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Phantom field withO<mml:mn/>(N)<mml:mn/>symmetry in an exponential potential

2003/03/31 by Xin-Zhou Li, Xin-zhou Li, Jiangang Hao +1 · 101 citations
Mathematics · Physics and Astronomy · #Algorithm #Combinatorics #Cosmology and Gravitation Theories #Field (mathematics) #Geometry #Imaging phantom #Mathematics #Optics #Physics #Pure mathematics #Quantum Electrodynamics and Casimir Effect #Quantum chaos and dynamical systems #Symmetry (geometry) #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.69.107303

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 69(10) (American Physical Society) · 5 pages, 3 figures, replaced with the version to appear on Phys. Rev. D

arxiv created 2004/03/17 · openalex publication_date 2004/05/27 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

In this paper, we study the phase space of a phantom model with O(N) symmetry in an exponential potential. Different from the model without O(N) symmetry, the introduction of the symmetry leads to a lower bound w&gt;\ensuremath-3 on the equation of state for the existence of a stable phantom dominated attractor phase. The reconstruction relation between the potential of the O(N) phantom system and redshift has been derived.

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