Jet-driven active galactic nucleus feedback in galaxy formation before black hole formation
Ealeal Bear, Noam Soker

TL;DR
This paper proposes a novel galaxy formation scenario where jets from a supermassive star, before black hole formation, influence galaxy evolution and establish a mass relation between the SMBH and the galaxy/bulge.
Contribution
It introduces a new feedback mechanism involving jets from a supermassive star prior to black hole formation, linking SMBH and galaxy mass.
Findings
Jets carry about 10% of SMS mass and have enough energy to impact galaxy gas.
A correlation between SMBH mass and galaxy/bulge stellar mass is established early.
Jets may unbind most of the gas in the galaxy/bulge during SMBH formation.
Abstract
We propose a scenario where during galaxy formation an active galactic nucleus (AGN) feedback mechanism starts before the formation of a supermassive black hole (SMBH). The supermassive star (SMS) progenitor of the SMBH accretes mass as it grows and launches jets. We simulate the evolution of SMSs and show that the escape velocity from their surface is approximately several 10^3 km/s, with large uncertainties. We could not converge with the parameters of the evolutionary numerical code MESA to resolve the uncertainties for SMS evolution. Under the assumption that the jets carry about ten percent of the mass of the SMS, we show that the energy in the jets is a substantial fraction of the binding energy of the gas in the galaxy/bulge. Therefore, the jets that the SMS progenitor of the SMBH launches carry sufficient energy to establish a feedback cycle with the gas in the inner zone of the…
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