Frank Castle
- 579
- 23
Haelfix said:Hmm?
Vacuum energy is a well defined concept in GR. Consider for concreteness the theory of a single scalar field with potential V(phi). The action is given by
S= \int d^{4}x\sqrt{-g}\left ( \frac{1}{2}g^{uv}\partial _{u}\Phi \partial _{v}\Phi -V\left ( \Phi \right )\right )
The corresponding energy momentum tensor is computed as:
T_{uv}= \frac{1}{2}\partial _{u}\Phi \partial _{v}\Phi + \frac{1}{2}\left (g^{\alpha \beta }\partial _{\alpha }\Phi \partial _{\beta }\Phi \right ) g_{uv} - V\left(\Phi\right) g_{uv}
The lowest energy density configuration if it exists is obtained when both the kinetic and gradient terms vanishes, which gives us our definition for vacuum energy and implies for this particular theory that:
T_{uv}^{vac}\equiv -\rho _{vac} g_{uv} =-V\left(\Phi_{0}\right) g_{uv}
Where \Phi _{0} is the value that minimizes the potential. Note that this is not necessarily zero. More generally you can argue by lorentz invariance that the form for vacuum energy is unique and fixed exactly as above.
Note that since the equations are sourced directly by the energy momentum tensor, you cannot simply subtract away dangerous (potentially infinite) renormalizations unlike the case for non gravitational theories.
This is my understanding of things - at least for semi-classical applications of GR, in which the gravitational sector is classical GR and the matter sector is quantum.
