Abstract
This work introduces a new gravitational redshift function to the Morris-Thorne wormhole model that is defined as Φ(r)≡r_0/r ln⁡(r/r_0 ) with spherical symmetry and stabilized by phantom energy.

Keywords
Wormhole, Morris-Thorne, redshift, ghost energy

Cite this paper
Raul Isea, A proposed new gravitational redshift function to the theoretical model of Morris-Thorne wormholes , SCIREA Journal of Astronomy. Volume 1, Issue 1, April 2017 | PP. 1-6.

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