The DOI matches its Crossref record; 38 of the 38 references it cites were found in a registry or an index.
Multi-scale initial conditions for cosmological simulations
Open accessAbstract
We discuss a new algorithm to generate multi-scale initial conditions with multiple levels of refinements for cosmological ‘zoom-in’ simulations. The method uses an adaptive convolution of Gaussian white noise with a real-space transfer function kernel together with an adaptive multi-grid Poisson solver to generate displacements and velocities following first- (1LPT) or second-order Lagrangian perturbation theory (2LPT). The new algorithm achieves rms relative errors of the order of 10−4 for displacements and velocities in the refinement region and thus improves in terms of errors by about two orders of magnitude over previous approaches. In addition, errors are localized at coarse-fine boundaries and do not suffer from Fourier-space-induced interference ringing. An optional hybrid multi-grid and Fast Fourier Transform (FFT) based scheme is introduced which has identical Fourier-space behaviour as traditional approaches. Using a suite of re-simulations of a galaxy cluster halo our real-space-based approach is found to reproduce correlation functions, density profiles, key halo properties and subhalo abundances with per cent level accuracy. Finally, we generalize our approach for two-component baryon and dark-matter simulations and demonstrate that the power spectrum evolution is in excellent agreement with linear perturbation theory. For initial baryon density fields, it is suggested to use the local Lagrangian approximation in order to generate a density field for mesh-based codes that is consistent with the Lagrangian perturbation theory instead of the current practice of using the Eulerian linearly scaled densities.
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Cites
The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
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The evolution of large-scale structure in a universe dominated by cold dark matter
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Baryonic Features in the Matter Transfer Function
Eisenstein, D. J., & Hu, W. (1998) · The Astrophysical Journal · doi:10.1086/305424 · Cited by 2,239
Cosmological hydrodynamics with adaptive mesh refinement: A new high resolution code called RAMSES
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Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
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Cited by
First results from the IllustrisTNG simulations: radio haloes and magnetic fields
Marinacci, F., Vogelsberger, M., Pakmor, R., Torrey, P., Springel, V., Hernquist, L., Nelson, D., Weinberger, R., Pillepich, A., Naiman, J., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2206 · Cited by 1,084
Wetzel, A. R., Hopkins, P. F., Kim, J.-H., Faucher-Giguère, C.-A., Kereš, D., & Quataert, E. (2016) · The Astrophysical Journal Letters · doi:10.3847/2041-8205/827/2/l23 · Cited by 623
Angulo, R. E., Springel, V., White, S. D. M., Jenkins, A., Baugh, C. M., & Frenk, C. S. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21830.x · Cited by 490
emerge – an empirical model for the formation of galaxies since z ∼ 10
Moster, B. P., Naab, T., & White, S. D. M. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty655 · Cited by 423
Core formation in dwarf haloes with self-interacting dark matter: no fine-tuning necessary
Elbert, O. D., Bullock, J. S., Garrison-Kimmel, S., Rocha, M., Oñorbe, J., & Peter, A. H. G. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1470 · Cited by 306
Metadata
- Authors
- Hahn, O., & Abel, T.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2011-07-18
- Volume
- 415
- Issue
- 3
- Pages
- 2101-2121
- ISSN
- 0035-8711 (ISSN-L)
- OpenAlex
- W1826719611
- Cited by
- 834
- References
- 38
- FWCI
- 7.09
- Type
- journal article
- Language
- en
- Open access
- hybrid
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