Darmois matching and $C^3$ matching

Abstract

We apply the Darmois and the $C^3$ matching conditions to three different spherically symmetric spacetimes. The exterior spacetime is described by the Schwarzschild vacuum solution whereas for the interior counterpart we choose different perfect fluid solutions with the same symmetry. We show that Darmois matching conditions are satisfied in all three cases whereas the $C^3$ conditions are not fulfilled. We argue that this difference is due to a non-physical behavior of the pressure on the matching surface.

Replaced with the version matching the published one in CQG

References in corpus (3)

• Characterizing repulsive gravity with curvature eigenvalues
• Revisiting the Darmois and Lichnerowicz junction conditions
• Repulsive regions in Lemaître-Tolman-Bondi gravitational collapse

Cited by in corpus (1)

• Fermi-normal coordinates for the Newtonian approximation of gravity