Complete model of cosmological evolution of a classical scalar field with the Higgs potential. I. Analysis of the model
Yu. G. Ignat'ev, A. R. Samigullina

TL;DR
This paper develops and analyzes a comprehensive cosmological model involving a classical scalar field with the Higgs potential, exploring its dynamics without assuming a nonnegative Hubble constant, and classifies the topology of the associated Einstein-Higgs hypersurfaces.
Contribution
It provides a complete analysis and simulation of the cosmological evolution of a scalar field with Higgs potential, including a classification of the global phase space topology.
Findings
Classified the topology of Einstein-Higgs hypersurfaces.
Performed computer simulations without assuming nonnegative Hubble constant.
Analyzed the global properties of phase trajectories in the model.
Abstract
A complete model of cosmological evolution of a classical scalar field with the Higgs potential is studied and simulated on a computer without assumption that the Hubble constant is nonnegative. The corresponding dynamical system is qualitatively analyzed and the Einstein-Higgs hypersurfaces the topology of which determines the global properties of the phase trajectories of the cosmological model are classified.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsMaterial Science and Thermodynamics · advanced mathematical theories · Heat Transfer and Mathematical Modeling
