WebDec 1, 2007 · In this work, we present a generalized Delta-Eddington phase function to simplify the radiative transfer equation to an integral equation with respect to photon fluence rate. Comparing to the ... WebAug 21, 2024 · We perform non-hydrodynamical 2.5D simulations to study the dynamics of material above accretion disk based on the disk radiation pressure acting on dust. We assume a super-accreting underlying disk with the accretion rate of 10 times the Eddington rate with central black hole mass ranging from 107 up to 109M⊙. Such high accretion …
Hyperaccretion during tidal disruption events: Weakly bound …
WebMay 3, 2004 · The super-Eddington phase may increase black hole mass by up to an order of magnitude at an accretion efficiency of 42+/-33% over a period of 44+/-22Myr. Our results imply that super-Eddington ... Webgrowth factor expected in sub-Eddington phase is only 2. Therefore, the cosmic BH growth by accretion is likely dominated by super-Eddington phase, rather than sub-Eddington phase which is the majority among AGNs. This analysis is based on the fraction and the average accretion rate of NLS1s and NLQs obtained for z 0.5. If those numbers csu bakersfield admissions office
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WebMar 1, 2008 · A generalized Delta-Eddington phase function deduced by Cong et al. 14 can also accurately model the light propagation in tissues over a wide range of optical properties and be less time consuming ... WebWe present a generalized Delta-Eddington phase function to simplify the radiative transfer equation to integral equations with respect to both photon fluence rate and flux vector. The photon fluence rate and flux can be solved from the system of integral equations. By comparing to the Monte Carlo simulation results, the solutions of the system ... WebJun 28, 2009 · model approximates the phase function in RTE using the generalized Delta-Eddington phase * The authors are grateful for the support from the following grants : NIH/NIBIB EB001685, NIH/NIBIB ... csu bakersfield application