Facial reconstruction

Search LJMU Research Online

Browse Repository | Browse E-Theses

The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations

Crain, RA and Schaye, J and Bower, RG and Furlong, M and Schaller, M and Theuns, T and Vecchia, CD and Frenk, CS and McCarthy, IG and Helly, JC and Jenkins, A and Rosas-Guevara, YM and White, SDM and Trayford, JW (2015) The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations. Monthly Notices of the Royal Astronomical Society, 450 (2). pp. 1937-1961. ISSN 0035-8711

WarningThere is a more recent version of this item available.
[img] Text
1501.01311v2.pdf - Accepted Version

Download (2MB)

Abstract

We present results from thirteen cosmological simulations that explore the parameter space of the "Evolution and Assembly of GaLaxies and their Environments" (EAGLE) simulation project. Four of the simulations follow the evolution of a periodic cube L = 50 cMpc on a side, and each employs a different subgrid model of the energetic feedback associated with star formation. The relevant parameters were adjusted so that the simulations each reproduce the observed galaxy stellar mass function at z = 0.1. Three of the simulations fail to form disc galaxies as extended as observed, and we show analytically that this is a consequence of numerical radiative losses that reduce the efficiency of stellar feedback in high-density gas. Such losses are greatly reduced in the fourth simulation - the EAGLE reference model - by injecting more energy in higher density gas. This model produces galaxies with the observed size distribution, and also reproduces many galaxy scaling relations. In the remaining nine simulations, a single parameter or process of the reference model was varied at a time. We find that the properties of galaxies with stellar mass <~ M* (the "knee" of the galaxy stellar mass function) are largely governed by feedback associated with star formation, while those of more massive galaxies are also controlled by feedback from accretion onto their central black holes. Both processes must be efficient in order to reproduce the observed galaxy population. In general, simulations that have been calibrated to reproduce the low-redshift galaxy stellar mass function will still not form realistic galaxies, but the additional requirement that galaxy sizes be acceptable leads to agreement with a large range of observables.

Item Type: Article
Additional Information: This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record; Crain, R. A., Schaye, J., Bower, R. G., Furlong, M., Schaller, T. T., Vecchia, C. D., Frenk, C. S., McCarthy, I. G., Helly, J. C., Jenkins, A., Rosas-Guevara, Y. M., White, S. D. M., Trayford, J. W. (2015) The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations, is available online at: http://dx.doi.org/10.1093/mnras/stv725.
Uncontrolled Keywords: astro-ph.GA; astro-ph.GA
Subjects: Q Science > QB Astronomy
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press
Related URLs:
Date Deposited: 27 May 2015 13:56
Last Modified: 27 May 2015 13:56
DOI or Identification number: /10.1093/mnras/stv725
URI: http://researchonline.ljmu.ac.uk/id/eprint/694

Available Versions of this Item

Actions (login required)

View Item View Item