English

New Scalar Field Quartessence

General Relativity and Quantum Cosmology 2019-02-27 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We propose a cosmological scenario involving a scalar field, φ\varphi, that is a source of Dark Matter as well as of Dark Energy. Besides φ\varphi, the Lagrangian of the field theory envisaged in our scenario contains a second field χ\chi, for simplicity assumed to be a scalar, too. For fixed values of χ\chi, the potential term decays exponentially at large positive values of φ\varphi. While φ\varphi is not coupled to Standard Model fields, χ\chi is assumed to be coupled to them, and the Green functions of χ\chi depend on the cosmological redshift in the expanding universe. We assume that the term in the Lagrangian coupling χ\chi to φ\varphi is such that, at redshifts zz larger than some critical redshift zcz_c, φ\varphi is trapped near φ=0\varphi=0, and oscillations of φ\varphi about φ=0\varphi=0 describing massive scalar particles give rise to Dark Matter. At redshifts below zcz_c, the field φ\varphi is no longer trapped near the origin and starts to `roll' towards large field values. A homogenous component of φ\varphi emerges that acts as Dark Energy. Within over-dense regions, such as galaxies and galaxy clusters, the redshifting of χ\chi stops, and φ\varphi therefore remains trapped near φ=0\varphi=0 as long as zcz_c is smaller than the redshift when structures on galactic scales decouple from the Hubble flow. Thus, at the present time, φ\varphi describes both Dark Energy and Dark Matter.

Keywords

Cite

@article{arxiv.1809.07409,
  title  = {New Scalar Field Quartessence},
  author = {Robert Brandenberger and Rodrigo R. Cuzinatto and Jürg Fröhlich and Ryo Namba},
  journal= {arXiv preprint arXiv:1809.07409},
  year   = {2019}
}

Comments

6 pages

R2 v1 2026-06-23T04:12:09.826Z