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Stability of thin shell wormholes with a modified Chaplygin gas in Einstein–Hoffman–Born–Infeld theory

Abstract

In the framework of Darmois–Israel formalism, the dynamics of motion equations of spherically symmetric thin shell wormholes that are supported by a modified Chaplygin gas in Einstein–Hoffman–Born–Infeld theory are constructed. The stability analysis of a thin shell wormhole is also discussed using a linearized radial perturbation around static solutions at the wormhole throat. The existence of stable static solutions depends on the value of some parameters of dynamical shell.

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Correspondence to A. Eid.

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Eid, A. Stability of thin shell wormholes with a modified Chaplygin gas in Einstein–Hoffman–Born–Infeld theory. Indian J Phys 91, 1451–1456 (2017). https://doi.org/10.1007/s12648-017-1030-2

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  • DOI: https://doi.org/10.1007/s12648-017-1030-2

Keywords

  • General relativity
  • Wormholes
  • Modified Chaplygin gas
  • EHBI theory

PACS No.

  • 04.20.Dw
  • 95.30.Sf
  • 98.80.-k
  • 04.50.Kd