Stability analysis of the Lorentz Chern-Simons expanding solutions

Chiaming Chang*, W. F. Kao, Ing Chen Lin

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    11 Scopus citations


    A class of Bianchi type II expanding solutions in a Lorentz Chern-Simons theory has been known to break the cosmic no-hair theorem. These solutions do not approach the late-time de Sitter Universe. We will show that there are two independent solutions classified by the parameter p for each given cosmological constant Λ. One of them is in the small-p phase; the other solution is in the large-p phase. It can be shown that an unstable mode always exists for the solution in its small-p phase that comes with smaller energy T00 and T00+T/2. The result indicates that the large-p phase is unlikely to be stable from an observation of a modified version of Wald's theorem.

    Original languageEnglish
    Article number063014
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Issue number6
    StatePublished - 26 Sep 2011


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