The Tolman-Oppenheimer-Volkoff (TOV) equation is a fundamental relationship in astrophysics that describes the structure of a stable, spherically symmetric star in hydrostatic equilibrium, particularly neutron stars. It extends the principles of general relativity to account for the effects of gravity on dense matter. The TOV equation can be expressed mathematically as:
where is the pressure, is the density, is the mass within radius , is the gravitational constant, and is the speed of light. This equation helps in understanding the maximum mass that a neutron star can have, known as the Tolman-Oppenheimer-Volkoff limit, which is crucial for predicting the outcomes of supernova explosions and the formation of black holes. By analyzing solutions to the TOV equation, astrophysicists
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