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Local non-Gaussianities from cross-correlations between the CMB and 21-cm
Giorgio Orlando, Thomas Flöss, P. Daniel Meerburg +1
The 21-cm brightness temperature fluctuation from the Dark Ages () will allow us to probe the inflationary epoch on very small scales ($>0.1 \, \mbox{Mpc}^{-1}$),…
Microlensing Black Hole Shadows
Himanshu Verma, Joseph Silk
A detailed analysis is presented of gravitational microlensing by intervening compact objects of the black hole shadows imaged by the Event Horizon Telescope (EHT). We show how the…
TRINITY III: Quasar Luminosity Functions Decomposed by Halo, Galaxy, and Black Hole Masses and Eddington Ratios from z=0-10
Haowen Zhang, Peter Behroozi, Marta Volonteri +5
We present the redshift evolution of quasar luminosity functions decomposed by halo mass, galaxy mass, supermassive black hole (SMBH) mass, and Eddington ratio, as well as SMBH kin…
Magnetic fields catalyze massive black hole formation and growth
Mitchell C. Begelman, Joseph Silk
Large-scale magnetic fields in the nuclear regions of protogalaxies can promote the formation and early growth of supermassive black holes (SMBHs) by direct collapse and magnetical…
Neutrino signals from Neutron Star implosions to Black Holes
Yossef Zenati, C. Albertus, M. Ángeles Pérez-García +1
We calculate the neutrino luminosity in an astrophysical scenario where dark matter is captured by a neutron star which eventually implodes to form a low mass black hole. The Troja…
TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at
Haowen Zhang, Peter Behroozi, Marta Volonteri +5
Using recent empirical constraints on the dark matter halo--galaxy--supermassive black hole (SMBH) connection from , we infer how undermassive, typical, and overmassive SMBH…