Abstract
The concepts of irreducible mass and of reversible and irreversible transformations in black holes are introduced, leading to the formula ${E}^{2}=m_{\mathrm{ir}}^{2}+(\frac{{L}^{2}}{4m_{\mathrm{ir}}^{2}})+{p}^{2}$ for a black hole of linear momentum $p$ and angular momentum $L$.
Keywords
Affiliated Institutions
Related Publications
Reversible Transformations of a Charged Black Hole
A formula is derived for the mass of a black hole as a function of its "irreducible mass," its angular momentum, and its charge. It is shown that 50% of the mass of an extreme c...
Extraction of Energy and Charge from a Black Hole
Misner has shown that in the scattering of massless wave fields by a Kerr black hole, certain modes are amplified at the expense of the rotational energy of the hole. We show he...
Pulses of Gravitational Radiation of a Particle Falling Radially into a Schwarzschild Black Hole
Using the Regge-Wheeler-Zerilli formalism of fully relativistic linear perturbations in the Schwarzschild metric, we analyze the radiation of a particle of mass $m$ falling into...
The Large Scale Structure of Space-Time
Einstein's General Theory of Relativity leads to two remarkable predictions: first, that the ultimate destiny of many massive stars is to undergo gravitational collapse and to d...
First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
Abstract We present measurements of the properties of the central radio source in M87 using Event Horizon Telescope data obtained during the 2017 campaign. We develop and fit ge...
Publication Info
- Year
- 1970
- Type
- article
- Volume
- 25
- Issue
- 22
- Pages
- 1596-1597
- Citations
- 665
- Access
- Closed
External Links
Social Impact
Social media, news, blog, policy document mentions
Citation Metrics
Cite This
Identifiers
- DOI
- 10.1103/physrevlett.25.1596