Boundary conditions for the Einstein-Christoffel formulation of Einstein's equations
Douglas N. Arnold, Nicolae Tarfulea
Abstract
Open-access reader
Douglas N. Arnold, Nicolae Tarfulea
Abstract
Open-access reader
Abstract. Specifying boundary conditions continues to be a challenge in numerical relativity in order to obtain a long time convergent numerical simulation of Einstein’s equations in domains with artificial boundaries. In this paper, we address this problem for the Einstein–Christoffel (EC) symmetric hyperbolic formulation of Einstein’s equations linearized around flat spacetime. First, we prescribe simple boundary conditions that make the problem well posed and preserve the constraints. Next, we indicate boundary conditions for a system that extends the linearized EC system by including the momentum constraints and whose solution solves Einstein’s equations in a bounded domain. 1.
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Abstract. Specifying boundary conditions continues to be a challenge in numerical relativity in order to obtain a long time convergent numerical simulation of Einstein’s equations in domains with artificial boundaries. In this paper, we address this problem for the Einstein–Christoffel (EC) symmetric hyperbolic formulation of Einstein’s equations linearized around flat spacetime. First, we prescribe simple boundary conditions that make the problem well posed and preserve the constraints. Next, we indicate boundary conditions for a system that extends the linearized EC system by including the momentum constraints and whose solution solves Einstein’s equations in a bounded domain. 1.
Key concepts: Christoffel symbols, Einstein, Einstein's constant, Mathematical physics, Boundary (topology), Einstein equations, Physics, Boundary value problem