M
Muhammad Latif
Researcher at King Faisal University
Publications - 371
Citations - 6534
Muhammad Latif is an academic researcher from King Faisal University. The author has contributed to research in topics: Convex function & Hermite polynomials. The author has an hindex of 38, co-authored 308 publications receiving 5187 citations. Previous affiliations of Muhammad Latif include University of the Witwatersrand & University of Göttingen.
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Early growth of high redshift black holes
TL;DR: In this article, the authors performed a radiation hydrodynamics cosmological simulation to study the growth of "normal" black holes in the high redshift universe and found that the stunted growth of MBH is a consequence of supernovae in tandem with MBH feedback which drive large outflows and evacuate the gas from MBH vicinity.
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Black hole formation in the early Universe
TL;DR: In this paper, the authors present the highest resolution cosmological large-eddy simulations to date which track the evolution of high-density regions on scales of $0.25$~AU beyond the formation of the first peak, and study the impact of subgrid-scale turbulence.
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The characteristic black hole mass resulting from direct collapse in the early Universe
TL;DR: In this article, the formation of supermassive black holes via cosmological large eddy simulations (LES) by employing sink particles and following their evolution for twenty thousand years after the creation of the first sink was investigated.
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Integrated application of upflow anaerobic sludge blanket reactor for the treatment of wastewaters.
TL;DR: The general characterization of wastewater, treatment in UASB reactor with operational parameters and reactor performance in terms of COD removal and biogas production are thoroughly discussed and concrete data illustrates the reactor configuration, thus giving maximum awareness about upflow anaerobic sludge blanket reactor for further research.
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Massive black hole factories: Supermassive and quasi-star formation in primordial halos
TL;DR: In this article, the authors explored how long rapidly accreting protostars remain on the Hayashi track, implying large protostellar radii and weak accretion luminosity feedback.