• In astrophysics, the TolmanOppenheimerVolkoff (TOV) equation constrains the structure of a spherically symmetric body of isotropic material which is...
    12 KB (2,080 words) - 05:37, 24 January 2024
  • The TolmanOppenheimerVolkoff limit (or TOV limit) is an upper bound to the mass of cold, non-rotating neutron stars, analogous to the Chandrasekhar limit...
    39 KB (4,295 words) - 05:40, 17 June 2024
  • Thumbnail for J. Robert Oppenheimer
    Cores," which demonstrated that there was a limit, known as the TolmanOppenheimerVolkoff limit, to the mass of stars beyond which they would not remain...
    169 KB (18,864 words) - 22:22, 15 June 2024
  • Thumbnail for Richard C. Tolman
    test Tolman's paradox Tolman's H theorem Tolman–Ehrenfest effect TolmanOppenheimerVolkoff equation TolmanOppenheimerVolkoff limit Lemaître–Tolman metric...
    12 KB (1,139 words) - 23:25, 10 December 2023
  • Thumbnail for Neutron star
    on constraining the equation of state with the speed of sound through hydrodynamics. The Tolman-Oppenheimer-Volkoff (TOV) equation can be used to describe...
    113 KB (13,658 words) - 02:35, 17 June 2024
  • stars, obtaining the Tolman-Oppenheimer-Volkoff limit. Oppenheimer would not revisit the topic in future publications. The Oppenheimer–Snyder model of continued...
    12 KB (1,515 words) - 22:08, 17 June 2024
  • field equations (EFE; also known as Einstein's equations) relate the geometry of spacetime to the distribution of matter within it. The equations were...
    34 KB (5,096 words) - 09:51, 5 June 2024
  • censorship hypothesis [3][4]), George Volkoff (TolmanOppenheimerVolkoff limit, TolmanOppenheimerVolkoff equation) Robert M. Wald (textbook, black-hole...
    20 KB (1,810 words) - 08:46, 15 October 2023
  • Chandrasekhar limit follows from this limit. Emden–Chandrasekhar equation TolmanOppenheimerVolkoff equation Chandrasekhar, Subrahmanyan, and Subrahmanyan Chandrasekhar...
    6 KB (1,430 words) - 15:35, 5 June 2024
  • Thumbnail for Hydrostatic equilibrium
    {\displaystyle \nabla _{\mu }T^{\mu \nu }=0} one can derive the TolmanOppenheimerVolkoff equation for the structure of a static, spherically symmetric relativistic...
    27 KB (4,411 words) - 09:40, 17 June 2024