BLACK HOLE GROWTH AND ACTIVE GALACTIC NUCLEI OBSCURATION BY INSTABILITY-DRIVEN INFLOWS IN HIGH-REDSHIFT DISK GALAXIES FED BY COLD STREAMS

Disk galaxies at high redshift have been predicted to maintain high gas surface densities due to continuous feeding by intense cold streams leading to violent gravitational instability, transient features, and giant clumps. Gravitational torques between the perturbations drive angular momentum out and mass in, and the inflow provides the energy for keeping strong turbulence. We use analytic estimates of the inflow for a self-regulated unstable disk at a Toomre stability parameter Q similar to 1, and isolated galaxy simulations capable of resolving the nuclear inflow down to the central parsec. We predict an average inflow rate similar to 10 M-circle dot yr(-1) through the disk of a 10(11) M-circle dot galaxy, with conditions representative of z similar to 2 stream-fed disks. The inflow rate scales with disk mass and (1 + z)(3/2). It includes clump migration and inflow of the smoother component, valid even if clumps disrupt. This inflow grows the bulge, while only a fraction of greater than or similar to 10(-3) of it needs to accrete onto a central black hole (BH), in order to obey the observed BH-bulge relation. A galaxy of 10(11) M-circle dot at z similar to 2 is expected to host a BH of similar to 10(8) M-circle dot, accreting on average with moderate sub-Eddington luminosity L-X similar to 10(42)-10(43) erg s(-1), accompanied by brighter episodes when dense clumps coalesce. We note that in rare massive galaxies at z similar to 6, the same process may feed similar to 10(9) M-circle dot BH at the Eddington rate. High central gas column densities can severely obscure active galactic nuclei in high-redshift disks, possibly hindering their detection in deep X-ray surveys.