Applies the f(R) = R - μ Rc (R/Rc)^p model and shape function b(r) = r log(r+1)/log(r0+1) to Morris-Thorne wormholes and analyzes energy conditions for non-exotic matter support.
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gr-qc 2years
2019 2verdicts
UNVERDICTED 2representative citing papers
Wormholes with b(r) = r0 tanh(r)/tanh(r0) in f(R) = R + α R^m - β R^{-n} gravity have energy conditions, EOS parameter, and anisotropy computed across parameter cases.
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Wormhole Modeling Supported by Non-Exotic Matter
Applies the f(R) = R - μ Rc (R/Rc)^p model and shape function b(r) = r log(r+1)/log(r0+1) to Morris-Thorne wormholes and analyzes energy conditions for non-exotic matter support.
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Non violation of energy conditions in wormholes modelling
Wormholes with b(r) = r0 tanh(r)/tanh(r0) in f(R) = R + α R^m - β R^{-n} gravity have energy conditions, EOS parameter, and anisotropy computed across parameter cases.