We compute the graviton one loop contribution to a classical energy in a traversable wormhole background. The form of the shape function considered is obtained by the equation of state p=ωρ. We investigate the size of the wormhole as a function of the parameter ω. 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 self-consistent source for the traversable wormhole.The case of the phantom region is briefly discussed
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
A possible candidate for the present accelerated expansion of the Universe is ''phantom energy'', wh...
We extend the notion of phantom energy, which is generally accepted for homogeneously distributed ma...
We compute the graviton one loop contribution to a classical energy in a traversable wormhole backgr...
We compute the graviton one-loop contribution to a classical energy in a traversable wormhole backgr...
We compute the graviton one loop contribution to a classical energy in a \textit{traversable} wormho...
We consider the effects of Gravity's Rainbow on the self-sustained equation which is responsible to ...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
It has been suggested that a possible candidate for the present accelerated expansion of the Univers...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
A possible candidate for the present accelerated expansion of the Universe is ''phantom energy'', wh...
We extend the notion of phantom energy, which is generally accepted for homogeneously distributed ma...
We compute the graviton one loop contribution to a classical energy in a traversable wormhole backgr...
We compute the graviton one-loop contribution to a classical energy in a traversable wormhole backgr...
We compute the graviton one loop contribution to a classical energy in a \textit{traversable} wormho...
We consider the effects of Gravity's Rainbow on the self-sustained equation which is responsible to ...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
It has been suggested that a possible candidate for the present accelerated expansion of the Univers...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
The ground state energy of the massive scalar field with nonconformal coupling ξ on a short-throat f...
Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive f...
A possible candidate for the present accelerated expansion of the Universe is ''phantom energy'', wh...
We extend the notion of phantom energy, which is generally accepted for homogeneously distributed ma...