期刊
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
卷 -, 期 9, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/1475-7516/2015/09/041
关键词
modified gravity; cosmological perturbation theory; dark energy theory
资金
- UPV/EHU
- Basque government (Spain) [IT592-13]
- Portuguese Agency Fundacao para a Ciencia e Tecnologia through an Investigador FCT Research contract [IF/01442/2013/CP1196/CT0001]
- Istituto Nazionale di Fisica Nucleare, (iniziativa specifica QGSKY)
- [PTDC/FIS/111032/2009]
- [UID/MAT/00212/2013]
- Fundação para a Ciência e a Tecnologia [IF/01442/2013/CP1196/CT0001] Funding Source: FCT
We discuss the possibility that suitable modifications of gravity could account for some amount of the radiation we observe today, in addition to the possibility of explaining the present speed up of the universe. We start introducing and reviewing cosmological reconstruction methods for metric f(R) theories of gravity that can be considered as one of the straightforward modifications of Einstein's gravity as soon as f(R) not equal R. We then take into account two possible f(R) models which could give rise to (dark) radiation. Constraints on the models are found by using the Planck Collaboration 2015 data within a cosmographic approach and by obtaining the matter power spectrum of those models. The conclusion is that f(R) gravity can only contribute minimally to the (dark) radiation to avoid departures from the observed matter power spectrum at the smallest scales (of the order of 0.01 Mpc(-1)), i.e., precisely those scales that exited the horizon at the radiation dominated epoch. This result could strongly contribute to select reliable f(R) models.
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