The Tolman-Oppenheimer-Volkoff (TOV) equation is a fundamental result in the field of astrophysics that describes the structure of a static, spherically symmetric body in hydrostatic equilibrium under the influence of gravity. It is particularly important for understanding the properties of neutron stars, which are incredibly dense remnants of supernova explosions. The TOV equation takes into account both the effects of gravity and the pressure within the star, allowing us to relate the pressure at a distance from the center of the star to the energy density .
The equation is given by:
where:
The TOV equation is pivotal in predicting the maximum mass of neutron stars, known as the **
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