Compact Objects in Brans-Dicke Gravity

This paper aims to investigate the existence and properties of anisotropic quark stars in context self-interacting Brans–Dicke theory. In this theory, gravitational constant general relativity is replaced by a dynamical massive scalar field accompanied potential function. Researchers believe that strange may evolve from neutron when neutrons fail endure extreme temperature pressure interior region. As consequence, they breakdown into their constituent particles, known as quarks. order construct well-behaved star model under influence field, we formulate equations employing MIT bag model. The (strange matter equation state) most suitable choice for it has successfully described compactness certain stellar bodies. Furthermore, estimates mass based on data cosmic events GW170817 GW190425 support developed considering three types matter: strange, up, down. involved differentiates between false true vacuum. We consider static sphere with fluid employ observed masses radii candidates (RXJ 1856-37 PSR J1614-2230) matching conditions at boundary evaluate value constant. Further, impact state parameters viability (via energy conditions) well stability (through speed sound constraints) self-gravitating objects. It found obtained values lie within accepted range (58.9 MeV/fm3 ≤ B 91.5 MeV/fm3). Moreover, structure meets necessary criteria.