MODIFIED CHAPLYGIN TRAVERSABLE WORMHOLES
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Publication:3636392
DOI10.1142/S0218271809014480zbMath1181.83041arXiv0707.1183OpenAlexW2042446901MaRDI QIDQ3636392
Subenoy Chakraborty, Tanwi Bandyopadhyay
Publication date: 30 June 2009
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0707.1183
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (10)
Lorentzian wormholes in an emergent universe ⋮ Lorentzian wormholes supported by tachyon matter ⋮ Traversable wormhole on the brane with non-exotic matter: a broader view ⋮ Intra-galactic thin shell wormhole and its stability ⋮ Traversable Lorentzian wormhole on the Shtanov-Sahni braneworld with matter obeying the energy conditions ⋮ Shadow images of Kerr-like wormholes ⋮ Phase space of static wormholes sustained by an isotropic perfect fluid ⋮ Traversable wormholes and energy conditions with two different shape functions in f(R) gravity ⋮ Revisiting the evolving Lorentzian wormhole: a general perspective ⋮ Stability of a charged rotating BTZ thin shell with a different variable equation of state
Cites Work
- On the thermodynamic stability of the modified Chaplygin gas
- Generalized Chaplygin gas model: dark energy -- dark matter unification and CMBR con\-straints
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Cosmological constant -- the weight of the vacuum
- Energy conditions, traversable wormholes and dust shells
- Traversable Wormholes with Arbitrarily Small Energy Condition Violations
- The cosmological constant and dark energy
- Self-sustained phantom wormholes in semi-classical gravity
- Null Energy Condition in Dynamic Wormholes
- Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
- Role of modified Chaplygin gas in accelerated universe
- Surface stresses on a thin shell surrounding a traversable wormhole
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Stability analysis of dynamic thin shells
- An alternative to quintessence
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