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The document discusses the shape function of wormholes and the associated energy conditions in the context of general relativity and modified gravity theories. It presents two models: one for anisotropic wormholes and another for isotropic wormholes, detailing the mathematical expressions for matter density, pressure, and energy conditions. The findings indicate that the wormhole spacetimes are not asymptotically flat and explore the implications of energy constraints on the models presented.
- Author
- Piyali Bhar
- Language
- EN