KnowraTolman–Oppenheimer–Volkoff limitLinked fromLinked fromThe 6 pages that link to Tolman–Oppenheimer–Volkoff limit, each with the reason it gives.All 6Related 5Compared with 1Neutron starRelated: Beyond this limit, pressure cannot prevent collapse into a black hole.Neutron degeneracy pressureRelated: It marks where pressure support can no longer balance gravity in a neutron star.Solar massRelated: Neutron-star mass estimates in solar masses test where this uncertain threshold lies.Degenerate matterRelated: It marks where gravity defeats the pressure and interactions sustaining a neutron star.Stellar black holeRelated: A collapsing remnant above this limit cannot remain a neutron star.