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(N+1)-dimensional Lorentzian evolving wormholes supported by polytropic matter

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Abstract

In this paper we study (N+1)-dimensional evolving wormholes supported by energy satisfying a polytropic equation of state. The considered evolving wormhole models are described by a constant redshift function and generalizes the standard flat Friedmann–Robertson–Walker spacetime. The polytropic equation of state allows us to consider in (3+1)-dimensions generalizations of the phantom energy and the generalized Chaplygin gas sources.

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Acknowledgements

This work was partially supported by CONICYT through Grant FONDECYT No. 1080530 and by the Dirección de Investigación de la Universidad del Bio-Bío through grants No. DIUBB 121007 2/R and No. GI121407/VBC (MC).

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Authors and Affiliations

  1. Departamento de Física, Facultad de Ciencias, Universidad del Bío-Bío, Avenida Collao 1202, Casilla 5-C, Concepción, Chile

    Mauricio Cataldo

  2. Departamento de Física, Universidad de Concepción, Casilla 160-C, Concepción, Chile

    Fernanda Aróstica & Sebastian Bahamonde

Authors
  1. Mauricio Cataldo
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  2. Fernanda Aróstica
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  3. Sebastian Bahamonde
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Correspondence to Mauricio Cataldo.

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Cataldo, M., Aróstica, F. & Bahamonde, S. (N+1)-dimensional Lorentzian evolving wormholes supported by polytropic matter. Eur. Phys. J. C 73, 2517 (2013). https://doi.org/10.1140/epjc/s10052-013-2517-4

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  • DOI: https://doi.org/10.1140/epjc/s10052-013-2517-4

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