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Future Stability of the FLRW Fluid Solutions in the Presence of a Positive Cosmological Constant

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Abstract

We introduce a new method for establishing the future non-linear stability of perturbations of FLRW solutions to the Einstein–Euler equations with a positive cosmological constant and a linear equation of state of the form p = . The method is based on a conformal transformation of the Einstein–Euler equations that compactifies the time domain and can handle the equation of state parameter values 0 < K ≤ 1/3 in a uniform manner. It also determines the asymptotic behavior of the perturbed solutions in the far future.

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Correspondence to Todd A. Oliynyk.

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Communicated by P. T. Chruściel

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Oliynyk, T.A. Future Stability of the FLRW Fluid Solutions in the Presence of a Positive Cosmological Constant. Commun. Math. Phys. 346, 293–312 (2016). https://doi.org/10.1007/s00220-015-2551-1

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  • DOI: https://doi.org/10.1007/s00220-015-2551-1

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