Room 515, Cosmology Building, NTU
(臺灣大學次震宇宙館 515研討室)
Static Manifolds and Quasi-local Mass in General Relativity
Brian Harvie (NCTS)
Abstract
Static manifolds are Riemannian manifolds of vanishing scalar curvature which give rise to equilibrium solutions of the Einstein equations in general relativity. In addition to playing a central role in the initial value problem of relativity, these manifolds are also important in definitions of mass in GR. While the Arnowitt-Deser-Misner (ADM) mass provides a suitable notion of total mass of an asymptotically flat, time-symmetric initial data set, defining the mass of a bounded open region in this data set is far more elusive.
Originally proposed by Robert Bartnik in 1986, the Bartnik mass is perhaps the most natural definition of quasi-local mass in GR. Given a compact Riemannian manifold with a spherical boundary component , the Bartnik mass of is conjectured to equal the ADM mass of an asymptotically flat static manifold which induces the same metric and mean curvature over as . This presents a challenge to differential geometers: show that a unique static extension always exists for any choice of positively-curved boundary metric and positive mean curvature function in order to verify the validity of the Bartnik mass.
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