmologie et astrophysique extra-galactique |
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| negative energy – pioneer effect |
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| Liste des fichiers attachés à ce document : | ||||||||||
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| hal-00007531, version 2 | |
| http://hal.archives-ouvertes.fr/hal-00007531 | |
| oai:hal.archives-ouvertes.fr:hal-00007531 | |
| Contributeur : Frederic Henry-Couannier | |
| Soumis le : Lundi 15 Août 2005, 14:06:56 | |
| Dernière modification le : Lundi 15 Août 2005, 17:48:52 | |
