pith. sign in

arxiv: 1610.00949 · v1 · pith:KJU6KTCDnew · submitted 2016-10-04 · 🌀 gr-qc

Scalar field with the source in the form of the stress-energy tensor trace as a dark energy model

classification 🌀 gr-qc
keywords scalarfieldparameterssourcestress-energytensortracechoice
0
0 comments X
read the original abstract

We consider a scalar-tensor theory of gravitation with the scalar source being the trace of the stress-energy tensor of the scalar field itself and matter. We obtain an example of a numerical solution of the cosmological equations which shows that under some special choice of the scalar parameters, there exists a slow-roll regime in which the modern values of the Hubble and deceleration parameters may be obtained.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Equatorial Periodic Orbits and Gravitational Wave Phenomenology around Spherically-symmetric vacuum solution in Freund-Nambu scalar-tensor gravity

    gr-qc 2026-06 unverdicted novelty 4.0

    Scalar couplings in Freund-Nambu gravity shift ISCO inward and produce detectable temporal dephasing in EMRI gravitational wave bursts while preserving orbit topology.