https://doi.org/10.1140/epjc/s10052-016-4470-5
Regular Article - Theoretical Physics
Observational constraints on cosmological future singularities
1
Aix Marseille Univ, Université de Toulon CNRS, CPT, Marseille, France
2
Fisika Teorikoaren eta Zientziaren Historia Saila, Zientzia eta Teknologia Fakultatea, Euskal Herriko Unibertsitatea, 644 Posta Kutxatila, 48080, Bilbao, Spain
3
Departamento de Física, Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências da Universidade de Lisboa, Edifício C8, Campo Grande, P-1749-016, Lisbon, Portugal
4
Institute of Physics, University of Szczecin, Wielkopolska 15, 70-451, Szczecin, Poland
* e-mail: jose.beltran@cpt.univ-mrs.fr
Received:
2
June
2016
Accepted:
1
November
2016
Published online:
19
November
2016
In this work we consider a family of cosmological models featuring future singularities. This type of cosmological evolution is typical of dark energy models with an equation of state violating some of the standard energy conditions (e.g. the null energy condition). Such a kind of behavior, widely studied in the literature, may arise in cosmologies with phantom fields, theories of modified gravity or models with interacting dark matter/dark energy. We briefly review the physical consequences of these cosmological evolution regarding geodesic completeness and the divergence of tidal forces in order to emphasize under which circumstances the singularities in some cosmological quantities correspond to actual singular spacetimes. We then introduce several phenomenological parameterizations of the Hubble expansion rate to model different singularities existing in the literature and use SN Ia, BAO and H(z) data to constrain how far in the future the singularity needs to be (under some reasonable assumptions on the behavior of the Hubble factor). We show that, for our family of parameterizations, the lower bound for the singularity time cannot be smaller than about 1.2 times the age of the universe, what roughly speaking means Gyrs from the present time.
© The Author(s), 2016