A5093550401- Galaxies: Formation, Evolution, Phenomena
- Cosmology and Gravitation Theories
- Adaptive optics and wavefront sensing
- Radio Astronomy Observations and Technology
- Black Holes and Theoretical Physics
- Pulsars and Gravitational Waves Research
- Astronomy and Astrophysical Research
- Computational Physics and Python Applications
- Astrophysical Phenomena and Observations
University of Hawaiʻi at Mānoa
2023-2024
University of Hawaii System
2024
Abstract Coupling of black hole mass to the cosmic expansion has been suggested as a possible path understanding dark energy content Universe. We test this hypothesis by comparing supermassive (SMBH) density at z = 0 total accreted in active galactic nuclei (AGN) since 6, constrain how much SMBH can arise from cosmologically coupled growth, opposed growth accretion. Using an estimate local ≈1.0 × 10 6 M ⊙ Mpc −1 , radiative accretion efficiency, η range 0.05 < 0.3, and observed AGN...
The assembly of supermassive black hole (SMBH) mass ($M_{\bullet}$) and stellar ($M_{*}$) in galaxies can be studied via the redshift evolution $M_{\bullet}-M_{*}$ relation, but ways which selection bias physical channels affect this are uncertain. To address this, we compare relation for local massive ($M_{*}>10^{10.5}$M$_{\odot}$) quiescent early-type (ETGs) to that ETGs hosting active galactic nuclei (AGN) at $z\sim0.8$. restrictions on galaxy type limit may connect two relations. For...
Abstract The assembly of supermassive black hole (SMBH) mass ( M • ) and stellar * in galaxies can be studied via the redshift evolution – relation, but ways which selection bias physical channels affect this are uncertain. To address this, we compare relation for local massive > 10 10.5 ⊙ quiescent early-type (ETGs) to that ETGs hosting active galactic nuclei (AGN) at z ∼ 0.8. restrictions on galaxy type limit may connect two relations. For sample find <mml:math...
Coupling of black hole mass to the cosmic expansion has been suggested as a possible path understanding dark energy content Universe. We test this hypothesis by comparing supermassive (SMBH) density at $z=0$ total accreted in AGN since $z=6$, constrain how much SMBH can arise from cosmologically-coupled growth, opposed growth accretion. Using an estimate local $\approx 1.0\times10^{6}\,$M$_{\odot}\,$Mpc$^{-1}$, radiative accretion efficiency, $\eta$: $0.05<\eta<0.3$, and observed luminosity...