Welcome to GALNUC Research Group's website!

GalNUC Research Group

Astrophysical Dynamics and

Statistical Mechanics of Galactic Nuclei


The GALNUC Astrodynamics and Statistical Mechanics Group (PI: Bence Kocsis) at Oxford and Eötvös University does research on topics related to galactic dynamics, dense stellar systems, physics of compact objects, statistical mechanics, ordered/disordered systems, and phase transitions. The group is funded by the ERC Starting Grant GalNUC and strives to develop a comprehensive model to describe the long term behavior of astrophysical multibody systems using revolutionary multidisciplanary methods.


We solve some of the major unsolved questions of galactic nuclei. Galactic nuclei host a central supermassive black hole, a dense population of stars and compact objects, and in many cases a bright gaseous disk feeding the supermassive black hole. The observed stellar distribution exhibits both spherical and counterrotating disk-like structures. Existing theoretical models cannot convincingly explain the origin of the stellar disks. Is there also a “dark cusp” or “dark disk” of stellar mass black holes? Are there intermediate mass black holes in the Galactic center? We examine the statistical physics of galactic nuclei and their long term dynamical evolution. A star orbiting a supermassive black hole on an eccentric precessing orbit covers an axisymmetric annulus. The long-term gravitational interaction between such annuli is similar to the Coulomb interaction between axisymmetric molecules constituting a liquid crystal. We apply standard methods of condensed matter physics to examine these astrophysical systems. The observed disk and spherical structures represent isotropic-nematic phase transitions. We derive the phase space distribution and time-evolution of different stellar components including a population of black holes. Further, we investigate the interaction of a stellar cluster with a gaseous disk, if present. This leads to the formation of gaps, warps, and spiral waves in the disk, the redistribution of stellar objects, and possibly the formation of intermediate mass black holes. We explore the implications for electromagnetic and gravitational wave observatories. Dark disks of black holes could provide the most frequent source of gravitational waves for LIGO and VIRGO. These detectors have recently opened a new window on the Universe; the proposed project opens a new field in gravitational wave astrophysics to interpret the sources. We also explore implications for electromagnetic observations.


European Research Council - Starting Grant GalNUC

on behalf of the European Commission



Horizon 2020

European Union funding

for Research & Innovation


Bence Kocsis

Email:        bence.kocsis@physics.ox.ac.uk

Address:    Rudolf Peierls Center for Theoretical Physics

                  University of Oxford

                  Parks Road

                  Oxford OX1 3PU

                  United Kingdom