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Phantom cosmology with general potentials

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arxiv gr-qc/0506095 v1 pith:S2BT5WSF submitted 2005-06-17 gr-qc astro-phhep-th

classification gr-qcastro-phhep-th
keywords phantomgeneralresultsassumptionsattractorscosmologyderiveddominated
verification ladder T0 review T1 audit T2 compute T3 formal
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We present a unified treatment of the phase space of a spatially flat homogeneous and isotropic universe dominated by a phantom field. Results on the dynamics and the late time attractors (Big Rip, de Sitter, etc.) are derived without specifying the form of the phantom potential, using only general assumptions on its shape. Many results found in the literature are quickly recovered and predictions are made for new scenarios.

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Forward citations

Cited by 3 Pith papers

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

  1. Anomalous Decay Rate and Greybody Factors for Regular Black Holes with Scalar Hair

    gr-qc 2026-02 unverdicted novelty 6.0 of 10

    Regular black holes with scalar hair exhibit anomalous decay rates for massive scalar perturbations, with longest-lived modes switching to lower angular momentum above a critical mass.

  2. Observational Tests of Regular Black Holes with Scalar Hair and their Stability

    gr-qc 2025-10 unverdicted novelty 5.0 of 10

    Regular black holes with phantom scalar hair are constrained by Solar System and EHT observations, with exact relations linking photon sphere Lyapunov exponent to shadow size and impact parameter.

  3. The old problem of the cosmological constant solved?

    gr-qc 2025-05 reject novelty 4.0 of 10

    A speculative essay claims that a model of gravity as superluminal phonons on a ring lattice solves the cosmological constant problem, but provides no derivation of the values or dynamics.

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