ECOSMOG: An efficient code for simulating modified gravity

Journal of Cosmology and Astroparticle Physics

Volumn 2012, Issue 1, 2012, Pages

  Li, Baojiu ^a,b,c   Zhao, Gong Bo ^d   Teyssier, Romain ^e,f   Koyama, Kazuya ^d  

^a DURHAM UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d UNIVERSITY OF PORTSMOUTH   (United Kingdom)

^e UNIVERSITY OF ZURICH   (Switzerland)

^f CEA SACLAY   (France)

Author keywords

cosmological simulations; dark energy theory; modified gravity; power spectrum

Indexed keywords

EID: 84863080786     PISSN: None     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2012/01/051     Document Type: Review

References (35)

1. E.J. Copeland, M. Sami and S. Tsujikawa, 2006 Dynamics of dark energy, Int. J. Mod. Phys. D 15 1753 [hep-th/0603057]
2. I. Zlatev, L.-M. Wang and P.J. Steinhardt, 1999 Quintessence, cosmic coincidence and the cosmological constant, Phys. Rev. Lett. 82 896 [astro-ph/9807002]
3. C. Armendariz-Picon, V. Mokhanov and P.J. Steinhardt, 2000 Dynamical solution to the problem of a small cosmological constant and late-time cosmic acceleration, Phys. Rev. Lett. 85 4438 [astro-ph/0004134]
4. L. Amendola, 2000 Coupled quintessence, Phys. Rev. D 62 043511 [astro-ph/9908023]
5. J. Khoury and A. Weltman, 2004 Chameleon cosmology, Phys. Rev. D 69 044026 [astro-ph/0309411]
6. D.F. Mota and D.J. Shaw, 2007 Evading equivalence principle violations, cosmological and other experimental constraints in scalar field theories with a strong coupling to matter, Phys. Rev. D 75 063501 [hep-ph/0608078]
7. K. Hinterbichler and J. Khoury, 2010 Symmetron fields: screening long-range forces through local symmetry restoration, Phys. Rev. Lett. 104 231301 [1001.4525]
8. S.M. Carroll et al., 2005 The cosmology of generalized modified gravity models, Phys. Rev. D 71 063513 [astro-ph/0410031]
9. F. Perrotta, C. Baccigalupi and S. Matarrese, 2000 Extended quintessence, Phys. Rev. D 61 023507 [astro-ph/9906066]
10. G. Dvali, G. Gabadadze and M. Porrati, 2000 4D gravity on a brane in 5D Minkowski space, Phys. Lett. B 485 208 [hep-th/0005016]
11. K. Koyama, 2008 The cosmological constant and dark energy in braneworlds, Gen. Rel. Grav. 40 421 [0706.1557]
12. R. Durrer and R. Maartens, 2008 Dark energy and dark gravity, Gen. Rel. Grav. 40 301 [0711.0077]
13. T.P. Sotiriou and V. Faraoni, 2010 f(R) theories of gravity, Rev. Mod. Phys. 82 451 [0805.1726]
14. B. Li and J.D. Barrow, 2007 The cosmology of f(R) gravity in metric variational approach, Phys. Rev. D 75 084010 [gr-qc/0701111]
15. H. Oyaizu, 2008 Non-linear evolution of f(R) cosmologies. 1. methodology, Phys. Rev. D 78 123523 [0807.2449]
16. H. Oyaizu, M. Lima and W. Hu, 2008 Nonlinear evolution of f(R) cosmologies. 2. Power spectrum, Phys. Rev. D 78 123524 [0807.2462]
17. F. Schmidt, M.V. Lima, H. Oyaizu and W. Hu, 2009 Non-linear evolution of f(R) cosmologies. 3. Halo statistics, Phys. Rev. D 79 083518 [0812.0545]
18. F. Schmidt and F. Schmidt, 2009 Self-consistent cosmological simulations of DGP braneworld gravity, Phys. Rev. D 80 043001 [0905.0858]
19. A. Knebe, A. Green and J. Binney, 2001 Multi-Level Adaptive Particle Mesh (MLAPM) - a C code for cosmological simulations, Mon. Not. Roy. Astron. Soc. 325 845 [astro-ph/0103503]
20. B. Li and H. Zhao, 2009 Structure formation by fifth force I: N-body vs. linear simulations, Phys. Rev. D 80 044027 [0906.3880]
21. B. Li and H. Zhao, 2010 Structure formation by the fifth force III: segregation of baryons and dark matter, Phys. Rev. D 81 104047 [1001.3152]
22. G.-B. Zhao, B. Li and K. Koyama, 2011 N-body simulations for f(R) gravity using a self-adaptive particle-mesh code, Phys. Rev. D 83 044007 [1011.1257]
23. B. Li and J.D. Barrow, 2011 N-body simulations for coupled scalar field cosmology, Phys. Rev. D 83 024007 [1005.4231]
24. B. Li, D.F. Mota and J.D. Barrow, 2011 Varying alpha from N-body simulations, Astrophys. J. 728 108 [1009.1396]
25. B. Li, D.F. Mota and J.D. Barrow, 2011 N-body simulations for extended quintessence models, Astrophys. J. 728 109 [1009.1400]
26. P. Brax, C. van de Bruck, A.-C. Davis, B. Li and D.J. Shaw, 2011 Nonlinear structure formation with the environmentally dependent dilaton, Phys. Rev. D 83 104026 [1102.3692]
27. C. Villforth, K. Nilsson, J. Heidt and T. Pursimo, Variability and stability in optical blazar jets: the case of OJ287, submitted to Astrophys. J. [1008.3082]
28. R. Teyssier, 2002 Cosmological hydrodynamics with adaptive mesh refinement: a new high resolution code called RAMSES, Astron. Astrophys. 385 337 [astro-ph/0111367]
29. W. Hu and I. Sawicki, 2007 Models of f(R) cosmic acceleration that evade solar-system tests, Phys. Rev. D 76 064004 [0705.1158]
30. H. Martel and P.R. Shapiro, 1998 A convenient set of comoving cosmological variables and their application, Mon. Not. Roy. Astron. Soc. 297 467 [astro-ph/9710119]
31. R.W. Hockney and J.W. Eastwood, 1988 Computer simulation using particles, published by the Taylor & Francis Group, New York U.S.A.
32. Virgo Consortium collaboration, R. Smith et al., 2003 Stable clustering, the halo model and nonlinear cosmological power spectra, Mon. Not. Roy. Astron. Soc. 341 1311 [astro-ph/0207664]
33. T. Guillet and R. Teyssier, 2011 A simple multigrid scheme for solving the Poisson equation with arbitrary domain boundaries, J. Comput. Phys. 230 4756 [1104.1703]
34. S. Prunet et al., Initial conditions for large cosmological simulations, [0804.3536]
35. S. Colombi, A.H. Jaffe, D. Novikov and C. Pichon, Accurate estimators of power spectra in N-body simulations, [0811.0313]