Fetching the paper…
Reading the bibliography…
We review the field of collisionless numerical simulations for the large-scale structure of the Universe.
1901
Earlier work this paper cites.
1901
Earlier work this paper cites.
1901
Earlier work this paper cites.
1901
Earlier work this paper cites.
1902
Earlier work this paper cites.
1902
Earlier work this paper cites.
1902
Earlier work this paper cites.
1903
Earlier work this paper cites.
1903
Earlier work this paper cites.
1903
Earlier work this paper cites.
1903
Earlier work this paper cites.
1903
Earlier work this paper cites.
1903
Earlier work this paper cites.
1904
Earlier work this paper cites.
1904
Earlier work this paper cites.
1904
Earlier work this paper cites.
1904
Earlier work this paper cites.
1904
Earlier work this paper cites.
1904
Earlier work this paper cites.
1904
Earlier work this paper cites.
1904
Earlier work this paper cites.
1905
Earlier work this paper cites.
1905
Earlier work this paper cites.
1905
Earlier work this paper cites.
1905
Earlier work this paper cites.
1905
Earlier work this paper cites.
1905
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1908
Earlier work this paper cites.
1908
Earlier work this paper cites.
1908
Earlier work this paper cites.
1908
Earlier work this paper cites.
1908
Earlier work this paper cites.
1909
Earlier work this paper cites.
1909
Earlier work this paper cites.
1909
Earlier work this paper cites.
1909
Earlier work this paper cites.
1909
Earlier work this paper cites.
1909
Earlier work this paper cites.
1910
Earlier work this paper cites.
1910
Earlier work this paper cites.
1910
Earlier work this paper cites.
1910
Earlier work this paper cites.
1910
Earlier work this paper cites.
1910
Earlier work this paper cites.
1910
Earlier work this paper cites.
1910
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1911
Earlier work this paper cites.
1912
Earlier work this paper cites.
1912
Earlier work this paper cites.
1912
Earlier work this paper cites.
1912
Earlier work this paper cites.
1912
Earlier work this paper cites.
Ewald PP (1921) Die Berechnung optischer und elektrostatischer Gitterpotentiale. Annalen der Physik 369(3):253–287. https://doi.org/10.1002/andp.19213690304
1921
Earlier work this paper cites.
Madelung E (1927) Quantentheorie in hydrodynamischer Form. Zeitschrift fur Physik 40:322–326. https://doi.org/10.1007/BF01400372
1927
Earlier work this paper cites.
1940
Earlier work this paper cites.
1943
Earlier work this paper cites.
Magnus W (1954) On the exponential solution of differential equations for a linear operator. Communications on Pure and Applied Mathematics 7(4):649–673. https://doi.org/10.1002/cpa.3160070404
1954
Earlier work this paper cites.
1957
Earlier work this paper cites.
von Hoerner S (1960) Die numerische Integration des n-Körper-Problemes für Sternhaufen. I. ZAp50
1960
Earlier work this paper cites.
1961
Earlier work this paper cites.
Aarseth SJ (1963) Dynamical evolution of clusters of galaxies, I. MNRAS126:223. https://doi.org/10.1093/mnras/126.3.223
1963
Earlier work this paper cites.
Hénon M (1964) L’évolution initiale d’un amas sphérique. Annales d’Astrophysique 27:83
1964
Earlier work this paper cites.
Hayli A (1967) Le problème des N corps dans un champ extérieur. Application à l’évolution dynamique des amas ouverts. I. In: Les Nouvelles Méthodes de la Dynamique Stellaire. p 67
1967
Earlier work this paper cites.
Miller RH, Prendergast KH (1968) Stellar Dynamics in a Discrete Phase Space. ApJ151:699. https://doi.org/10.1086/149469
1968
Earlier work this paper cites.
Zel’dovich YB (1970) Gravitational instability: An approximate theory for large density perturbations. A&A5:84–89
1970
Earlier work this paper cites.
Choquet-Bruhat Y (1971) Problème de cauchy pour le système intégro-différentiel d’einstein-liouville. Annales de l’Institut Fourier 21(3):181–201. https://doi.org/10.5802/aif.385 , URL http://www.numdam.org/articles/10.5802/aif.385/
1971
Earlier work this paper cites.
Ehlers J (1971) Problème de Cauchy pour le système intégro-différentiel d’Einstein-Liouville. (Cauchy problem for the Einstein-Liouville integro-differential system). In: General Relativity and Cosmology. vol 21. Université Joseph Fourier, Grenoble; Association des Annales de l’Institut Fourier, Saint-Martin d’Hères
1971
Earlier work this paper cites.
Orszag SA (1971) On the Elimination of Aliasing in Finite-Difference Schemes by Filtering High-Wavenumber Components. J Atmosph Sci 28:1074–1074. https://doi.org/10.1175/1520-0469(1971)028<1074:OTEOAI>2.0.CO;2
1971
Earlier work this paper cites.
Peebles PJE (1971) Rotation of Galaxies and the Gravitational Instability Picture. A&A11:377
1971
Earlier work this paper cites.
Vainshtein AI (1972) To the problem of nonvanishing gravitation mass. Phys Lett B 39:393–394. https://doi.org/10.1016/0370-2693(72)90147-5
1972
Earlier work this paper cites.
Doroshkevich AG, Ryaben’kii VS, Shandarin SF (1973) Nonlinear theory of the development of potential perturbations. Astrophysics 9:144–153. https://doi.org/10.1007/BF01011421
1973
Earlier work this paper cites.
Misner C, Thorne K, Wheeler J (1973) Gravitation. W. H. Freeman
1973
Earlier work this paper cites.
Chen L, Bruce Langdon A, Birdsall CK (1974) Reduction of the Grid Effects in Simulation Plasmas. J Comput Phys 14(2):200–222. https://doi.org/10.1016/0021-9991(74)90014-X
1974
Earlier work this paper cites.
Hayli A (1974) The method of the doubly individual step for N-body computations. In: Numerical Solution of Ordinary Differential Equations. pp 304–312
1974
Earlier work this paper cites.
Press WH, Schechter P (1974) Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation. ApJ187:425–438. https://doi.org/10.1086/152650
1974
Earlier work this paper cites.
1975
Earlier work this paper cites.
Miyoshi K, Kihara T (1975) Development of the correlation of galaxies in an expanding universe. PASJ27:333–346
1975
Earlier work this paper cites.
Brandt A (1977) Multi-level adaptive solutions to boundary-value problems. Mathematics of Computation 31(138):333–390
1977
Earlier work this paper cites.
White SDM, Rees MJ (1978) Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering. MNRAS183:341–358. https://doi.org/10.1093/mnras/183.3.341
1978
Earlier work this paper cites.
Tremaine S, Gunn JE (1979) Dynamical role of light neutral leptons in cosmology. Phys. Rev. Lett.42(6):407–410. https://doi.org/10.1103/PhysRevLett.42.407
1979
Earlier work this paper cites.
Doroshkevich AG, Kotok EV, Poliudov AN, Shandarin SF, Sigov IS, Novikov ID (1980) Two-dimensional simulation of the gravitational system dynamics and formation of the large-scale structure of the universe. MNRAS192:321–337. https://doi.org/10.1093/mnras/192.2.321
1980
Earlier work this paper cites.
Peebles PJE (1980) The large-scale structure of the universe. Princeton University Press, Princeton, N.J
1980
Earlier work this paper cites.
Fujiwara T (1981) Vlasov Simulations of Stellar Systems - Infinite Homogeneous Case. PASJ33:531
1981
Earlier work this paper cites.
Hockney RW, Eastwood JW (1981) Computer Simulation Using Particles. Computer Simulation Using Particles, New York: McGraw-Hill, 1981
1981
Earlier work this paper cites.
Press WH, Davis M (1982) How to identify and weigh virialized clusters of galaxies in a complete redshift catalog. ApJ259:449–473. https://doi.org/10.1086/160183
1982
Earlier work this paper cites.
Centrella J, Melott AL (1983) Three-dimensional simulation of large-scale structure in the universe. Nature305:196–198. https://doi.org/10.1038/305196a0
1983
Earlier work this paper cites.
Klypin AA, Shandarin SF (1983) Three-dimensional numerical model of the formation of large-scale structure in the Universe. MNRAS204:891–907. https://doi.org/10.1093/mnras/204.3.891
1983
Earlier work this paper cites.
Miller RH (1983) Numerical experiments on the clustering of galaxies. ApJ270:390–409. https://doi.org/10.1086/161133
1983
Earlier work this paper cites.
Shapiro PR, Struck-Marcell C, Melott AL (1983) Pancakes and the formation of galaxies in a neutrino-dominated universe. ApJ275:413–429. https://doi.org/10.1086/161543
1983
Earlier work this paper cites.
White SDM, Frenk CS, Davis M (1983) Clustering in a neutrino-dominated universe. ApJ274:L1–L5. https://doi.org/10.1086/184139
1983
Earlier work this paper cites.
Taha TR, Ablowitz MI (1984) Analytical and numerical aspects of certain nonlinear evolution equations. ii. numerical, nonlinear schrödinger equation. Journal of Computational Physics 55(2):203–230. https://doi.org/https://doi.org/10.1016/0021-9991(84)90003-2 , URL https://www.sciencedirect.com/science/article/pii/0021999184900032
1984
Earlier work this paper cites.
Appel AW (1985) An Efficient Program for Many-Body Simulation. SIAM J Sci Statist Computing 6(1):85–103
1985
Earlier work this paper cites.
Bertschinger E (1985) Self-similar secondary infall and accretion in an Einstein-de Sitter universe. ApJS58:39–65. https://doi.org/10.1086/191028
1985
Earlier work this paper cites.
Davis M, Efstathiou G, Frenk CS, White SDM (1985) The evolution of large-scale structure in a universe dominated by cold dark matter. ApJ292:371–394. https://doi.org/10.1086/163168
1985
Earlier work this paper cites.
Gurbatov SN, Saichev AI, Shandarin SF (1985) A model for describing the development of the large-scale structure of the universe. Soviet Physics Doklady 20:921
1985
Earlier work this paper cites.
Barnes J, Hut P (1986) A hierarchical O(N log N) force-calculation algorithm. Nature324(6096):446–449. https://doi.org/10.1038/324446a0
1986
Earlier work this paper cites.
Goroff MH, Grinstein B, Rey SJ, Wise MB (1986) Coupling of modes of cosmological mass density fluctuations. ApJ311:6–14. https://doi.org/10.1086/164749
1986
Earlier work this paper cites.
Lanczos C (1986) The Variational Principles of Mechanics. Dover Books On Physics, Dover Publications
1986
Earlier work this paper cites.
McMillan SLW (1986) The Vectorization of Small-N Integrators. In: Hut P, McMillan SLW (eds) The Use of Supercomputers in Stellar Dynamics. Lecture Notes in Physics, vol 267. Springer, Berlin, Heidelberg, p 156. https://doi.org/10.1007/BFb0116406
1986
Earlier work this paper cites.
Greengard L, Rokhlin V (1987) A fast algorithm for particle simulations. J Comput Phys 73(2):325 – 348. https://doi.org/10.1016/0021-9991(87)90140-9
1987
Earlier work this paper cites.
Bouchet FR, Hernquist L (1988) Cosmological Simulations Using the Hierarchical Tree Method. ApJS68:521. https://doi.org/10.1086/191299
1988
Earlier work this paper cites.
Centrella JM, Gallagher JS III, Melott AL, Bushouse HA (1988) A case study of large-scale structure in a ’hot’ model universe. ApJ333:24–53. https://doi.org/10.1086/166722
1988
Earlier work this paper cites.
Kofman LA, Shandarin SF (1988) Theory of adhesion for the large-scale structure of the Universe. Nature334(6178):129–131. https://doi.org/10.1038/334129a0
1988
Earlier work this paper cites.
Buchert T (1989) A class of solutions in Newtonian cosmology and the pancake theory. A&A223:9–24
1989
Earlier work this paper cites.
Peebles PJE, Melott AL, Holmes MR, Jiang LR (1989) A model for the formation of the Local Group. ApJ345:108–121. https://doi.org/10.1086/167885
1989
Earlier work this paper cites.
Hernquist L, Barnes JE (1990) Are Some N-Body Algorithms Intrinsically Less Collisional than Others? ApJ349:562. https://doi.org/10.1086/168343
1990
Earlier work this paper cites.
Press WH, Ryden BS, Spergel DN (1990) Single mechanism for generating large-scale structure and providing dark missing matter. Physical Review Letters 64:1084–1087. https://doi.org/10.1103/PhysRevLett.64.1084
1990
Earlier work this paper cites.
Yoshida H (1990) Construction of higher order symplectic integrators. Phys Lett A 150:262–268. https://doi.org/10.1016/0375-9601(90)90092-3
1990
Earlier work this paper cites.
Coles P, Jones B (1991) A lognormal model for the cosmological mass distribution. MNRAS248:1–13. https://doi.org/10.1093/mnras/248.1.1
1991
Earlier work this paper cites.
Heggie DC (1991) Chaos in the N-body problem of stellar dynamics. In: Predictability, Stability, and Chaos in N-Body Dynamical Systems. NATO Advanced Study Institute (ASI) Series B, vol 272. pp 47–62
1991
Earlier work this paper cites.
Hoffman Y, Ribak E (1991) Constrained Realizations of Gaussian Fields: A Simple Algorithm. ApJ380:L5. https://doi.org/10.1086/186160
1991
Earlier work this paper cites.
Oteo JA, Ros J (1991) The Magnus expansion for classical Hamiltonian systems. J Phys A 24:5751–5762. https://doi.org/10.1088/0305-4470/24/24/011
1991
Earlier work this paper cites.
White SDM, Frenk CS (1991) Galaxy Formation through Hierarchical Clustering. ApJ379:52. https://doi.org/10.1086/170483
1991
Earlier work this paper cites.
Earn DJD, Tremaine S (1992) Exact numerical studies of Hamiltonian maps: Iterating without roundoff error. Physica D Nonlinear Phenomena 56(1):1–22. https://doi.org/10.1016/0167-2789(92)90047-Q
1992
Earlier work this paper cites.
Kofman L, Pogosyan D, Shandarin SF, Melott AL (1992) Coherent Structures in the Universe and the Adhesion Model. ApJ393:437. https://doi.org/10.1086/171517
1992
Earlier work this paper cites.
1993
Earlier work this paper cites.
Goodman J, Heggie DC, Hut P (1993) On the Exponential Instability of N-Body Systems. ApJ415:715. https://doi.org/10.1086/173196
1993
Earlier work this paper cites.
Kauffmann G, White SDM, Guiderdoni B (1993) The formation and evolution of galaxies within merging dark matter haloes. MNRAS264:201–218. https://doi.org/10.1093/mnras/264.1.201
1993
Earlier work this paper cites.
Klypin A, Holtzman J, Primack J, Regos E (1993) Structure Formation with Cold plus Hot Dark Matter. ApJ416:1. https://doi.org/10.1086/173210 . arXiv:astro-ph/9305011 [astro-ph]
1993
Earlier work this paper cites.
Laskar J (1993) Frequency analysis for multi-dimensional systems. Global dynamics and diffusion. Physica D Nonlinear Phenomena 67:257–281. https://doi.org/10.1016/0167-2789(93)90210-R
1993
Earlier work this paper cites.
Widrow LM, Kaiser N (1993) Using the Schrödinger Equation to Simulate Collisionless Matter. ApJ416:L71. https://doi.org/10.1086/187073
1993
Earlier work this paper cites.
Bernardeau F (1994) The Nonlinear Evolution of Rare Events. ApJ427:51. https://doi.org/10.1086/174121 . arXiv:astro-ph/9311066 [astro-ph]
1994
Earlier work this paper cites.
Buchert T (1994) Lagrangian Theory of Gravitational Instability of Friedman-Lemaitre Cosmologies - a Generic Third-Order Model for Nonlinear Clustering. MNRAS267:811. https://doi.org/10.1093/mnras/267.4.811 . astro-ph/9309055
1994
Earlier work this paper cites.
Cole S, Aragon-Salamanca A, Frenk CS, Navarro JF, Zepf SE (1994) A recipe for galaxy formation. MNRAS271:781–806. https://doi.org/10.1093/mnras/271.4.781 . arXiv:astro-ph/9402001 [astro-ph]
1994
Earlier work this paper cites.
Ferrell R, Bertschinger E (1994) Particle-Mesh Methods on the Connection Machine. Int J Mod Phys C 5(6):933–956. https://doi.org/10.1142/S0129183194001069 . arXiv:comp-gas/9310002 [nlin.CG]
1994
Earlier work this paper cites.
Jessop C, Duncan M, Chau WY (1994) Multigrid Methods for N-Body Gravitational Systems. J Comput Phys 115(2):339–351. https://doi.org/10.1006/jcph.1994.1200
1994
Earlier work this paper cites.
Katz N, Quinn T, Bertschinger E, Gelb JM (1994) Formation of Quasars at High Redshift. MNRAS270:L71. https://doi.org/10.1093/mnras/270.1.L71
1994
Earlier work this paper cites.
Lacey C, Cole S (1994) Merger Rates in Hierarchical Models of Galaxy Formation - Part Two - Comparison with N-Body Simulations. MNRAS271:676. https://doi.org/10.1093/mnras/271.3.676 . arXiv:astro-ph/9402069 [astro-ph]
1994
Earlier work this paper cites.
Ma CP, Bertschinger E (1994) A Calculation of the Full Neutrino Phase Space in Cold + Hot Dark Matter Models. ApJ429:22. https://doi.org/10.1086/174298 . arXiv:astro-ph/9308006 [astro-ph]
1994
Earlier work this paper cites.
Munshi D, Sahni V, Starobinsky AA (1994) Nonlinear approximations to gravitational instability: A comparison in the quasi-linear regime. ApJ436:517–527. https://doi.org/10.1086/174925 . astro-ph/9402065
1994
Earlier work this paper cites.
van de Weygaert R (1994) Fragmenting the Universe. 3: The constructions and statistics of 3-D Voronoi tessellations. A&A283(2):361–406
1994
Earlier work this paper cites.
White SDM (1994) Formation and Evolution of Galaxies: Les Houches Lectures. arXiv e-prints astro-ph/9410043. arXiv:astro-ph/9410043 [astro-ph]
1994
Earlier work this paper cites.
Bouchet FR, Colombi S, Hivon E, Juszkiewicz R (1995) Perturbative Lagrangian approach to gravitational instability. A&A296:575. astro-ph/9406013
1995
Earlier work this paper cites.
Catelan P (1995) Lagrangian dynamics in non-flat universes and non-linear gravitational evolution. MNRAS276:115–124. https://doi.org/10.1093/mnras/276.1.115 . astro-ph/9406016
1995
Earlier work this paper cites.
Habib S, Ryne RD (1995) Symplectic Calculation of Lyapunov Exponents. Phys. Rev. Lett.74(1):70–73. https://doi.org/10.1103/PhysRevLett.74.70 . arXiv:chao-dyn/9406010 [nlin.CD]
1995
Earlier work this paper cites.
Suisalu I, Saar E (1995) An adaptive multigrid solver for high-resolution cosmological simulations. MNRAS274(1):287–299. https://doi.org/10.1093/mnras/274.1.287 . arXiv:astro-ph/9412043 [astro-ph]
1995
Earlier work this paper cites.
Bond JR, Kofman L, Pogosyan D (1996) How filaments of galaxies are woven into the cosmic web. Nature380(6575):603–606. https://doi.org/10.1038/380603a0 . arXiv:astro-ph/9512141 [astro-ph]
1996
Earlier work this paper cites.
Kolb EW, Tkachev II (1996) Femtolensing and Picolensing by Axion Miniclusters. ApJ460:L25. https://doi.org/10.1086/309962 . arXiv:astro-ph/9510043 [astro-ph]
1996
Earlier work this paper cites.
Moore B, Katz N, Lake G (1996) On the Destruction and Overmerging of Dark Halos in Dissipationless N-Body Simulations. ApJ457:455. https://doi.org/10.1086/176745 . arXiv:astro-ph/9503088 [astro-ph]
1996
Earlier work this paper cites.
Navarro JF, Eke VR, Frenk CS (1996) The cores of dwarf galaxy haloes. MNRAS283(3):L72–L78. https://doi.org/10.1093/mnras/283.3.L72 . arXiv:astro-ph/9610187 [astro-ph]
1996
Earlier work this paper cites.
van de Weygaert R, Bertschinger E (1996) Peak and gravity constraints in Gaussian primordial density fields: An application of the Hoffman-Ribak method. MNRAS281:84. https://doi.org/10.1093/mnras/281.1.84 . arXiv:astro-ph/9507024 [astro-ph]
1996
Earlier work this paper cites.
Kravtsov AV, Klypin AA, Khokhlov AM (1997) Adaptive Refinement Tree: A New High-Resolution N-Body Code for Cosmological Simulations. ApJS111(1):73–94. https://doi.org/10.1086/313015 . arXiv:astro-ph/9701195 [astro-ph]
1997
Earlier work this paper cites.
Melott AL, Shandarin SF, Splinter RaJ, Suto Y (1997) Demonstrating Discreteness and Collision Error in Cosmological N-Body Simulations of Dark Matter Gravitational Clustering. ApJ479(2):L79–L83. https://doi.org/10.1086/310590 . arXiv:astro-ph/9609152 [astro-ph]
1997
Earlier work this paper cites.
Navarro JF, Frenk CS, White SDM (1997) A Universal Density Profile from Hierarchical Clustering. ApJ490:493–508. https://doi.org/10.1086/304888 . astro-ph/9611107
1997
Earlier work this paper cites.
Pearce FR, Couchman HMP (1997) Hydra: a parallel adaptive grid code. New A2(5):411–427. https://doi.org/10.1016/S1384-1076(97)00025-0 . arXiv:astro-ph/9703183 [astro-ph]
1997
Earlier work this paper cites.
Pen UL (1997) Generating Cosmological Gaussian Random Fields. ApJ490(2):L127–L130. https://doi.org/10.1086/311042 . arXiv:astro-ph/9709261 [astro-ph]
1997
Earlier work this paper cites.
Quinn T, Katz N, Stadel J, Lake G (1997) Time stepping N-body simulations. arXiv astro-ph/9710043 astro-ph/9710043
1997
Earlier work this paper cites.
Schmalzing J, Buchert T (1997) Beyond Genus Statistics: A Unifying Approach to the Morphology of Cosmic Structure. ApJ482(1):L1–L4. https://doi.org/10.1086/310680 . arXiv:astro-ph/9702130 [astro-ph]
1997
Earlier work this paper cites.
Bryan GL, Norman ML (1998) Statistical Properties of X-Ray Clusters: Analytic and Numerical Comparisons. ApJ495(1):80–99. https://doi.org/10.1086/305262 . arXiv:astro-ph/9710107 [astro-ph]
1998
Earlier work this paper cites.
Eisenstein DJ, Hut P (1998) HOP: A New Group-Finding Algorithm for N-Body Simulations. ApJ498(1):137–142. https://doi.org/10.1086/305535 . arXiv:astro-ph/9712200 [astro-ph]
1998
Earlier work this paper cites.
Johansen H, Colella P (1998) A Cartesian Grid Embedded Boundary Method for Poisson’s Equation on Irregular Domains. J Comput Phys 147(1):60–85. https://doi.org/10.1006/jcph.1998.5965
1998
Earlier work this paper cites.
Martel H, Shapiro PR (1998) A convenient set of comoving cosmological variables and their application. MNRAS297:467–485. https://doi.org/10.1046/j.1365-8711.1998.01497.x . astro-ph/9710119
1998
Earlier work this paper cites.
Scoccimarro R (1998) Transients from initial conditions: a perturbative analysis. MNRAS299:1097–1118. https://doi.org/10.1046/j.1365-8711.1998.01845.x . astro-ph/9711187
1998
Earlier work this paper cites.
Splinter RJ, Melott AL, Shand arin SF, Suto Y (1998) Fundamental Discreteness Limitations of Cosmological N-Body Clustering Simulations. ApJ497(1):38–61. https://doi.org/10.1086/305450 . arXiv:astro-ph/9706099 [astro-ph]
1998
Earlier work this paper cites.
Syer D, White SDM (1998) Dark halo mergers and the formation of a universal profile. MNRAS293(4):337–342. https://doi.org/10.1046/j.1365-8711.1998.01285.x
1998
Earlier work this paper cites.
van de Weygaert R, Bernardeau F (1998) Velocity Fields and Tessellation Techniques: Unbiased Estimators of Omega. In: Mueller V, Gottloeber S, Muecket JP, Wambsganss J (eds) Large Scale Structure: Tracks and Traces. pp 207–216
1998
Earlier work this paper cites.
Frenk CS, White SDM, Bode P, Bond JR, Bryan GL, Cen R, Couchman HMP, Evrard AE, Gnedin N, Jenkins A, Khokhlov AM, Klypin A, Navarro JF, Norman ML, Ostriker JP, Owen JM, Pearce FR, Pen UL, Steinmetz M, Thomas PA, Villumsen JV, Wadsley JW, Warren MS, Xu G, Yepes G (1999) The Santa Barbara Cluster Comparison Project: A Comparison of Cosmological Hydrodynamics Solutions. ApJ525(2):554–582. https://doi.org/10.1086/307908 . arXiv:astro-ph/9906160 [astro-ph]
1999
Earlier work this paper cites.
Moore B, Ghigna S, Governato F, Lake G, Quinn T, Stadel J, Tozzi P (1999) Dark Matter Substructure within Galactic Halos. ApJ524(1):L19–L22. https://doi.org/10.1086/312287 . arXiv:astro-ph/9907411 [astro-ph]
1999
Earlier work this paper cites.
Pichon C, Bernardeau F (1999) Vorticity generation in large-scale structure caustics. A&A343:663–681. arXiv:astro-ph/9902142 [astro-ph]
1999
Earlier work this paper cites.
Burkert A (2000) The Structure and Evolution of Weakly Self-interacting Cold Dark Matter Halos. ApJ534(2):L143–L146. https://doi.org/10.1086/312674 . arXiv:astro-ph/0002409 [astro-ph]
2000
Earlier work this paper cites.
Cole S, Lacey CG, Baugh CM, Frenk CS (2000) Hierarchical galaxy formation. MNRAS319(1):168–204. https://doi.org/10.1046/j.1365-8711.2000.03879.x . arXiv:astro-ph/0007281 [astro-ph]
2000
Earlier work this paper cites.
Dehnen W (2000) A Very Fast and Momentum-conserving Tree Code. ApJ536(1):L39–L42. https://doi.org/10.1086/312724 . arXiv:astro-ph/0003209 [astro-ph]
2000
Earlier work this paper cites.
Dvali G, Gabadadze G, Porrati M (2000) 4D gravity on a brane in 5D Minkowski space. Phys Lett B 485(1-3):208–214. https://doi.org/10.1016/S0370-2693(00)00669-9 . arXiv:hep-th/0005016 [hep-th]
2000
Earlier work this paper cites.
Hu W, Barkana R, Gruzinov A (2000) Fuzzy Cold Dark Matter: The Wave Properties of Ultralight Particles. Phys. Rev. Lett.85(6):1158–1161. https://doi.org/10.1103/PhysRevLett.85.1158 . arXiv:astro-ph/0003365 [astro-ph]
2000
Earlier work this paper cites.
Knebe A, Kravtsov AV, Gottlöber S, Klypin AA (2000) On the effects of resolution in dissipationless cosmological simulations. MNRAS317(3):630–648. https://doi.org/10.1046/j.1365-8711.2000.03673.x . arXiv:astro-ph/9912257 [astro-ph]
2000
Earlier work this paper cites.
Kochanek CS, White M (2000) A Quantitative Study of Interacting Dark Matter in Halos. ApJ543:514–520. https://doi.org/10.1086/317149 . astro-ph/0003483
2000
Earlier work this paper cites.
Lewis A, Challinor A, Lasenby A (2000) Efficient computation of CMB anisotropies in closed FRW models. ApJ538:473–476. https://doi.org/10.1086/309179 . arXiv:astro-ph/9911177 [astro-ph]
2000
Earlier work this paper cites.
Yoshida N, Springel V, White SDM, Tormen G (2000) Weakly Self-interacting Dark Matter and the Structure of Dark Halos. ApJ544:L87–L90. https://doi.org/10.1086/317306 . astro-ph/0006134
2000
Earlier work this paper cites.
Avila-Reese V, Colín P, Valenzuela O, D’Onghia E, Firmani C (2001) Formation and Structure of Halos in a Warm Dark Matter Cosmology. ApJ559(2):516–530. https://doi.org/10.1086/322411 . arXiv:astro-ph/0010525 [astro-ph]
2001
Earlier work this paper cites.
Bertschinger E (2001) Multiscale Gaussian Random Fields and Their Application to Cosmological Simulations. ApJS137(1):1–20. https://doi.org/10.1086/322526 . arXiv:astro-ph/0103301 [astro-ph]
2001
Earlier work this paper cites.
Bode P, Ostriker JP, Turok N (2001) Halo Formation in Warm Dark Matter Models. ApJ556(1):93–107. https://doi.org/10.1086/321541 . arXiv:astro-ph/0010389 [astro-ph]
2001
Earlier work this paper cites.
Bullock JS, Kolatt TS, Sigad Y, Somerville RS, Kravtsov AV, Klypin AA, Primack JR, Dekel A (2001) Profiles of dark haloes: evolution, scatter and environment. MNRAS321(3):559–575. https://doi.org/10.1046/j.1365-8711.2001.04068.x . arXiv:astro-ph/9908159 [astro-ph]
2001
Earlier work this paper cites.
Chin SA, Chen CR (2001) Fourth order gradient symplectic integrator methods for solving the time-dependent Schrödinger equation. J. Chem. Phys.114:7338–7341. https://doi.org/10.1063/1.1362288 . physics/0012017
2001
Earlier work this paper cites.
2001
Earlier work this paper cites.
2001
Earlier work this paper cites.
Hofmann S, Schwarz DJ, Stöcker H (2001) Damping scales of neutralino cold dark matter. Phys. Rev. D64(8):083507. https://doi.org/10.1103/PhysRevD.64.083507 . arXiv:astro-ph/0104173 [astro-ph]
2001
Earlier work this paper cites.
Jenkins A, Frenk CS, White SDM, Colberg JM, Cole S, Evrard AE, Couchman HMP, Yoshida N (2001) The mass function of dark matter haloes. MNRAS321:372–384. https://doi.org/10.1046/j.1365-8711.2001.04029.x . astro-ph/0005260
2001
Earlier work this paper cites.
2001
Earlier work this paper cites.
Springel V, White SDM, Tormen G, Kauffmann G (2001a) Populating a cluster of galaxies - I. Results at [formmu2]z=0. MNRAS328(3):726–750. https://doi.org/10.1046/j.1365-8711.2001.04912.x . arXiv:astro-ph/0012055 [astro-ph]
2001
Earlier work this paper cites.
Stadel JG (2001) Cosmological N-body simulations and their analysis. PhD thesis, UNIVERSITY OF WASHINGTON
2001
Earlier work this paper cites.
2001
Earlier work this paper cites.
Taylor JE, Navarro JF (2001) The Phase-Space Density Profiles of Cold Dark Matter Halos. ApJ563(2):483–488. https://doi.org/10.1086/324031 . arXiv:astro-ph/0104002 [astro-ph]
2001
Earlier work this paper cites.
Trottenberg U, Oosterlee CW, Schüller A (2001) Multigrid, Texts in Applied Mathematics. Bd., vol 33. Academic Press, San Diego. With contributions by A. Brandt, P. Oswald and K. Stüben
2001
Earlier work this paper cites.
Bagla JS (2002) TreePM: A Code for Cosmological N-Body Simulations. J Astrophys Astron 23:185–196. https://doi.org/10.1007/BF02702282 . arXiv:astro-ph/9911025 [astro-ph]
2002
Earlier work this paper cites.
2002
Earlier work this paper cites.
Bernardeau F, Colombi S, Gaztañaga E, Scoccimarro R (2002) Large-scale structure of the Universe and cosmological perturbation theory. Phys. Rep.367(1-3):1–248. https://doi.org/10.1016/S0370-1573(02)00135-7 . arXiv:astro-ph/0112551 [astro-ph]
2002
Earlier work this paper cites.
2002
Earlier work this paper cites.
2002
Earlier work this paper cites.
Dehnen W (2002) A Hierarchical <E10>O</E10>(N) Force Calculation Algorithm. J Comput Phys 179(1):27–42. https://doi.org/10.1006/jcph.2002.7026 . arXiv:astro-ph/0202512 [astro-ph]
2002
Earlier work this paper cites.
Evrard AE, MacFarland TJ, Couchman HMP, Colberg JM, Yoshida N, White SDM, Jenkins A, Frenk CS, Pearce FR, Peacock JA, Thomas PA (2002) Galaxy Clusters in Hubble Volume Simulations: Cosmological Constraints from Sky Survey Populations. ApJ573(1):7–36. https://doi.org/10.1086/340551 . arXiv:astro-ph/0110246 [astro-ph]
2002
Earlier work this paper cites.
Goldstein H, Poole C, Safko J (2002) Classical mechanics. Addison-Wesley, San Francisco
2002
Earlier work this paper cites.
2002
Earlier work this paper cites.
2002
Earlier work this paper cites.
Kravtsov AV, Klypin A, Hoffman Y (2002) Constrained Simulations of the Real Universe. II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region. ApJ571(2):563–575. https://doi.org/10.1086/340046 . arXiv:astro-ph/0109077 [astro-ph]
2002
Earlier work this paper cites.
Monaco P, Theuns T, Taffoni G (2002) The pinocchio algorithm: pinpointing orbit-crossing collapsed hierarchical objects in a linear density field. MNRAS331(3):587–608. https://doi.org/10.1046/j.1365-8711.2002.05162.x . arXiv:astro-ph/0109323 [astro-ph]
2002
Earlier work this paper cites.
Scoccimarro R, Sheth RK (2002) PTHALOS: a fast method for generating mock galaxy distributions. MNRAS329(3):629–640. https://doi.org/10.1046/j.1365-8711.2002.04999.x . arXiv:astro-ph/0106120 [astro-ph]
2002
Earlier work this paper cites.
Teyssier R (2002) Cosmological hydrodynamics with adaptive mesh refinement. A new high resolution code called RAMSES. A&A385:337–364. https://doi.org/10.1051/0004-6361:20011817 . astro-ph/0111367
2002
Earlier work this paper cites.
Valageas P (2002) Transients from Zel’dovich initial conditions. A&A385:761–767. https://doi.org/10.1051/0004-6361:20020187 . astro-ph/0112102
2002
Earlier work this paper cites.
Zhang P, Zheng Y, Mauser NJ (2002) The limit from the schrödinger-poisson to the vlasov-poisson equations with general data in one dimension. Communications on Pure and Applied Mathematics 55(5):582–632. https://doi.org/https://doi.org/10.1002/cpa.3017
2002
Earlier work this paper cites.
Acquaviva V, Bartolo N, Matarrese S, Riotto A (2003) Gauge-invariant second-order perturbations and non-Gaussianity from inflation. Nuclear Physics B 667(1-2):119–148. https://doi.org/10.1016/S0550-3213(03)00550-9 . arXiv:astro-ph/0209156 [astro-ph]
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
Bagla JS, Ray S (2003) Performance characteristics of TreePM codes. New A8(7):665–677. https://doi.org/10.1016/S1384-1076(03)00056-3 . arXiv:astro-ph/0212129 [astro-ph]
2003
Earlier work this paper cites.
Berezinsky V, Dokuchaev V, Eroshenko Y (2003) Small-scale clumps in the galactic halo and dark matter annihilation. Phys. Rev. D68(10):103003. https://doi.org/10.1103/PhysRevD.68.103003 . arXiv:astro-ph/0301551 [astro-ph]
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
Chernin AD, Nagirner DI, Starikova SV (2003) Growth rate of cosmological perturbations in standard model: Explicit analytical solution. A&A399:19–21. https://doi.org/10.1051/0004-6361:20021763 . arXiv:astro-ph/0110107 [astro-ph]
2003
Earlier work this paper cites.
Creminelli P (2003) On non-Gaussianities in single-field inflation. J. Cosmology Astropart. Phys2003(10):003. https://doi.org/10.1088/1475-7516/2003/10/003 . arXiv:astro-ph/0306122 [astro-ph]
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
Klypin A, Hoffman Y, Kravtsov AV, Gottlöber S (2003) Constrained Simulations of the Real Universe: The Local Supercluster. ApJ596(1):19–33. https://doi.org/10.1086/377574 . arXiv:astro-ph/0107104 [astro-ph]
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
Maldacena J (2003) Non-gaussian features of primordial fluctuations in single field inflationary models. J High Energy Phys 2003(5):013. https://doi.org/10.1088/1126-6708/2003/05/013 . arXiv:astro-ph/0210603 [astro-ph]
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
Power C, Navarro JF, Jenkins A, Frenk CS, White SDM, Springel V, Stadel J, Quinn T (2003) The inner structure of Λ \Lambda CDM haloes - I. A numerical convergence study. MNRAS338(1):14–34. https://doi.org/10.1046/j.1365-8711.2003.05925.x . arXiv:astro-ph/0201544 [astro-ph]
2003
Earlier work this paper cites.
Reed D, Gardner J, Quinn T, Stadel J, Fardal M, Lake G, Governato F (2003) Evolution of the mass function of dark matter haloes. MNRAS346(2):565–572. https://doi.org/10.1046/j.1365-2966.2003.07113.x . arXiv:astro-ph/0301270 [astro-ph]
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
Smith RE, Peacock JA, Jenkins A, White SDM, Frenk CS, Pearce FR, Thomas PA, Efstathiou G, Couchman HMP (2003) Stable clustering, the halo model and non-linear cosmological power spectra. MNRAS341(4):1311–1332. https://doi.org/10.1046/j.1365-8711.2003.06503.x . arXiv:astro-ph/0207664 [astro-ph]
2003
Earlier work this paper cites.
2003
Earlier work this paper cites.
van den Bosch FC, Yang X, Mo HJ (2003) Linking early- and late-type galaxies to their dark matter haloes. MNRAS340(3):771–792. https://doi.org/10.1046/j.1365-8711.2003.06335.x . arXiv:astro-ph/0210495 [astro-ph]
2003
Earlier work this paper cites.
Yoshida N, Sugiyama N, Hernquist L (2003) The evolution of baryon density fluctuations in multicomponent cosmological simulations. MNRAS344(2):481–491. https://doi.org/10.1046/j.1365-8711.2003.06829.x . arXiv:astro-ph/0305210 [astro-ph]
2003
Earlier work this paper cites.
2004
Earlier work this paper cites.
Aubert D, Pichon C, Colombi S (2004) The origin and implications of dark matter anisotropic cosmic infall on ≈ L ⋆ \approx L_{\star} haloes. MNRAS352(2):376–398. https://doi.org/10.1111/j.1365-2966.2004.07883.x . arXiv:astro-ph/0402405 [astro-ph]
2004
Earlier work this paper cites.
Bartolo N, Komatsu E, Matarrese S, Riotto A (2004) Non-Gaussianity from inflation: theory and observations. Phys. Rep.402:103–266. https://doi.org/10.1016/j.physrep.2004.08.022 . astro-ph/0406398
2004
Earlier work this paper cites.
Baugh CM, Lacey CG, Frenk CS, Granato GL, Silva L, Bressan A, Benson AJ, Cole S (2005) Can the faint submillimetre galaxies be explained in the Λ \Lambda cold dark matter model? MNRAS356(3):1191–1200. https://doi.org/10.1111/j.1365-2966.2004.08553.x . arXiv:astro-ph/0406069 [astro-ph]
2004
Earlier work this paper cites.
Bertone G, Hooper D, Silk J (2004) Particle dark matter: evidence, candidates and constraints. Phys. Rep.405:279–390
2004
Earlier work this paper cites.
Diemand J, Moore B, Stadel J (2004a) Velocity and spatial biases in cold dark matter subhalo distributions. MNRAS352(2):535–546. https://doi.org/10.1111/j.1365-2966.2004.07940.x . arXiv:astro-ph/0402160 [astro-ph]
2004
Earlier work this paper cites.
Diemand J, Moore B, Stadel J, Kazantzidis S (2004b) Two-body relaxation in cold dark matter simulations. MNRAS348(3):977–986. https://doi.org/10.1111/j.1365-2966.2004.07424.x . arXiv:astro-ph/0304549 [astro-ph]
2004
Earlier work this paper cites.
Gao L, De Lucia G, White SDM, Jenkins A (2004) Galaxies and subhaloes in Λ \Lambda CDM galaxy clusters. MNRAS352(2):L1–L5. https://doi.org/10.1111/j.1365-2966.2004.08098.x . arXiv:astro-ph/0405010 [astro-ph]
2004
Earlier work this paper cites.
Gill SPD, Knebe A, Gibson BK (2004) The evolution of substructure - I. A new identification method. MNRAS351(2):399–409. https://doi.org/10.1111/j.1365-2966.2004.07786.x . arXiv:astro-ph/0404258 [astro-ph]
2004
Earlier work this paper cites.
Green AM, Hofmann S, Schwarz DJ (2004) The power spectrum of SUSY-CDM on subgalactic scales. MNRAS353(3):L23–L27. https://doi.org/10.1111/j.1365-2966.2004.08232.x . arXiv:astro-ph/0309621 [astro-ph]
2004
Earlier work this paper cites.
2004
Earlier work this paper cites.
Kravtsov AV, Berlind AA, Wechsler RH, Klypin AA, Gottlöber S, Allgood Bo, Primack JR (2004) The Dark Side of the Halo Occupation Distribution. ApJ609(1):35–49. https://doi.org/10.1086/420959 . arXiv:astro-ph/0308519 [astro-ph]
2004
Earlier work this paper cites.
2004
Earlier work this paper cites.
Lesgourgues J, Pastor S, Perotto L (2004) Probing neutrino masses with future galaxy redshift surveys. Phys. Rev. D70(4):045016. https://doi.org/10.1103/PhysRevD.70.045016 . arXiv:hep-ph/0403296 [hep-ph]
2004
Earlier work this paper cites.
Nakagami T, Matsubara T, Schmalzing J, Jing Y (2004) An Analysis of the Large Scale N-body Simulation using the Minkowski Functionals. arXiv e-prints astro-ph/0408428. arXiv:astro-ph/0408428 [astro-ph]
2004
Earlier work this paper cites.
Neyrinck MC, Gnedin NY, Hamilton AJS (2005) VOBOZ: an almost-parameter-free halo-finding algorithm. MNRAS356(4):1222–1232. https://doi.org/10.1111/j.1365-2966.2004.08505.x . arXiv:astro-ph/0402346 [astro-ph]
2004
Earlier work this paper cites.
2004
Earlier work this paper cites.
2004
Earlier work this paper cites.
2004
Earlier work this paper cites.
2004
Earlier work this paper cites.
Vale A, Ostriker JP (2004) Linking halo mass to galaxy luminosity. MNRAS353(1):189–200. https://doi.org/10.1111/j.1365-2966.2004.08059.x . arXiv:astro-ph/0402500 [astro-ph]
2004
Earlier work this paper cites.
Blaizot J, Wadadekar Y, Guiderdoni B, Colombi ST, Bertin E, Bouchet FR, Devriendt JEG, Hatton S (2005) MoMaF: the Mock Map Facility. MNRAS360(1):159–175. https://doi.org/10.1111/j.1365-2966.2005.09019.x . arXiv:astro-ph/0309305 [astro-ph]
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
Diemand J, Moore B, Stadel J (2005) Earth-mass dark-matter haloes as the first structures in the early Universe. Nature433(7024):389–391. https://doi.org/10.1038/nature03270 . arXiv:astro-ph/0501589 [astro-ph]
2005
Earlier work this paper cites.
Ellis GFR, Buchert T (2005) The universe seen at different scales [rapid communication]. Phys Lett A 347:38–46. https://doi.org/10.1016/j.physleta.2005.06.087 . arXiv:gr-qc/0506106 [gr-qc]
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
Frigo M, Johnson SG (2005) The design and implementation of FFTW3. Proceedings of the IEEE 93(2):216–231. Special issue on “Program Generation, Optimization, and Platform Adaptation”
2005
Earlier work this paper cites.
Gao L, White SDM, Jenkins A, Frenk CS, Springel V (2005) Early structure in Λ \Lambda CDM. MNRAS363(2):379–392. https://doi.org/10.1111/j.1365-2966.2005.09509.x . arXiv:astro-ph/0503003 [astro-ph]
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
Heitmann K, Ricker PM, Warren MS, Habib S (2005) Robustness of Cosmological Simulations. I. Large-Scale Structure. ApJS160(1):28–58. https://doi.org/10.1086/432646 . arXiv:astro-ph/0411795 [astro-ph]
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
Jing YP (2005) Correcting for the Alias Effect When Measuring the Power Spectrum Using a Fast Fourier Transform. ApJ620(2):559–563. https://doi.org/10.1086/427087 . arXiv:astro-ph/0409240 [astro-ph]
2005
Earlier work this paper cites.
Joyce M, Marcos B, Gabrielli A, Baertschiger T, Sylos Labini F (2005) Gravitational Evolution of a Perturbed Lattice and its Fluid Limit. Physical Review Letters 95(1):011304. https://doi.org/10.1103/PhysRevLett.95.011304 . astro-ph/0504213
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
Loeb A, Zaldarriaga M (2005) Small-scale power spectrum of cold dark matter. Phys. Rev. D71(10):103520. https://doi.org/10.1103/PhysRevD.71.103520 . arXiv:astro-ph/0504112 [astro-ph]
2005
Earlier work this paper cites.
Merz H, Pen UL, Trac H (2005) Towards optimal parallel PM N-body codes: PMFAST. New A10(5):393–407. https://doi.org/10.1016/j.newast.2005.02.001 . arXiv:astro-ph/0402443 [astro-ph]
2005
Earlier work this paper cites.
Mohayaee R, Mathis H, Colombi S, Silk J (2006) Reconstruction of primordial density fields. MNRAS365(3):939–959. https://doi.org/10.1111/j.1365-2966.2005.09774.x . arXiv:astro-ph/0501217 [astro-ph]
2005
Earlier work this paper cites.
O’Shea BW, Nagamine K, Springel V, Hernquist L, Norman ML (2005) Comparing AMR and SPH Cosmological Simulations. I. Dark Matter and Adiabatic Simulations. ApJS160(1):1–27. https://doi.org/10.1086/432645 . arXiv:astro-ph/0312651 [astro-ph]
2005
Earlier work this paper cites.
Padilla ND, Ceccarelli L, Lambas DG (2005) Spatial and dynamical properties of voids in a Λ \Lambda cold dark matter universe. MNRAS363(3):977–990. https://doi.org/10.1111/j.1365-2966.2005.09500.x . arXiv:astro-ph/0508297 [astro-ph]
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
2005
Earlier work this paper cites.
Sirko E (2005) Initial Conditions to Cosmological N-Body Simulations, or, How to Run an Ensemble of Simulations. ApJ634:728–743. https://doi.org/10.1086/497090 . astro-ph/0503106
2005
Earlier work this paper cites.
Springel V (2005) The cosmological simulation code GADGET-2. MNRAS364:1105–1134. https://doi.org/10.1111/j.1365-2966.2005.09655.x . astro-ph/0505010
2005
Earlier work this paper cites.
Springel V, White SDM, Jenkins A, Frenk CS, Yoshida N, Gao L, Navarro J, Thacker R, Croton D, Helly J, Peacock JA, Cole S, Thomas P, Couchman H, Evrard A, Colberg J, Pearce F (2005) Simulations of the formation, evolution and clustering of galaxies and quasars. Nature435(7042):629–636. https://doi.org/10.1038/nature03597 . arXiv:astro-ph/0504097 [astro-ph]
2005
Earlier work this paper cites.
Viel M, Lesgourgues J, Haehnelt MG, Matarrese S, Riotto A (2005) Constraining warm dark matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman- α \alpha forest. Phys. Rev. D71(6):063534. https://doi.org/10.1103/PhysRevD.71.063534 . arXiv:astro-ph/0501562 [astro-ph]
2005
Earlier work this paper cites.
Weller J, Ostriker JP, Bode P, Shaw L (2005) Fast identification of bound structures in large N-body simulations. MNRAS364(3):823–832. https://doi.org/10.1111/j.1365-2966.2005.09602.x . arXiv:astro-ph/0405445 [astro-ph]
2005
Earlier work this paper cites.
Zehavi I, Zheng Z, Weinberg DH, Frieman JA, Berlind AA, Blanton MR, Scoccimarro R, Sheth RK, Strauss MA, Kayo I, Suto Y, Fukugita M, Nakamura O, Bahcall NA, Brinkmann J, Gunn JE, Hennessy GS, Ivezić Ž, Knapp GR, Loveday J, Meiksin A, Schlegel DJ, Schneider DP, Szapudi I, Tegmark M, Vogeley MS, York DG, SDSS Collaboration (2005) The Luminosity and Color Dependence of the Galaxy Correlation Function. ApJ630(1):1–27. https://doi.org/10.1086/431891 . arXiv:astro-ph/0408569 [astro-ph]
2005
Earlier work this paper cites.
Zheng Z, Berlind AA, Weinberg DH, Benson AJ, Baugh CM, Cole S, Davé R, Frenk CS, Katz N, Lacey CG (2005) Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies. ApJ633(2):791–809. https://doi.org/10.1086/466510 . arXiv:astro-ph/0408564 [astro-ph]
2005
Earlier work this paper cites.
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Baugh CM (2006) A primer on hierarchical galaxy formation: the semi-analytical approach. Reports on Progress in Physics 69(12):3101–3156. https://doi.org/10.1088/0034-4885/69/12/R02 . arXiv:astro-ph/0610031 [astro-ph]
2006
Earlier work this paper cites.
Bower RG, Benson AJ, Malbon R, Helly JC, Frenk CS, Baugh CM, Cole S, Lacey CG (2006) Breaking the hierarchy of galaxy formation. MNRAS370(2):645–655. https://doi.org/10.1111/j.1365-2966.2006.10519.x . arXiv:astro-ph/0511338 [astro-ph]
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Conroy C, Wechsler RH, Kravtsov AV (2006) Modeling Luminosity-dependent Galaxy Clustering through Cosmic Time. ApJ647(1):201–214. https://doi.org/10.1086/503602 . arXiv:astro-ph/0512234 [astro-ph]
2006
Earlier work this paper cites.
Crocce M, Scoccimarro R (2006) Memory of initial conditions in gravitational clustering. Phys. Rev. D73(6):063520. https://doi.org/10.1103/PhysRevD.73.063520 . arXiv:astro-ph/0509419 [astro-ph]
2006
Earlier work this paper cites.
Crocce M, Pueblas S, Scoccimarro R (2006) Transients from initial conditions in cosmological simulations. MNRAS373:369–381. https://doi.org/10.1111/j.1365-2966.2006.11040.x . astro-ph/0606505
2006
Earlier work this paper cites.
Diemand J, Kuhlen M, Madau P (2006) Early Supersymmetric Cold Dark Matter Substructure. ApJ649(1):1–13. https://doi.org/10.1086/506377 . arXiv:astro-ph/0603250 [astro-ph]
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Hahn O, Porciani C, Carollo CM, Dekel A (2007b) Properties of dark matter haloes in clusters, filaments, sheets and voids. MNRAS375(2):489–499. https://doi.org/10.1111/j.1365-2966.2006.11318.x . arXiv:astro-ph/0610280 [astro-ph]
2006
Earlier work this paper cites.
Hairer E, Lubich C, Wanner G (2006) Geometric Numerical Integration: Structure-Preserving Algorithms for Ordinary Differential Equations; 2nd ed. Springer, Dordrecht
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Kim J, Park C (2006) A New Halo-finding Method for N-Body Simulations. ApJ639(2):600–616. https://doi.org/10.1086/499761 . arXiv:astro-ph/0401386 [astro-ph]
2006
Earlier work this paper cites.
Kurzak, J, Pettitt, B M (2006) Fast multipole methods for particle dynamics. Molecular simulation 32(10-11):775–790
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Lemson G, Virgo Consortium t (2006) Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony. arXiv e-prints astro-ph/0608019. arXiv:astro-ph/0608019 [astro-ph]
2006
Earlier work this paper cites.
Marcos B, Baertschiger T, Joyce M, Gabrielli A, Sylos Labini F (2006) Linear perturbative theory of the discrete cosmological N-body problem. Phys. Rev. D73(10):103507. https://doi.org/10.1103/PhysRevD.73.103507 . astro-ph/0601479
2006
Earlier work this paper cites.
Power C, Knebe A (2006) The impact of box size on the properties of dark matter haloes in cosmological simulations. MNRAS370(2):691–701. https://doi.org/10.1111/j.1365-2966.2006.10562.x . arXiv:astro-ph/0512281 [astro-ph]
2006
Earlier work this paper cites.
Price DJ, Monaghan JJ (2007) An energy-conserving formalism for adaptive gravitational force softening in smoothed particle hydrodynamics and N-body codes. MNRAS374(4):1347–1358. https://doi.org/10.1111/j.1365-2966.2006.11241.x . arXiv:astro-ph/0610872 [astro-ph]
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Springel V, Frenk CS, White SDM (2006) The large-scale structure of the Universe. Nature440(7088):1137–1144. https://doi.org/10.1038/nature04805 . arXiv:astro-ph/0604561 [astro-ph]
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Svrcek P, Witten E (2006) Axions in string theory. J High Energy Phys 6:051. https://doi.org/10.1088/1126-6708/2006/06/051 . hep-th/0605206
2006
Earlier work this paper cites.
2006
Earlier work this paper cites.
Warren MS, Abazajian K, Holz DE, Teodoro L (2006) Precision Determination of the Mass Function of Dark Matter Halos. ApJ646(2):881–885. https://doi.org/10.1086/504962 . arXiv:astro-ph/0506395 [astro-ph]
2006
Earlier work this paper cites.
2007
Cited alongside, same era.
2007
Cited alongside, same era.
Bartolo N, Matarrese S, Riotto A (2007) Course 5 - cosmic microwave background anisotropies up to second order. In: Bernardeau F, Grojean C, Dalibard J (eds) Particle Physics and Cosmology: The Fabric of Spacetime. Les Houches, vol 86. Elsevier, pp 233 – 285. https://doi.org/https://doi.org/10.1016/S0924-8099(07)80031-X
2007
Cited alongside, same era.
Klypin A, Prada F, Yepes G, Heß S, Gottlöber S (2015) Halo abundance matching: accuracy and conditions for numerical convergence. MNRAS447(4):3693–3707. https://doi.org/10.1093/mnras/stu2685
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
2007
Cited alongside, same era.
Colombi S, Touma J (2008) Vlasov Poisson: The waterbag method revisited. Communications in Nonlinear Science and Numerical Simulations 13(1):46–52. https://doi.org/10.1016/j.cnsns.2007.03.012
2007
Cited alongside, same era.
Creminelli P, Senatore L, Zaldarriaga M (2007) Estimators for local non-Gaussianities. J. Cosmology Astropart. Phys3:019. https://doi.org/10.1088/1475-7516/2007/03/019 . astro-ph/0606001
2007
Cited alongside, same era.
2007
Cited alongside, same era.
2007
Cited alongside, same era.
2007
Cited alongside, same era.
Hansen SH, Agertz O, Joyce M, Stadel J, Moore B, Potter D (2007) An Alternative to Grids and Glasses: Quaquaversal Pre-Initial Conditions for N-Body Simulations. ApJ656(2):631–635. https://doi.org/10.1086/510477 . arXiv:astro-ph/0606148 [astro-ph]
2007
Cited alongside, same era.
2007
Cited alongside, same era.
2007
Cited alongside, same era.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
Blanes S, Casas F (2016) A Concise Introduction to Geometric Numerical Integration, 1st edn. Chapman and Hall/CRC Press, New York
2016
Later among the works it cites.
2016
Later among the works it cites.
Borsanyi S, Fodor Z, Guenther J, Kampert KH, Katz SD, Kawanai T, Kovacs TG, Mages SW, Pasztor A, Pittler F, Redondo J, Ringwald A, Szabo KK (2016) Calculation of the axion mass based on high-temperature lattice quantum chromodynamics. Nature539(7627):69–71. https://doi.org/10.1038/nature20115
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
Igouchkine O, Leaf N, Ma KL (2016) Volume rendering dark matter simulations using cell projection and order-independent transparency. In: SIGGRAPH ASIA 2016 Symposium on Visualization. SA ’16. ACM, New York, NY, USA, pp 8:1–8:8. https://doi.org/10.1145/3002151.3002163
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
Potter D, Stadel J (2016) PKDGRAV3: Parallel gravity code. ascl:1609.016
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
2017
Later among the works it cites.
Baldi M, Villaescusa-Navarro F (2018) Cosmic degeneracies - II. Structure formation in joint simulations of warm dark matter and f(R) gravity. MNRAS473(3):3226–3240. https://doi.org/10.1093/mnras/stx2594
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
Li B (2018) Simulating Large-Scale Structure for Models of Cosmic Acceleration. https://doi.org/10.1088/978-0-7503-1587-6
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
Villaescusa-Navarro F (2018) Pylians: Python libraries for the analysis of numerical simulations. ascl:1811.008
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2018
Later among the works it cites.
2019
Later among the works it cites.
Anderson L, Pontzen A, Font-Ribera A, Villaescusa-Navarro F, Rogers KK, Genel S (2019) Cosmological Hydrodynamic Simulations with Suppressed Variance in the Ly α \alpha Forest Power Spectrum. ApJ871(2):144. https://doi.org/10.3847/1538-4357/aaf576
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
Carr B, Clesse S, García-Bellido J, Kühnel F (2021) Cosmic conundra explained by thermal history and primordial black holes. Physics of the Dark Universe 31:100755. https://doi.org/10.1016/j.dark.2020.100755
2020
Later among the works it cites.
2020
Later among the works it cites.
2020
Later among the works it cites.
2020
Later among the works it cites.
2020
Later among the works it cites.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
Ferreira EGM (2021) Ultra-light dark matter. The Astronomy and Astrophysics Review 29(1):7. https://doi.org/10.1007/s00159-021-00135-6 , URL https://doi.org/10.1007/s00159-021-00135-6
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
Hui L (2021) Wave Dark Matter. arXiv e-prints arXiv:2101.11735. arXiv:2101.11735 [astro-ph.CO]
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2021
Closest in time.
2041
Closest in time.
2043
Closest in time.
2050
Closest in time.
2054
Closest in time.
2072
Closest in time.
2076
Closest in time.
Frieman JA, Hill CT, Stebbins A, Waga I (1995) Cosmology with Ultralight Pseudo Nambu-Goldstone Bosons. Physical Review Letters 75:2077–2080. https://doi.org/10.1103/PhysRevLett.75.2077 . astro-ph/9505060
2077
Closest in time.
Demianski M, Golda ZA, Woszczyna A (2005) Evolution of density perturbations in a realistic universe. General Relativity and Gravitation 37(12):2063–2082. https://doi.org/10.1007/s10714-005-0180-2 . arXiv:gr-qc/0504089 [gr-qc]
2082
Closest in time.
2082
Closest in time.
2094
Closest in time.