Matches in SemOpenAlex for { <https://semopenalex.org/work/W4381330481> ?p ?o ?g. }
- W4381330481 endingPage "515" @default.
- W4381330481 startingPage "473" @default.
- W4381330481 abstract "We review the progress in modeling the galaxy population in hydrodynamical simulations of the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed spatial clustering of galaxies; the distributions of key characteristics, such as mass, size, and SFR; and scaling relations connecting diverse properties to mass. Such improvements engender confidence in the insight drawn from simulations. Many important outcomes, however, particularly the properties of circumgalactic gas, are sensitive to the details of the subgrid models used to approximate the macroscopic effects of unresolved physics, such as feedback processes. We compare the outcomes of leading simulation suites with observations, and with each other, to identify the enduring successes they have cultivated and the outstanding challenges to be tackled with the next generation of models. Our key conclusions include the following: ▪ Realistic galaxies can be reproduced by calibrating the ill-constrained parameters of subgrid feedback models. Feedback is dominated by stars and black holes in low-mass and high-mass galaxies, respectively. ▪ Adjusting or disabling the processes implemented in simulations can elucidate their impact on observables, but outcomes can be degenerate. ▪ Similar galaxy populations can emerge in simulations with dissimilar feedback implementations. However, these models generally predict markedly different gas flow rates into, and out of, galaxies and their halos. CGM observations are thus a promising means of breaking this degeneracy and guiding the development of new feedback models." @default.
- W4381330481 created "2023-06-21" @default.
- W4381330481 creator A5007574967 @default.
- W4381330481 creator A5036077043 @default.
- W4381330481 date "2023-08-18" @default.
- W4381330481 modified "2023-10-04" @default.
- W4381330481 title "Hydrodynamical Simulations of the Galaxy Population: Enduring Successes and Outstanding Challenges" @default.
- W4381330481 cites W1488192889 @default.
- W4381330481 cites W1524313320 @default.
- W4381330481 cites W1529464840 @default.
- W4381330481 cites W1530653340 @default.
- W4381330481 cites W1534735367 @default.
- W4381330481 cites W1735913374 @default.
- W4381330481 cites W1753342680 @default.
- W4381330481 cites W1786331656 @default.
- W4381330481 cites W1801137374 @default.
- W4381330481 cites W1833181682 @default.
- W4381330481 cites W1843369788 @default.
- W4381330481 cites W1853164862 @default.
- W4381330481 cites W1859386239 @default.
- W4381330481 cites W1865574940 @default.
- W4381330481 cites W1894477963 @default.
- W4381330481 cites W1911876284 @default.
- W4381330481 cites W1921256341 @default.
- W4381330481 cites W1930253690 @default.
- W4381330481 cites W1934100704 @default.
- W4381330481 cites W1940538082 @default.
- W4381330481 cites W1941164020 @default.
- W4381330481 cites W1955258801 @default.
- W4381330481 cites W1964344398 @default.
- W4381330481 cites W1966671643 @default.
- W4381330481 cites W1968869120 @default.
- W4381330481 cites W1968879722 @default.
- W4381330481 cites W1969668528 @default.
- W4381330481 cites W1969717379 @default.
- W4381330481 cites W1970439842 @default.
- W4381330481 cites W1970587228 @default.
- W4381330481 cites W1975209025 @default.
- W4381330481 cites W1975983552 @default.
- W4381330481 cites W1977544711 @default.
- W4381330481 cites W1977635644 @default.
- W4381330481 cites W1978826987 @default.
- W4381330481 cites W1982221906 @default.
- W4381330481 cites W1982496618 @default.
- W4381330481 cites W1986545671 @default.
- W4381330481 cites W1988066154 @default.
- W4381330481 cites W1990523382 @default.
- W4381330481 cites W1993132186 @default.
- W4381330481 cites W1999114023 @default.
- W4381330481 cites W2005631644 @default.
- W4381330481 cites W2008429960 @default.
- W4381330481 cites W2008441954 @default.
- W4381330481 cites W2009802717 @default.
- W4381330481 cites W2011297915 @default.
- W4381330481 cites W2013997547 @default.
- W4381330481 cites W2015637674 @default.
- W4381330481 cites W2022594795 @default.
- W4381330481 cites W2027547158 @default.
- W4381330481 cites W2033599776 @default.
- W4381330481 cites W2035936423 @default.
- W4381330481 cites W2039226225 @default.
- W4381330481 cites W2039241537 @default.
- W4381330481 cites W2040364743 @default.
- W4381330481 cites W2040912209 @default.
- W4381330481 cites W2042081950 @default.
- W4381330481 cites W2042540695 @default.
- W4381330481 cites W2042561599 @default.
- W4381330481 cites W2042749826 @default.
- W4381330481 cites W2043137394 @default.
- W4381330481 cites W2047075180 @default.
- W4381330481 cites W2047501081 @default.
- W4381330481 cites W2047806989 @default.
- W4381330481 cites W2049062775 @default.
- W4381330481 cites W2049708373 @default.
- W4381330481 cites W2050322824 @default.
- W4381330481 cites W2050990527 @default.
- W4381330481 cites W2053740521 @default.
- W4381330481 cites W2054801391 @default.
- W4381330481 cites W2057367689 @default.
- W4381330481 cites W2062237753 @default.
- W4381330481 cites W2067029170 @default.
- W4381330481 cites W2067857092 @default.
- W4381330481 cites W2068262275 @default.
- W4381330481 cites W2068306188 @default.
- W4381330481 cites W2070803987 @default.
- W4381330481 cites W2071818181 @default.
- W4381330481 cites W2073424199 @default.
- W4381330481 cites W2075481628 @default.
- W4381330481 cites W2076246932 @default.
- W4381330481 cites W2077678988 @default.
- W4381330481 cites W2077852080 @default.
- W4381330481 cites W2078506508 @default.
- W4381330481 cites W2080977367 @default.
- W4381330481 cites W2084531715 @default.
- W4381330481 cites W2086089232 @default.
- W4381330481 cites W2089051030 @default.
- W4381330481 cites W2089118837 @default.
- W4381330481 cites W2093317565 @default.