CURVATURE QUINTESSENCE MATCHED WITH OBSERVATIONAL DATA
By Salvatore Capozziello, Vincenzo F. Cardone, Sante Carloni, Antonio Troisi. 2003
457 citations recorded by the source corpus.
Quintessence issues can be achieved by taking into account higher order curvature invariants into the effective action of gravitational field. Such an approach is naturally related to fundamental theories of quantum gravity which predict higher order terms in loop expansion of quantum fields in curved space-times. In this framework, we obtain a class of cosmological solutions which are fitted against cosmological data. We reproduce encouraging results able to fit high redshift supernovae and WMAP observations. The age of the universe and other cosmological parameters are discussed in this context.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/092ba86d8b61df16f8dae83a821dadeab7b536f7
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In Astronomy and Astrophysics
- Salvatore Capozziello
- M. De Laurentis
- S. Tsujikawa
- Emmanuel N. Saridakis
- Antonio de Felice
- Valerio Faraoni
- Rafael C. Nunes
- Sergei D. Odintsov
In Nuclear and High Energy Physics
- Salvatore Capozziello
- S. Tsujikawa
- Antonio de Felice
- M. De Laurentis
- Emmanuel N. Saridakis
- Valerio Faraoni
- Rafael C. Nunes
- Sergei D. Odintsov
Citations in the corpus
- A Bird's Eye View of f (R)-Gravity (2009, methodology): “Combinations of non-minimally oupled and higher order terms an emergeas ontributions to e e tive Lagrangians; then we have higher order-s alar-tensor theories of gravity.From the mathemati al point of view, the problem of redu ing generalized theories to an Einstein-like form has beenextensively dis”
- Low surface brightness galaxy rotation curves in the low energy limit of Rn gravity: no need for dark matter? (2006, methodology): “…that the choice (3), with n 6= 1 and standard matter, is able to properly fit the Hubble diagram of Type Ia Supernovae without the need of dark energy (Capozziello et al. 2003; Carloni et al. 2005) and could also be reconciled with the constraints on the PPN parameters (Capozziello & Troisi 2005).”