Gas Accretion versus BH Merger driven Growth Modes of Supermassive Black Holes and Implications for the Little Red Dots
BibTeX Entry
@article{2026arXiv260215952B,
author = {{Barai}, Paramita},
title = {{Gas Accretion versus BH Merger driven Growth Modes of Supermassive Black Holes and Implications for the Little Red Dots}},
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics, High Energy Astrophysical Phenomena},
year = {2026},
month = feb,
eid = {arXiv:2602.15952},
pages = {arXiv:2602.15952},
archiveprefix = {arXiv},
eprint = {2602.15952},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260215952B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {agn-dominated, black hole mass, simulation, super-eddington, theory},
month_numeric = {2}
}
Back to bibliography