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New spherically symmetric gravastar solutions, stable to radial perturbations, are found by utilising the construction of Visser and Wiltshire. The solutions possess an anti–de Sitter or de Sitter interior and a Schwarzschild–(anti)–de Sitter or Reissner–Nordstr"{o}m exterior. We find a wide range of parameters which allow stable gravastar solutions, and present the different qualitative behaviours of the equation of state for these parameters.

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