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'''Semiclassical gravity''' is the approximation to theory of ] in which one treats ]s as being quantum and the ] as being classical. | '''Semiclassical gravity''' is the approximation to the theory of ] in which one treats ]s as being quantum and the ] as being classical. | ||
In semiclassical gravity, matter is represented by quantum matter fields that propagate according to the theory of ]. The spacetime in which |
In semiclassical gravity, matter is represented by quantum matter fields that propagate according to the theory of ]. The spacetime in which the fields propagate is classical but dynamical. The curvature of the spacetime is given by the ''semiclassical Einstein equations'', which relate the curvature of the spacetime, given by the ] <math>G_{\mu\nu}</math>, to the expectation value of the ] operator, <math>T_{\mu\nu}</math>, of the matter fields: | ||
:<math> G_{\mu\nu} = 8 \pi G \left\langle \hat T_{\mu\nu} \right\rangle_\psi </math> | :<math> G_{\mu\nu} = 8 \pi G \left\langle \hat T_{\mu\nu} \right\rangle_\psi </math> | ||
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where ''G'' is ] and <math>\psi</math> indicates the quantum state of the matter fields. | where ''G'' is ] and <math>\psi</math> indicates the quantum state of the matter fields. | ||
Since the theory of quantum gravity is yet |
Since the theory of quantum gravity is not yet known, it is difficult to say what is the regime of validity of semiclassical gravity. However, one can formally show that semiclassical gravity could be deduced from quantum gravity by considering ''N'' copies of the quantum matter fields, and taking the limit of ''N'' going to infinity while keeping the product ''GN'' constant. At diagrammatic level, semiclassical gravity corresponds to summing all ]s which do not have loops of gravitons (but have an arbitrary number of matter loops). Semiclassical gravity can also be deduced from an axiomatic approach. | ||
''''. | ''''. |
Revision as of 11:06, 10 December 2004
Semiclassical gravity is the approximation to the theory of quantum gravity in which one treats matter fields as being quantum and the gravitational field as being classical.
In semiclassical gravity, matter is represented by quantum matter fields that propagate according to the theory of quantum fields in curved spacetime. The spacetime in which the fields propagate is classical but dynamical. The curvature of the spacetime is given by the semiclassical Einstein equations, which relate the curvature of the spacetime, given by the Einstein tensor , to the expectation value of the energy-momentum tensor operator, , of the matter fields:
where G is Newton's constant and indicates the quantum state of the matter fields.
Since the theory of quantum gravity is not yet known, it is difficult to say what is the regime of validity of semiclassical gravity. However, one can formally show that semiclassical gravity could be deduced from quantum gravity by considering N copies of the quantum matter fields, and taking the limit of N going to infinity while keeping the product GN constant. At diagrammatic level, semiclassical gravity corresponds to summing all Feynman diagrams which do not have loops of gravitons (but have an arbitrary number of matter loops). Semiclassical gravity can also be deduced from an axiomatic approach.
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