The loss-cone problem in dense nuclei

We address the classical problem of star accretion on to a supermassive central gaseous object in a galactic nucleus. The resulting supermassive central star-gas object is assumed to be located at the centre of a dense stellar system for which we use a simplified model consisting of a Plummer model with an embedded density cusp using stellar point masses. From the number of stars belonging to the loss-cone, which plunge on to the central object on elongated orbits from outside, we estimate the accretion rate taking into account a possible anisotropy of the surrounding stellar distribution. The total heating rate in the supermassive star as a result of the loss-cone stars plunging on to it is estimated. This semi-analytical study, revisiting and expanding the work of the classical paper, is a starting point for future work on a more detailed study of early evolutionary phases of galactic nuclei. It merits closer examination, because it is one of the key features for the link between cosmology and galaxy formation.