In f(R,T) gravity, a wormhole from one model can satisfy energy conditions, while another model requires exotic matter, and the Karmarkar condition does not remove that need.
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Evolution of Wormholes under f(R, T) Theory, the Karmarkar Condition and the Casimir Energy
In f(R,T) gravity, a wormhole from one model can satisfy energy conditions, while another model requires exotic matter, and the Karmarkar condition does not remove that need.