FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4311158903> ?p ?o ?g. }

• W4311158903 endingPage "3181" @default.
• W4311158903 startingPage "3154" @default.
• W4311158903 abstract "Increasingly, uncertainties in predictions from galaxy formation simulations (at sub-Milky Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we present the full set of updates from the FIRE-2 version of the Feedback In Realistic Environments (FIRE) project code, to the next version, FIRE-3. While the transition from FIRE-1 to FIRE-2 focused on improving numerical methods, here we update the stellar evolution tracks used to determine stellar feedback inputs, e.g. stellar mass-loss (O/B and AGB), spectra (luminosities and ionization rates), and supernova rates (core-collapse and Ia), as well as detailed mass-dependent yields. We also update the low-temperature cooling and chemistry, to enable improved accuracy at $T lesssim 10^{4},$K and densities $ngg 1,{rm cm^{-3}}$, and the meta-galactic ionizing background. All of these synthesize newer empirical constraints on these quantities and updated stellar evolution and yield models from a number of groups, addressing different aspects of stellar evolution. To make the updated models as accessible as possible, we provide fitting functions for all of the relevant updated tracks, yields, etc, in a form specifically designed so they can be directly 'plugged in' to existing galaxy formation simulations. We also summarize the default FIRE-3 implementations of 'optional' physics, including spectrally-resolved cosmic rays and supermassive black hole growth and feedback." @default.
• W4311158903 created "2022-12-24" @default.
• W4311158903 creator A5000130235 @default.
• W4311158903 creator A5006598619 @default.
• W4311158903 creator A5007260627 @default.
• W4311158903 creator A5008589829 @default.
• W4311158903 creator A5013583777 @default.
• W4311158903 creator A5017618068 @default.
• W4311158903 creator A5028360288 @default.
• W4311158903 creator A5030482289 @default.
• W4311158903 creator A5030664030 @default.
• W4311158903 creator A5038345854 @default.
• W4311158903 creator A5038938655 @default.
• W4311158903 creator A5039703536 @default.
• W4311158903 creator A5042534433 @default.
• W4311158903 creator A5044296184 @default.
• W4311158903 creator A5054017292 @default.
• W4311158903 creator A5063586360 @default.
• W4311158903 creator A5070973306 @default.
• W4311158903 creator A5071642553 @default.
• W4311158903 creator A5078455868 @default.
• W4311158903 creator A5083397483 @default.
• W4311158903 creator A5084431981 @default.
• W4311158903 creator A5091350146 @default.
• W4311158903 date "2022-12-02" @default.
• W4311158903 modified "2023-10-18" @default.
• W4311158903 title "FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations" @default.
• W4311158903 cites W1488192889 @default.
• W4311158903 cites W1569925696 @default.
• W4311158903 cites W1587885137 @default.
• W4311158903 cites W1624693442 @default.
• W4311158903 cites W1647534366 @default.
• W4311158903 cites W1737490605 @default.
• W4311158903 cites W1766563480 @default.
• W4311158903 cites W1810790886 @default.
• W4311158903 cites W1831661775 @default.
• W4311158903 cites W1850315173 @default.
• W4311158903 cites W1894488274 @default.
• W4311158903 cites W1894745560 @default.
• W4311158903 cites W1925826255 @default.
• W4311158903 cites W1929623410 @default.
• W4311158903 cites W1933422323 @default.
• W4311158903 cites W1947399493 @default.
• W4311158903 cites W1963813317 @default.
• W4311158903 cites W1964055719 @default.
• W4311158903 cites W1966671643 @default.
• W4311158903 cites W1968879722 @default.
• W4311158903 cites W1969514664 @default.
• W4311158903 cites W1973306255 @default.
• W4311158903 cites W1975983552 @default.
• W4311158903 cites W1977457396 @default.
• W4311158903 cites W1977635644 @default.
• W4311158903 cites W1978220441 @default.
• W4311158903 cites W1985147370 @default.
• W4311158903 cites W1986303447 @default.
• W4311158903 cites W1987861871 @default.
• W4311158903 cites W1993230081 @default.
• W4311158903 cites W1994671833 @default.
• W4311158903 cites W2000672249 @default.
• W4311158903 cites W2006147525 @default.
• W4311158903 cites W2006869439 @default.
• W4311158903 cites W2008951787 @default.
• W4311158903 cites W2013285588 @default.
• W4311158903 cites W2016258946 @default.
• W4311158903 cites W2018314021 @default.
• W4311158903 cites W2019387002 @default.
• W4311158903 cites W2025078251 @default.
• W4311158903 cites W2026328109 @default.
• W4311158903 cites W2028466334 @default.
• W4311158903 cites W2029712140 @default.
• W4311158903 cites W2034303391 @default.
• W4311158903 cites W2035110056 @default.
• W4311158903 cites W2039115612 @default.
• W4311158903 cites W2047075180 @default.
• W4311158903 cites W2047798125 @default.
• W4311158903 cites W2048258434 @default.
• W4311158903 cites W2048274049 @default.
• W4311158903 cites W2049247811 @default.
• W4311158903 cites W2050322824 @default.
• W4311158903 cites W2051468747 @default.
• W4311158903 cites W2053740521 @default.
• W4311158903 cites W2054450804 @default.
• W4311158903 cites W2054801391 @default.
• W4311158903 cites W2056935071 @default.
• W4311158903 cites W2059037849 @default.
• W4311158903 cites W2060128328 @default.
• W4311158903 cites W2065437916 @default.
• W4311158903 cites W2066265110 @default.
• W4311158903 cites W2068928940 @default.
• W4311158903 cites W2069887781 @default.
• W4311158903 cites W2070922409 @default.
• W4311158903 cites W2071884317 @default.
• W4311158903 cites W2071933657 @default.
• W4311158903 cites W2073315382 @default.
• W4311158903 cites W2075481628 @default.
• W4311158903 cites W2076246932 @default.
• W4311158903 cites W2077363791 @default.
• W4311158903 cites W2078030216 @default.

• next