- #1
Sergei65
- 6
- 1
Momentum constraint in GR in ADM formalism is written in the form
$$\mathcal M_i=\gamma_{ij}D_k\pi^{kj},~~~~~~~~~~(1a)$$ or equivalently
$$\mathcal M_i=D_k\pi^{k}_i,~~~~~~~~~~(1b)$$ where
##\pi^{ij}=-\gamma^{1/2}\left(K^{ij}-\gamma^{ij}K\right)~##, ##K=\gamma^{ij}K_{ij}~##, ##\gamma=\det \gamma_{ij}~## and ##D_i~## is covariant derivative. This is from DeWitt1967 parer and original ADM parer.
However, those who deal with numerical relativity uses $$\mathcal
M_i=D_jK^j_i-D_iK.~~~~~~~~~~~~~~~(2)$$
What formula is right? (they coincides only if ##\gamma## does not depend on spatial coordinates, which is evidently not the case.
$$\mathcal M_i=\gamma_{ij}D_k\pi^{kj},~~~~~~~~~~(1a)$$ or equivalently
$$\mathcal M_i=D_k\pi^{k}_i,~~~~~~~~~~(1b)$$ where
##\pi^{ij}=-\gamma^{1/2}\left(K^{ij}-\gamma^{ij}K\right)~##, ##K=\gamma^{ij}K_{ij}~##, ##\gamma=\det \gamma_{ij}~## and ##D_i~## is covariant derivative. This is from DeWitt1967 parer and original ADM parer.
However, those who deal with numerical relativity uses $$\mathcal
M_i=D_jK^j_i-D_iK.~~~~~~~~~~~~~~~(2)$$
What formula is right? (they coincides only if ##\gamma## does not depend on spatial coordinates, which is evidently not the case.