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Complex field as inflaton and quintessence

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arxiv hep-th/0208129 v1 pith:H7EB5KOJ submitted 2002-08-19 hep-th

classification hep-th
keywords complexfieldacceleratedcosmologicalinflationquintessenceuniverseacceleration
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abstract

We investigate cosmology with complex scalar field. It is shown that such models can describe two stages of inflation and the oscillatory regime. Thus we don't need both quintessence and $\Lambda$-term. It is enough to have single complex field to obtain both inflation and present accelerated universe. If the present accelerated expansion was created by the complex field then universe must escape eternal acceleration. Besides, we will show that cosmological equations with complex field admit stationary solution without any cosmological constant.

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Cited by 1 Pith paper

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

  1. Complex Inflaton Potentials with Nonminimal Coupling: Robust Inflation and Geometric Reheating

    gr-qc 2026-02 reject novelty 5.0 of 10

    A complex-scalar inflation model with a non-Hermitian imaginary potential claims geometric reheating, but the reheating evidence is internally contradictory and the CMB predictions reduce to fitted α-attractor results.

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