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Canonical quantum gravity : ウィキペディア英語版
Canonical quantum gravity

In physics, canonical quantum gravity is an attempt to quantize the canonical formulation of general relativity (or canonical gravity). It is a Hamiltonian formulation of Einstein's general theory of relativity. The basic theory was outlined by Bryce DeWitt in a seminal 1967 paper, and based on earlier work by Peter G. Bergmann using the so-called canonical quantization techniques for constrained Hamiltonian systems invented by Paul Dirac. Dirac's approach allows the quantization of systems that include gauge symmetries using Hamiltonian techniques in a fixed gauge choice. Newer approaches based in part on the work of DeWitt and Dirac include the Hartle–Hawking state, Regge calculus, the Wheeler–DeWitt equation and loop quantum gravity.
== Canonical quantization ==

In the Hamiltonian formulation of ordinary classical mechanics the Poisson bracket is an important concept. A "canonical coordinate system" consists of canonical position and momentum variables that satisfy canonical Poisson-bracket relations,
\ = \delta_
where the Poisson bracket is given by
:\ = \sum_^ \left(
\frac_i = \,
\dot_i = \.
These equations describe a ``flow" or orbit in phase space generated by the Hamiltonian H. Given any phase space function F (q,p), we have
F (q_i,p_i) = \.
In canonical quantization the phase space variables are promoted to quantum operators on a Hilbert space and the Poisson bracket between phase space variables is replaced by the canonical commutation relation:
(, \hat ) = i \hbar.
In the so-called position representation this commutation relation is realized by the choice:
\hat \psi (q) = q \psi (q) and \hat \psi (q) = -i \hbar \psi (q)
The dynamics are described by Schrödinger equation:
i \hbar \psi = \hat \psi
where \hat is the operator formed from the Hamiltonian H (q,p) with the replacement q \mapsto q and p \mapsto -i \hbar .

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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