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We compute the graviton one loop contribution to a classical energy in a wormhole background. The form of the shape function considered is obtained by the equation of state . We investigate the size of the wormhole as a function of the parameter . The investigation is evaluated by means of a variational approach with Gaussian trial wave functionals. A zeta function regularization is involved to handle with divergences. A renormalization procedure is introduced and the finite one loop energy is considered as a source for the traversable wormhole.The case of the phantom region is briefly discussed.

生成讲解博客的中文版本

生成AI智能校验的中文版本