Fully-constrained formulation of Einstein's field equations using ...
Fully-constrained formulation of Einstein's field equations using ...
Fully-constrained formulation of Einstein's field equations using ...
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Constrained<br />
<strong>formulation</strong> <strong>of</strong><br />
Einstein<br />
<strong>equations</strong><br />
Jérôme Novak<br />
Introduction<br />
Constraints<br />
Motivations<br />
Formulation<br />
Conformal<br />
decomposition<br />
Equations<br />
Strategy<br />
Simulations<br />
Gravitational<br />
Waves<br />
Neutron stars<br />
Summary<br />
Stationary axisymmetric models<br />
Deviation from conformal flatness<br />
For all components (except h rϕ and h θϕ ,<br />
which are null), h ij max ∼ 0.005 (up to ∼ 0.02<br />
in more compact cases)<br />
⇒comparable with γθθ − γϕϕ in<br />
quasi-isotropic gauge
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