Published October 2008 | Version v1
Journal article

Enlarging minimal-supergravity parameter space by decreasing pre-nucleosynthesis Hubble rate in scalar-tensor cosmologies

  • 1. Scuola Internazionale Superiore di Studi Avanzati, Via Beirut 2-4, I-34014 Trieste (Italy)
  • 2. Dipartimento di Fisica Teorica, Universita di Torino, via P. Giuria 1, I-10125 Torino (Italy)
  • 3. Dipartimento di Fisica, Universita di Padova, via Marzolo 8, I-35131, Padova (Italy)
  • 4. Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, I-35131, Padova (Italy)
  • 5. Istituto Nazionale di Fisica Nucleare, Sezione di Torino, via P. Giuria 1, I-10125 Torino (Italy)

Description

We determine under what conditions Scalar Tensor cosmologies predict an expansion rate which is reduced as compared to the standard General Relativity case. We show that ST theories with a single matter sector typically predict an enhanced Hubble rate in the past, as a consequence of the requirement of an attractive fixed point towards General Relativity at late times. Instead, when additional matter sectors with different conformal factors are added, the late time convergence to General Relativity is maintained and at the same time a reduced expansion rate in the past can be driven. For suitable choices of the parameters which govern the scalar field evolution, a sizeable reduction of the Hubble rate prior to Big Bang Nucleosynthesis can be obtained. We then discuss the impact of these cosmological models on the relic abundance of dark matter in minimal Supergravity models: we show that the cosmologically allowed regions in parameter space are significantly enlarged in this class of ST theories with reduced Hubble rate. The ensuing effect on the potential reach of LHC are briefly discussed.

Availability note (English)

Available from http://dx.doi.org/10.1088/1126-6708/2008/10/003

Additional details

Publishing Information

Journal Title
Journal of High Energy Physics
Journal Volume
10
Journal Issue
2008
Journal Page Range
p. 003
ISSN
1126-6708