Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5130448 | Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics | 2016 | 4 Pages |
â¢Equilibrium in static spherical stars has been studied in the literature.â¢The relevant equation is referred to with two names, OV or TOV (more popular).â¢We compare Tolman׳s and Oppenheimer & Volkoff׳s papers.â¢We find that they adopt diametrically opposite approaches to the same problem.â¢The equation is a product of the OV approach, so should be called the OV equation.
The well-known equation for hydrostatic equilibrium in a static spherically symmetric spacetime supported by an isotropic perfect fluid is referred to as the Oppenheimer-Volkoff (OV) equation or the Tolman-Oppenheimer-Volkoff (TOV) equation in various General Relativity textbooks or research papers. We scrutinize the relevant original publications to argue that the former is the more appropriate terminology.