کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
5130448 | 1490420 | 2016 | 4 صفحه PDF | دانلود رایگان |
- Equilibrium in static spherical stars has been studied in the literature.
- The relevant equation is referred to with two names, OV or TOV (more popular).
- We compare Tolman׳s and Oppenheimer & Volkoff׳s papers.
- We find that they adopt diametrically opposite approaches to the same problem.
- 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.
Journal: Studies in History and Philosophy of Science Part B: Studies in History and Philosophy of Modern Physics - Volume 56, November 2016, Pages 13-16