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.
Visser, Lorentzian wormholes: from Einstein to Hawking, AIP Press, New York (1995)
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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.