Buchdahl compactness limit and gravitational field energy
Naresh Dadhich
Abstract
The main aim of this paper is essentially to point out that the Buchdahl compactness limit of a static object is given by \it{gravitational field energy being less than or equal to half of its non-gravitational matter energy}. It is thus entirely determined without any reference to interior distribution by the exterior unique solutions, the Schwarzschild for neutral and the Reissner-Nordstr{$\ddot o$}m for charged object. In terms of surface potential, it reads as $\Phi(R) = (M-Q^2/2R)/R \leq 4/9$ which translates to surface red-shift being less than or equal to $3$. It also prescribes an upper bound on charge an object could have, $Q^2/M^2 \leq 9/8 > 1$.
Topics & Concepts
PhysicsCompact spaceLimit (mathematics)Schwarzschild radiusGravitational fieldGravitationUpper and lower boundsField (mathematics)Surface (topology)Classical mechanicsDistribution (mathematics)Charge (physics)Point particleGeneral relativityPoint (geometry)Object (grammar)Gravitational energyEnergy (signal processing)Schwarzschild metricType (biology)Mathematical physicsWork (physics)Theoretical physicsCompact starCosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsHigh-Energy Particle Collisions Research