A Convenient Set of Comoving Cosmological Variables and Their Application
arXiv:astro-ph/9710119 · doi:10.1046/j.1365-8711.1998.01497.x
Abstract
We present a set of cosmological variables, called "supercomoving variables," which are particularly useful for describing the gas dynamics of cosmic structure formation. For ideal gas with gamma=5/3, the supercomoving position, velocity, density, temperature, and pressure are constant in time in a uniform, isotropic, adiabatically expanding universe. Expressed in terms of these supercomoving variables, the cosmological fluid conservation equations and the Poisson equation closely resemble their noncosmological counterparts. This makes it possible to generalize noncosmological results and techniques to cosmological problems, for a wide range of cosmological models. These variables were initially introduced by Shandarin for matter-dominated models only. We generalize supercomoving variables to models with a uniform component corresponding to a nonzero cosmological constant, domain walls, cosmic strings, a nonclumping form of nonrelativistic matter (e.g. massive nettrinos), or radiation. Each model is characterized by the value of the density parameter Omega0 of the nonrelativistic matter component in which density fluctuation is possible, and the density parameter OmegaX of the additional, nonclumping component. For each type of nonclumping background, we identify FAMILIES within which different values of Omega0 and OmegaX lead to fluid equations and solutions in supercomoving variables which are independent of Omega0 and OmegaX. We also include the effects of heating, radiative cooling, thermal conduction, viscosity, and magnetic fields. As an illustration, we describe 3 familiar cosmological problems in supercomoving variables: the growth of linear density fluctuations, the nonlinear collapse of a 1D plane-wave density fluctuation leading to pancake formation, and the Zel'dovich approximation.
38 pages (AAS latex) + 2 figures (postscript) combined in one gzip-ed tar file. Identical to original posted version, except for addition of 2 references. Monthly Notices of the R.A.S., in press
Cited by in corpus (60)
- Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
- RAMSES-RT: Radiation hydrodynamics in the cosmological context
- Constrained Simulations of the Real Universe: II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region
- ECOSMOG: An Efficient Code for Simulating Modified Gravity
- Large-scale dark matter simulations
- Nonlinear structure formation in the Cubic Galileon gravity model
- ISIS: a new N-body cosmological code with scalar fields based on RAMSES. Code presentation and application to the shapes of clusters
- Exploring Vainshtein mechanism on adaptively refined meshes
- Systematic simulations of modified gravity: symmetron and dilaton models
- Simulating the quartic Galileon gravity model on adaptively refined meshes
- Numerical Studies of Diffusive Shock Acceleration at Spherical Shocks
- The Postcollapse Equilibrium Structure of Cosmological Haloes in a Low-Density Universe
- Cosmological simulations of screened modified gravity out of the static approximation: effects on matter distribution
- Implementing the DC Mode in Cosmological Simulations with Supercomoving Variables
- Systematic simulations of modified gravity: chameleon models
- The impact of baryon physics on the structure of high-redshift galaxies
- A three-phase amplification of the cosmic magnetic field in galaxies
- ColDICE: a parallel Vlasov-Poisson solver using moving adaptive simplicial tessellation
- How primordial magnetic fields shrink galaxies
- Speeding up -body simulations of modified gravity: Chameleon screening models
- EMMA: an AMR cosmological simulation code with radiative transfer
- A small-scale dynamo in feedback-dominated galaxies - III. Cosmological simulations
- Simulation of the growth of the 3D Rayleigh-Taylor instability in Supernova Remnants using an expanding reference frame
- Post-collapse perturbation theory in 1D cosmology -- beyond shell-crossing
- GRAMSES: a new route to general relativistic -body simulations in cosmology. Part I. Methodology and code description
- Hydrodynamic Effects in the Symmetron and -gravity Models
- Phase-space structure of protohalos: Vlasov versus Particle-Mesh
- The Cosmological Simulation Code OpenGadget3 -- Implementation of Meshless Finite Mass
- Halo Formation from Yukawa Forces in the Very Early Universe
- The velocity field in MOND cosmology
- Cosmological simulations with disformally coupled symmetron fields
- Cosmological Magnetogenesis: The Biermann Battery during the Epoch of Reionization
- Explosion Implosion Duality and the Laboratory Simulation of Astrophysical Systems
- Mass-Temperature relation in CDM and modified gravity
- Simulation techniques for modified gravity
- Effects of Photoionization and Photoheating on Lyman-alpha Forest Properties from Cholla Cosmological Simulations
- Hydrodynamical structure formation in Milgromian cosmology
- Filaments and sheets of the warm-hot intergalactic medium
- Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
- Tidal disruption of star clusters in galaxy formation simulations
- Investigating the influence of magnetic fields upon structure formation with AMIGA - a C code for cosmological magnetohydrodynamics
- Cosmological simulations with hydrodynamics of screened scalar-tensor gravity with non-universal coupling
- A detailed view of filaments and sheets in the warm-hot intergalactic medium. I. Pancake formation
- SCALAR: an AMR code to simulate axion-like dark matter models
- Structure formation in a Dirac-Milne universe: comparison with the standard cosmological model
- Parameter study of decaying magnetohydrodynamic turbulence
- Halo formation and evolution in scalar field dark matter and cold dark matter: New insights from the fluid approach
- Proca-stinated Cosmology I: A N-body code for the vector Galileon
- Perturbation-theory informed integrators for cosmological simulations
- Spherical accretion of collisional gas in modified gravity I: self-similar solutions and a new cosmological hydrodynamical code
- Collapse of spherical overdensities in superfluid models of dark matter
- Fuzzy dark matter simulations
- Magnetic field amplification during a turbulent collapse
- Non-linear Phenomenology of Disformally Coupled Quintessence
- PySCo: A fast Particle-Mesh -body code for modified gravity simulations in Python
- Non-linear structure formation with elastic interactions in the dark sector
- The effects on structure of a momentum coupling between dark matter and quintessence
- A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
- Hydromagnetic waves in an expanding universe -- cosmological MHD code tests using analytic solutions
- Post-collapse Lagrangian perturbation theory in three dimensions