nLab
structure formation

Contents

Contents

Idea

In the context of cosmology, structure formation refers to the process by which cosmological structures such as galaxy clusters and galaxies themselves form under gravitational collapse of a primordial gas.

Various computer simulations (Millennium I, Millennium II, Millennium XXL, Illustris) test theory against observations, such as those by the Planck Collaboration, see Springel 13 for survey.

graphics from The Millennium Simulation Project

Feedback mechanisms and realistic dark matter models

A revolution in realism of computer simulations of galaxy structure formation occurred after ~2010 when hardware and software advances allowed to resolve various feedback mechanisms, such as notably the effect of star-formation inside a gas cloud collapsing to a galaxy. This advance is reflected in the naming of the FIRE-project: Feedback In Realistic Environments.

The resolution of such feedback mechanisms in simulation of galaxy formation seems to resolve long-standing apparent discrepancies of dark matter models with observed galaxy-scale phenomena: For example galactic rotation curves are qualitatively reproduced (Hopkins 17, Figure 4, Figure 5) as is the baryonic Tully-Fisher relation (El-Badry 18, Figure 4).

For more on this see also at dark matter the section On galactic scales.

From Vogelsberger et al. 14:

The simulation reproduces reasonably well the cosmic star formation rate density, the galaxy luminosity function, and baryon conversion efficiency at z=0z=0. It also qualitatively captures the impact of galaxy environment on the red fractions of galaxies. The internal velocity structure of selected well-resolved disk galaxies obeys the stellar and baryonic Tully-Fisher relation together with flat circular velocity curves. In the well-resolved regime the simulation reproduces the observed mix of early-type and late-type galaxies.

See also Illustris Project Website: What are we learning? and Preliminary Results.

References

Review includes

  • Joel Primack, Dark Matter and Structure Formation in the Universe, Chapter 1 of Formation of Structure in the Universe, Proceedings of the Jerusalem Winter School 1996, edited by A. Dekel and J.P. Ostriker (arXiv:astro-ph/9707285)

  • Daniel Baumann, The big bang and the origin of structure, 2019 (web)

Galaxy formation:

  • Julio Navarro, Simulations of Galaxy Formation: the State of the Art (pdf)

  • Justin Read et al. EDGE I: the mass-metallicity relation as a critical test of galaxy formation physics (arXiv:1904.02723)

See also

Computer simulation

There are various computer simulations for cosmic structure formation, listed below. Review includes the following:

Millennium Project

Millennium I
Millennium II
  • Michael Boylan-Kolchin, Volker Springel, Simon D. M. White, Adrian Jenkins, Gerard Lemson, Resolving Cosmic Structure Formation with the Millennium-II Simulation, Mon.Not.Roy.Astron.Soc.398:1150, 2009 (arXiv:0903.3041)
Millennium XXL
  • The Millennium-XXL Project: Simulating the Galaxy Population of dark Energy Universes (pdf)

  • R. E. Angulo, V. Springel, S. D. M. White, A. Jenkins, C. M. Baugh, C. S. Frenk, Scaling relations for galaxy clusters in the Millennium-XXL simulation, Monthly Notices of the Royal Astronomical Society, Volume 426, Issue 3, 1 November 2012, Pages 2046–2062, (doi:10.1111/j.1365-2966.2012.21830.x, arXiv:1203.3216)

Illustris Project

  • Illustris Project Website

  • Wikipedia, Illustris project

  • Mark Vogelsberger, Shy Genel, Volker Springel, Paul Torrey, Debora Sijacki, Dandan Xu, Greg Snyder, Dylan Nelson, Lars Hernquist, Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe (arXiv:1405.2921)

FIRE

galaxy formation

galactic rotation curves qualitatively reproduced in Hopkins 17, Figure 4, Figure 5

baryonic Tully-Fisher relation qualitatively reproduced in El-Badry 18, Figure 4

  • Daniel Angles-Alcazar, Multi-scale physical modeling in galaxy formation and evolution, 2019 (web)

Other

Last revised on April 10, 2020 at 11:36:23. See the history of this page for a list of all contributions to it.