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

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.

6 pages, 2 figures, accepted for publication in European Physical Journal C

References in corpus (9)

• Asymptotically (anti) de Sitter Black Holes and Wormholes with a Self Interacting Scalar Field in Four Dimensions
• Phantom stars and topology change
• Thin-shell wormholes with a generalized Chaplygin gas
• N-dimensional static and evolving Lorentzian wormholes with cosmological constant
• Evolving Lorentzian wormholes supported by phantom matter and cosmological constant
• Wormhole Solutions in Gauss-Bonnet-Born-Infeld Gravity
• The LambdaCDM model on the lead -- a Bayesian cosmological models comparison
• Two-fluid evolving Lorentzian wormholes
• Classical and quantum wormholes in a 5D compact Kaluza-Klein theory

Cited by in corpus (11)

• Generalized uncertainty principle corrections in Rastall-Rainbow Casimir wormholes
• Cosmological wormholes in $f(R)$ theories of gravity
• Dynamic wormhole solutions in Einstein-Cartan gravity
• Wormhole solutions with a polynomial equation-of-state and minimal violation of the null energy condition
• Dynamic wormhole geometries in hybrid metric-Palatini gravity
• Static phantom wormholes of finite size
• Evolving wormhole in the brane-world scenario
• Dynamical wormholes in Lovelock gravity
• Stability of a $d$-dimensional thin-shell wormhole surrounded by quintessence
• Evolving traversable wormholes satisfying the energy conditions in the presence of pole dark energy
• Evolving wormhole formation in dRGT massive gravity