We prove upper bounds on angular momentum and centre of mass in terms of the Hamiltonian mass and cosmological constant for non-singular asymptotically anti-de Sitter initial data sets satisfying the dominant energy condition. We work in all space-dimensions larger than or equal to three, and allow a large class of asymptotic backgrounds, with spherical and non-spherical conformal infinities; in the latter case, a spin-structure compatibility condition is imposed. We give a large class of non-trivial examples saturating the inequality. We analyse exhaustively the borderline case in space-time dimension four: for spherical cross-sections of Scri, equality together with completeness occurs only in anti-de Sitter space-time. On the other hand,...
We prove that for any vacuum, maximal, asymptotically flat, axisymmetric initial data for Einstein e...
The assumption of asymptotic flatness for isolated astrophysical bodies may be considered an approxi...
The assumption of asymptotic flatness for isolated astrophysical bodies may be considered an approxi...
We prove upper bounds on angular momentum and centre of mass in terms of the Hamiltonian mass and co...
We prove upper bounds on angular momentum and centre of mass in terms of the Hamiltonian mass and co...
International audienceWe present the key elements of the proof of an upper bound for angular-momentu...
We prove an inequality relating the trace of the extrinsic curvature, the total angular momentum, th...
WOS:000271759400013 (Nº de Acesso Web of Science)We present the key elements of the proof of an uppe...
We consider n-dimensional spacetimes which are axisymmetric—but not necessarily stationary—in the se...
The calculation of conserved charges of black holes is a rich problem, for which many methods are kn...
For a stable, marginally outer trapped surface (MOTS) in an axially symmetric spacetime with cosmolo...
We prove that extreme Kerr initial data set is a unique absolute minimum of the total mass in a (phy...
Contains fulltext : 195553.pdf (publisher's version ) (Open Access
In this talk we answer an interesting question about extension of Dain’s inequality to higher dimens...
For a stable, marginally outer trapped surface (MOTS) in an axially symmetric spacetime with cosmolo...
We prove that for any vacuum, maximal, asymptotically flat, axisymmetric initial data for Einstein e...
The assumption of asymptotic flatness for isolated astrophysical bodies may be considered an approxi...
The assumption of asymptotic flatness for isolated astrophysical bodies may be considered an approxi...
We prove upper bounds on angular momentum and centre of mass in terms of the Hamiltonian mass and co...
We prove upper bounds on angular momentum and centre of mass in terms of the Hamiltonian mass and co...
International audienceWe present the key elements of the proof of an upper bound for angular-momentu...
We prove an inequality relating the trace of the extrinsic curvature, the total angular momentum, th...
WOS:000271759400013 (Nº de Acesso Web of Science)We present the key elements of the proof of an uppe...
We consider n-dimensional spacetimes which are axisymmetric—but not necessarily stationary—in the se...
The calculation of conserved charges of black holes is a rich problem, for which many methods are kn...
For a stable, marginally outer trapped surface (MOTS) in an axially symmetric spacetime with cosmolo...
We prove that extreme Kerr initial data set is a unique absolute minimum of the total mass in a (phy...
Contains fulltext : 195553.pdf (publisher's version ) (Open Access
In this talk we answer an interesting question about extension of Dain’s inequality to higher dimens...
For a stable, marginally outer trapped surface (MOTS) in an axially symmetric spacetime with cosmolo...
We prove that for any vacuum, maximal, asymptotically flat, axisymmetric initial data for Einstein e...
The assumption of asymptotic flatness for isolated astrophysical bodies may be considered an approxi...
The assumption of asymptotic flatness for isolated astrophysical bodies may be considered an approxi...