Quark Masses, Black Neutron Stars and SSI Conception of the Universe

Abstract

Recently, it was found that a quark’s mass in the scalar strong interaction hadron theory SSI can deviate from some mean value within certain limits, depending upon the flavor and spin of its companion antiquark in a meson. Here, such values and limits are determined and specified with greater accuracy that led to improved predictions of meson masses. The black neutron star recent observed in the kilonova S250206dm confirms the 2019 SSI prediction of such an object. This prediction has been further developed to a “peach” model for conventional black holes. A neutron star at the verge of its Tolman, Oppenheimer, Volkoff limit replaces the gravitational singularity in the expected black hole. Such a black object, including supermassive such, is actually a black neutron star with a dense core of a neutron star of about 3.65 solar masses and a 10.8 km radius. Our present conception of the basic forces and their relations in the universe based upon the standard model is hereby modified to accommodate SSI.