13.06.2015 Views

Kiefer C. Quantum gravity

Kiefer C. Quantum gravity

Kiefer C. Quantum gravity

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

112 HAMILTONIAN FORMULATION OF GENERAL RELATIVITY<br />

p N ≡ ∂Lg<br />

∂Ṅ =0,<br />

pg a ≡ ∂Lg =0. (4.62)<br />

∂Ṅ a<br />

Because lapse function and shift vector are only Lagrange multipliers (similar<br />

to A 0 in electrodynamics), these are constraints (called ‘primary constraints’<br />

according to Dirac (1964), since they do not involve the dynamical equations).<br />

Second,<br />

p ab ≡ ∂Lg<br />

∂ḣab<br />

= 1<br />

16πG Gabcd K cd =<br />

√<br />

h (<br />

K ab − Kh ab) . (4.63)<br />

16πG<br />

Note that the gravitational constant G appears here explicitly, although no coupling<br />

to matter is involved. This is the reason why it will appear in vacuum<br />

quantum <strong>gravity</strong>; see Section 5.2. One therefore has the Poisson-bracket relation<br />

13 {h ab (x),p cd (y)} = δ(a c δd b) δ(x, y) . (4.64)<br />

Recalling (4.48) and taking the trace of (4.63), one can express the velocities in<br />

terms of the momenta,<br />

ḣ ab = 32πGN √<br />

(p ab − 1 )<br />

h 2 ph ab + D a N b + D b N a , (4.65)<br />

where p ≡ p ab h ab . One can now calculate the canonical Hamiltonian density<br />

H g = p ab ḣ ab −L g ,<br />

for which one gets the expression 14<br />

√<br />

h(<br />

H g =16πGNG abcd p ab p cd (3) R − 2Λ)<br />

− N<br />

− 2N b (D a p ab ) . (4.66)<br />

16πG<br />

The full Hamiltonian is found by integration,<br />

∫<br />

∫<br />

H g ≡ d 3 x H g ≡ d 3 x (NH g ⊥ + N a Ha) g . (4.67)<br />

The action (4.61) can be written in the form<br />

∫ (<br />

)<br />

16πG S EH = dtd 3 x p ab ḣ ab − NH g ⊥ − N a Ha<br />

g . (4.68)<br />

Variation with respect to the Lagrange multipliers N and N a yields the constraints<br />

15<br />

13 This is formal at this stage since it does not take into account that √ h>0.<br />

14 This holds modulo a total divergence which does not contribute in the integral because Σ<br />

is compact.<br />

15 These also follow from the preservation of the primary constraints, {p N ,H g } = 0 =<br />

{p g a,H g }.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!