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单词 Oppenheimer–Volkoff limit
释义
Oppenheimer–Volkoff limit

Physics
  • The maximum mass a neutron star can have before it undergoes gravitational collapse to a black hole. It is more difficult to estimate this limit than the analogous Chandrasekhar limit for white dwarf stars. It is thought that the Oppenheimer–Volkoff limit is between two and three times the mass of the sun. It was first calculated by Robert Oppenheimer (1904–67) and George Volkoff (1914–2000) in 1939.


Astronomy
  • The maximum mass that a neutron star can have without it being overwhelmed by its own gravity. Calculations put this between 1.6 and 2 solar masses, although the exact figure is uncertain. A neutron star with a mass greater than this is expected to collapse further into a black hole. The limit is named after the American physicist (Julius) Robert Oppenheimer (1904–67) and the Russian-born Canadian George Michael Volkoff (1914–2000).


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