The Coyote Universe. I. Precision Determination of the Nonlinear Matter Power Spectrum
Near-future cosmological observations targeted at investigations of dark energy pose stringent requirements on the accuracy of theoretical predictions for the nonlinear clustering of matter. Currently, N-body simulations comprise the only viable approach to this problem. In this paper, we study vari...
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| Published in | The Astrophysical journal Vol. 715; no. 1; pp. 104 - 121 |
|---|---|
| Main Authors | , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Bristol
IOP Publishing
20.05.2010
IOP |
| Subjects | |
| Online Access | Get full text |
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| Abstract | Near-future cosmological observations targeted at investigations of dark energy pose stringent requirements on the accuracy of theoretical predictions for the nonlinear clustering of matter. Currently, N-body simulations comprise the only viable approach to this problem. In this paper, we study various sources of computational error and methods to control them. By applying our methodology to a large suite of cosmological simulations we show that results for the (gravity-only) nonlinear matter power spectrum can be obtained at 1% accuracy out to k {approx} 1 h Mpc{sup -1}. The key components of these high accuracy simulations are precise initial conditions, very large simulation volumes, sufficient mass resolution, and accurate time stepping. This paper is the first in a series of three; the final aim is a high-accuracy prediction scheme for the nonlinear matter power spectrum that improves current fitting formulae by an order of magnitude. |
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| AbstractList | Near-future cosmological observations targeted at investigations of dark energy pose stringent requirements on the accuracy of theoretical predictions for the nonlinear clustering of matter. Currently, N-body simulations comprise the only viable approach to this problem. In this paper, we study various sources of computational error and methods to control them. By applying our methodology to a large suite of cosmological simulations we show that results for the (gravity-only) nonlinear matter power spectrum can be obtained at 1% accuracy out to k {approx} 1 h Mpc{sup -1}. The key components of these high accuracy simulations are precise initial conditions, very large simulation volumes, sufficient mass resolution, and accurate time stepping. This paper is the first in a series of three; the final aim is a high-accuracy prediction scheme for the nonlinear matter power spectrum that improves current fitting formulae by an order of magnitude. |
| Author | Wagner, Christian Higdon, David Heitmann, Katrin White, Martin Habib, Salman |
| Author_xml | – sequence: 1 fullname: Heitmann, Katrin – sequence: 2 fullname: White, Martin – sequence: 3 fullname: Wagner, Christian – sequence: 4 fullname: Habib, Salman – sequence: 5 fullname: Higdon, David |
| BackLink | http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=22806852$$DView record in Pascal Francis https://www.osti.gov/biblio/21448764$$D View this record in Osti.gov |
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| Cites_doi | 10.1046/j.1365-8711.1998.01845.x 10.1088/0067-0049/180/2/306 10.1109/MCG.2008.101 10.1086/313015 10.1051/0004-6361:20078522 10.1051/0004-6361/200811247 10.1146/annurev.aa.30.090192.002435 10.1088/1749-4699/1/1/015003 10.1086/176904 10.1103/PhysRevD.57.3290 10.1086/507781 10.1088/0004-637X/705/1/156 10.1111/j.1365-2966.2005.09655.x 10.1103/PhysRevD.80.043531 10.1093/pasj/61.2.321 10.1111/j.1365-2966.2008.14176.x 10.1109/PACIFICVIS.2008.4475478 10.1086/506448 10.1086/426712 10.1016/j.astropartphys.2005.02.006 10.1046/j.1365-8711.2003.06503.x 10.1086/503418 10.1086/523083 10.1103/PhysRevD.75.063512 10.1111/j.1365-2966.2008.14290.x 10.1086/519440 10.1111/j.1365-2966.2008.13092.x 10.1111/j.1365-2966.2008.13731.x 10.1086/516599 10.1103/PhysRevD.68.083507 10.1016/S0370-1573(02)00135-7 10.1111/j.1365-2966.2006.11040.x 10.1016/S0370-1573(02)00276-4 10.1103/PhysRevD.76.083503 10.1111/j.1365-2966.2007.12202.x 10.1086/342752 10.1086/432646 10.1051/0004-6361/200811054 10.1103/PhysRevD.77.043525 10.1088/0004-637X/713/2/1322 10.1103/PhysRevD.56.596 10.1093/mnras/280.3.L19 10.1103/PhysRevD.78.063529 10.1086/503547 10.1086/186057 10.1086/523836 10.1016/j.astropartphys.2004.06.001 |
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| References | 44 45 46 47 49 Bouchet (4) 1995; 296 Lawrence (33) 2010; 713 Zel'dovich (54) 1970; 5 Baugh (1) 1995; 274 51 52 53 11 14 Heitmann (18) 2006; 646 15 16 Dunkley (10) 2009; 180 17 Guillet (13) 2009 White (50) 2002; 143 Jarvis (27) 2006; 644 2 3 5 6 7 8 9 Peacock (39) 1996; 280 22 Peacock (38) 1999 24 25 26 Heitmann (20) 2005; 160 Massey (36) 2007; 172 Jing (29) 2006; 640 Lukić (34) 2007; 671 Heitmann (21) 2008; 1 Göttlober (12) 2008 Kravtsov (32) 1997; 111 Ma (35) 2007; 665 30 31 Tang (48) 2008 Hockney (23) 1989 Nishimichi (37) 2009; 61 Jeong (28) 2006; 651 Rudd (40) 2008; 672 Zhan (55) 2004; 616 Heitmann (19) 2009; 705 41 42 43 |
| References_xml | – ident: 42 doi: 10.1046/j.1365-8711.1998.01845.x – volume: 180 start-page: 306 issn: 0067-0049 year: 2009 ident: 10 publication-title: ApJS doi: 10.1088/0067-0049/180/2/306 – ident: 16 doi: 10.1109/MCG.2008.101 – start-page: 29 year: 2008 ident: 12 publication-title: High Performance Computing in Science and Engineering Garching/Munich 2007 – volume: 111 start-page: 73 issn: 0067-0049 year: 1997 ident: 32 publication-title: ApJS doi: 10.1086/313015 – ident: 11 doi: 10.1051/0004-6361:20078522 – ident: 31 doi: 10.1051/0004-6361/200811247 – ident: 6 doi: 10.1146/annurev.aa.30.090192.002435 – volume: 1 start-page: 015003 issn: 1749-4699 year: 2008 ident: 21 publication-title: Comput. Sci. Discovery doi: 10.1088/1749-4699/1/1/015003 – ident: 52 doi: 10.1086/176904 – year: 1999 ident: 38 publication-title: Cosmological Physics – ident: 24 doi: 10.1103/PhysRevD.57.3290 – volume: 651 start-page: 619 issn: 0004-637X year: 2006 ident: 28 publication-title: ApJ doi: 10.1086/507781 – volume: 705 start-page: 156 issn: 0004-637X year: 2009 ident: 19 publication-title: ApJ doi: 10.1088/0004-637X/705/1/156 – ident: 47 doi: 10.1111/j.1365-2966.2005.09655.x – ident: 5 doi: 10.1103/PhysRevD.80.043531 – volume: 61 start-page: 321 issn: 0004-6264 year: 2009 ident: 37 publication-title: PASJ doi: 10.1093/pasj/61.2.321 – ident: 7 doi: 10.1111/j.1365-2966.2008.14176.x – ident: 17 doi: 10.1109/PACIFICVIS.2008.4475478 – volume: 646 start-page: L1 issn: 1538-4357 year: 2006 ident: 18 publication-title: ApJ doi: 10.1086/506448 – volume: 616 start-page: L75 issn: 1538-4357 year: 2004 ident: 55 publication-title: ApJ doi: 10.1086/426712 – ident: 26 doi: 10.1016/j.astropartphys.2005.02.006 – ident: 46 doi: 10.1046/j.1365-8711.2003.06503.x – volume: 644 start-page: 71 issn: 0004-637X year: 2006 ident: 27 publication-title: ApJ doi: 10.1086/503418 – volume: 671 start-page: 1160 issn: 0004-637X year: 2007 ident: 34 publication-title: ApJ doi: 10.1086/523083 – ident: 44 doi: 10.1103/PhysRevD.75.063512 – ident: 30 doi: 10.1111/j.1365-2966.2008.14290.x – volume: 665 start-page: 887 issn: 0004-637X year: 2007 ident: 35 publication-title: ApJ doi: 10.1086/519440 – ident: 53 doi: 10.1111/j.1365-2966.2008.13092.x – volume: 296 start-page: 575 issn: 0004-6361 year: 1995 ident: 4 publication-title: A&A – ident: 49 doi: 10.1111/j.1365-2966.2008.13731.x – year: 1989 ident: 23 publication-title: Computer Simulation Using Particles – volume: 172 start-page: 239 issn: 0067-0049 year: 2007 ident: 36 publication-title: ApJS doi: 10.1086/516599 – volume: 5 start-page: 84 issn: 0004-6361 year: 1970 ident: 54 publication-title: A&A – ident: 43 doi: 10.1103/PhysRevD.68.083507 – ident: 3 doi: 10.1016/S0370-1573(02)00135-7 – ident: 9 doi: 10.1111/j.1365-2966.2006.11040.x – ident: 8 doi: 10.1016/S0370-1573(02)00276-4 – ident: 14 doi: 10.1103/PhysRevD.76.083503 – ident: 2 doi: 10.1111/j.1365-2966.2007.12202.x – volume: 143 start-page: 241 issn: 0067-0049 year: 2002 ident: 50 publication-title: ApJS doi: 10.1086/342752 – volume: 160 start-page: 28 issn: 0067-0049 year: 2005 ident: 20 publication-title: ApJS doi: 10.1086/432646 – ident: 22 doi: 10.1051/0004-6361/200811054 – ident: 45 doi: 10.1103/PhysRevD.77.043525 – volume: 713 start-page: 1322 issn: 0004-637X year: 2010 ident: 33 publication-title: ApJ doi: 10.1088/0004-637X/713/2/1322 – ident: 25 doi: 10.1103/PhysRevD.56.596 – volume: 274 start-page: 1049 issn: 0035-8711 year: 1995 ident: 1 publication-title: MNRAS – volume: 280 start-page: L19 issn: 0035-8711 year: 1996 ident: 39 publication-title: MNRAS doi: 10.1093/mnras/280.3.L19 – ident: 41 doi: 10.1103/PhysRevD.78.063529 – year: 2008 ident: 48 – issn: 0004-6361 year: 2009 ident: 13 publication-title: A&A – volume: 640 start-page: L119 issn: 1538-4357 year: 2006 ident: 29 publication-title: ApJ doi: 10.1086/503547 – ident: 15 doi: 10.1086/186057 – volume: 672 start-page: 19 issn: 0004-637X year: 2008 ident: 40 publication-title: ApJ doi: 10.1086/523836 – ident: 51 doi: 10.1016/j.astropartphys.2004.06.001 |
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| Snippet | Near-future cosmological observations targeted at investigations of dark energy pose stringent requirements on the accuracy of theoretical predictions for the... |
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| SubjectTerms | Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Earth, ocean, space Exact sciences and technology GRAVITATION MASS RESOLUTION MATTER NONLINEAR PROBLEMS NONLUMINOUS MATTER RESOLUTION UNIVERSE |
| Title | The Coyote Universe. I. Precision Determination of the Nonlinear Matter Power Spectrum |
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