@article{dave_simba_2019,
	title = {{SIMBA}: {Cosmological} simulations with black hole growth and feedback},
	volume = {486},
	shorttitle = {{SIMBA}},
	url = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D/abstract},
	doi = {10.1093/mnras/stz937},
	abstract = {We introduce the SIMBA simulations, the next generation of the MUFASA cosmological galaxy formation simulations run with GIZMO's meshless finite mass hydrodynamics. SIMBA includes updates to MUFASA's sub-resolution star formation and feedback prescriptions, and introduces black hole growth via the torque-limited accretion model of Anglés-Alcázar et al. from cold gas and Bondi accretion from hot gas, along with black hole feedback via kinetic bipolar outflows and X-ray energy. Ejection velocities are taken to be \{̃ \} 10{\textasciicircum}3 km s{\textasciicircum}\{-1\} at high Eddington ratios, increasing to \{̃ \} 8000 km s{\textasciicircum}\{-1\} at Eddington ratios below 2 per cent, with a constant momentum input of 20L/c. SIMBA further includes an on-the-fly dust production, growth, and destruction model. Our SIMBA run with (100h{\textasciicircum}\{-1\} Mpc){\textasciicircum}3 and 1024{\textless}SUP{\textgreater}3{\textless}/SUP{\textgreater} gas elements reproduces numerous observables, including galaxy stellar mass functions at z = 0-6, the stellar mass-star formation rate main sequence, H I and H{\textless}SUB{\textgreater}2{\textless}/SUB{\textgreater} fractions, the mass-metallicity relation at z ≈ 0, 2, star-forming galaxy sizes, hot gas fractions in massive haloes, and z = 0 galaxy dust properties. However, SIMBA also yields an insufficiently sharp truncation of the z = 0 mass function, and too-large sizes for low-mass quenched galaxies. We show that SIMBA's jet feedback is primarily responsible for quenching massive galaxies.},
	language = {en},
	number = {2},
	urldate = {2019-05-06},
	journal = {Monthly Notices of the Royal Astronomical Society},
	author = {Davé, Romeel and Anglés-Alcázar, Daniel and Narayanan, Desika and Li, Qi and Rafieferantsoa, Mika H. and Appleby, Sarah},
	month = jun,
	year = {2019},
	pages = {2827},
}

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SIMBA includes updates to MUFASA's sub-resolution star formation and feedback prescriptions, and introduces black hole growth via the torque-limited accretion model of Anglés-Alcázar et al. from cold gas and Bondi accretion from hot gas, along with black hole feedback via kinetic bipolar outflows and X-ray energy. Ejection velocities are taken to be \\̃ \\ 10\\textasciicircum3 km s\\textasciicircum\\-1\\ at high Eddington ratios, increasing to \\̃ \\ 8000 km s\\textasciicircum\\-1\\ at Eddington ratios below 2 per cent, with a constant momentum input of 20L/c. SIMBA further includes an on-the-fly dust production, growth, and destruction model. Our SIMBA run with (100h\\textasciicircum\\-1\\ Mpc)\\textasciicircum3 and 1024\\textlessSUP\\textgreater3\\textless/SUP\\textgreater gas elements reproduces numerous observables, including galaxy stellar mass functions at z = 0-6, the stellar mass-star formation rate main sequence, H I and H\\textlessSUB\\textgreater2\\textless/SUB\\textgreater fractions, the mass-metallicity relation at z ≈ 0, 2, star-forming galaxy sizes, hot gas fractions in massive haloes, and z = 0 galaxy dust properties. However, SIMBA also yields an insufficiently sharp truncation of the z = 0 mass function, and too-large sizes for low-mass quenched galaxies. We show that SIMBA's jet feedback is primarily responsible for quenching massive galaxies.","language":"en","number":"2","urldate":"2019-05-06","journal":"Monthly Notices of the Royal Astronomical Society","author":[{"propositions":[],"lastnames":["Davé"],"firstnames":["Romeel"],"suffixes":[]},{"propositions":[],"lastnames":["Anglés-Alcázar"],"firstnames":["Daniel"],"suffixes":[]},{"propositions":[],"lastnames":["Narayanan"],"firstnames":["Desika"],"suffixes":[]},{"propositions":[],"lastnames":["Li"],"firstnames":["Qi"],"suffixes":[]},{"propositions":[],"lastnames":["Rafieferantsoa"],"firstnames":["Mika","H."],"suffixes":[]},{"propositions":[],"lastnames":["Appleby"],"firstnames":["Sarah"],"suffixes":[]}],"month":"June","year":"2019","pages":"2827","bibtex":"@article{dave_simba_2019,\n\ttitle = {{SIMBA}: {Cosmological} simulations with black hole growth and feedback},\n\tvolume = {486},\n\tshorttitle = {{SIMBA}},\n\turl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D/abstract},\n\tdoi = {10.1093/mnras/stz937},\n\tabstract = {We introduce the SIMBA simulations, the next generation of the MUFASA cosmological galaxy formation simulations run with GIZMO's meshless finite mass hydrodynamics. SIMBA includes updates to MUFASA's sub-resolution star formation and feedback prescriptions, and introduces black hole growth via the torque-limited accretion model of Anglés-Alcázar et al. from cold gas and Bondi accretion from hot gas, along with black hole feedback via kinetic bipolar outflows and X-ray energy. Ejection velocities are taken to be \\{̃ \\} 10{\\textasciicircum}3 km s{\\textasciicircum}\\{-1\\} at high Eddington ratios, increasing to \\{̃ \\} 8000 km s{\\textasciicircum}\\{-1\\} at Eddington ratios below 2 per cent, with a constant momentum input of 20L/c. SIMBA further includes an on-the-fly dust production, growth, and destruction model. Our SIMBA run with (100h{\\textasciicircum}\\{-1\\} Mpc){\\textasciicircum}3 and 1024{\\textless}SUP{\\textgreater}3{\\textless}/SUP{\\textgreater} gas elements reproduces numerous observables, including galaxy stellar mass functions at z = 0-6, the stellar mass-star formation rate main sequence, H I and H{\\textless}SUB{\\textgreater}2{\\textless}/SUB{\\textgreater} fractions, the mass-metallicity relation at z ≈ 0, 2, star-forming galaxy sizes, hot gas fractions in massive haloes, and z = 0 galaxy dust properties. However, SIMBA also yields an insufficiently sharp truncation of the z = 0 mass function, and too-large sizes for low-mass quenched galaxies. We show that SIMBA's jet feedback is primarily responsible for quenching massive galaxies.},\n\tlanguage = {en},\n\tnumber = {2},\n\turldate = {2019-05-06},\n\tjournal = {Monthly Notices of the Royal Astronomical Society},\n\tauthor = {Davé, Romeel and Anglés-Alcázar, Daniel and Narayanan, Desika and Li, Qi and Rafieferantsoa, Mika H. and Appleby, Sarah},\n\tmonth = jun,\n\tyear = {2019},\n\tpages = {2827},\n}\n\n","author_short":["Davé, R.","Anglés-Alcázar, D.","Narayanan, D.","Li, Q.","Rafieferantsoa, M. H.","Appleby, S."],"key":"dave_simba_2019","id":"dave_simba_2019","bibbaseid":"dav-anglsalczar-narayanan-li-rafieferantsoa-appleby-simbacosmologicalsimulationswithblackholegrowthandfeedback-2019","role":"author","urls":{"Paper":"https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D/abstract"},"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://bibbase.org/zotero/polyphant","dataSources":["7gvjSdWrEu7z5vjjj"],"keywords":[],"search_terms":["simba","cosmological","simulations","black","hole","growth","feedback","davé","anglés-alcázar","narayanan","li","rafieferantsoa","appleby"],"title":"SIMBA: Cosmological simulations with black hole growth and feedback","year":2019}