4,745 research outputs found
Linear perturbations for the vacuum axisymmetric Einstein equations
In axial symmetry, there is a gauge for Einstein equations such that the
total mass of the spacetime can be written as a conserved, positive definite,
integral on the spacelike slices. This property is expected to play an
important role in the global evolution. In this gauge the equations reduce to a
coupled hyperbolic-elliptic system which is formally singular at the axis. Due
to the rather peculiar properties of the system, the local in time existence
has proved to resist analysis by standard methods. To analyze the principal
part of the equations, which may represent the main source of the difficulties,
we study linear perturbation around the flat Minkowski solution in this gauge.
In this article we solve this linearized system explicitly in terms of integral
transformations in a remarkable simple form. This representation is well suited
to obtain useful estimates to apply in the non-linear case.Comment: 13 pages. We suppressed the statements about decay at infinity. The
proofs of these statements were incomplete. The complete proofs will require
extensive technical analysis. We will studied this in a subsequent work. We
also have rewritten the introduction and slighted changed the titl
Angular momentum-mass inequality for axisymmetric black holes
In these notes we describe recent results concerning the inequality for axially symmetric black holes.Comment: 7 pages, 1 figur
The Yamabe invariant for axially symmetric two Kerr black holes initial data
An explicit 3-dimensional Riemannian metric is constructed which can be
interpreted as the (conformal) sum of two Kerr black holes with aligned angular
momentum. When the separation distance between them is large we prove that this
metric has positive Ricci scalar and hence positive Yamabe invariant. This
metric can be used to construct axially symmetric initial data for two Kerr
black holes with large angular momentum.Comment: 14 pages, 2 figure
Initial data for black hole collisions
I describe the construction of initial data for the Einstein vacuum equations
that can represent a collision of two black holes. I stress in the main
physical ideas.Comment: 5 pages, 2 figures. To appear in the Proceedings of the Spanish
Relativity Meeting Gravitation and Cosmology ERE - 2002; isbn: 978844752738
Proof of the (local) angular momemtum-mass inequality for axisymmetric black holes
We prove that for any vacuum, maximal, asymptotically flat, axisymmetric
initial data for Einstein equations close to extreme Kerr data, the inequality
is satisfied, where and are the total mass and
angular momentum of the data. The proof consists in showing that extreme Kerr
is a local minimum of the mass.Comment: 14 page
On black holes as inner boundaries for the constraint equations
General aspects of the boundary value problem for the constraint equations
and their application to black holes are discussed.Comment: 8 pages. Seventh Hungarian Relativity Workshop, Sarospatak, Hungary,
10-15 August, 2003. To appear in the proceedings; isbn: 978963058187
Generalized Korn's inequality and conformal Killing vectors
Korn's inequality plays an important role in linear elasticity theory. This
inequality bounds the norm of the derivatives of the displacement vector by the
norm of the linearized strain tensor. The kernel of the linearized strain
tensor are the infinitesimal rigid-body translations and rotations (Killing
vectors). We generalize this inequality by replacing the linearized strain
tensor by its trace free part. That is, we obtain a stronger inequality in
which the kernel of the relevant operator are the conformal Killing vectors.
The new inequality has applications in General Relativity.Comment: 8 page
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