Aspects of Black Hole Physics and Formation of Super-massive Black Holes from Ultra-light Dark Bosons
Patrick Das Gupta, Fazlu Rahman

TL;DR
This paper explores how ultra-light dark bosons forming Bose-Einstein condensates could lead to supermassive black hole formation and generate detectable gravitational waves, linking dark matter physics with galaxy evolution.
Contribution
It proposes a novel mechanism for SMBH formation via dark boson BEC collapse and analyzes potential GW signals, integrating dark matter physics with black hole and galaxy formation theories.
Findings
SMBHs can form from dark boson BEC collapse within 10^8 years.
Oscillations in BECs may cause star formation bursts in galactic nuclei.
Estimated GW signals could be detectable by Pulsar Timing Arrays.
Abstract
First, we verify that the physical parameters estimated for the four directly detected gravitational wave (GW) events involving coalescence of binary black holes (BHs) indeed uphold the second law of BH thermodynamics, strengthening further the case for BH physics. Non-spherical gravitational collapse leading to BH formation may entail very high GW luminosities during the final phase of implosion, reaching non-negligible fraction of Dyson luminosity . Most galaxies harbor supermassive black holes (SMBHs) in their nuclear regions. Several bright quasars detected at redshifts 6 are powered by accreting SMBHs of mass when the universe was only yrs old. We posit that creation of SMBHs occurs due to collapse (on dynamical time scales yrs) of ultra-light bosonic dark matter (DM) particles that have undergone Bose-Einstein…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Cosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena
