Abstract
We describe the two-dimensional TreePM method in this paper. The 2d TreePM code is an accurate and efficient technique to carry out large two-dimensional N-body simulations in cosmology. This hybrid code combines the 2d Barnes and Hut Tree method and the 2d Particle-Mesh method. We describe the splitting of force between the PM and the Tree parts. We also estimate error in force for a realistic configuration. Finally, we discuss some tests of the code.
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Bagla, J. S., Padmanabhan, T. 1997,Pramana — Journal of Physics,49, 161.
Bagla, J. S., Engineer, S., Padmanabhan, T. 1998,ApJ,495, 25.
Bagla, J. S. 2002,JAA,23, 185.
Bagla, J. S., Ray, S. 2002,New Astronomy,8, 665.
Bagla, J. S. 2003,A parallel TreePM code, Numerical Simulations in Astronomy (eds) K. Tomisaka and T. Hanawa, 2003, p. 32.
Barnes, J., Hut, P. 1986,Nature,324, 446.
Barnes, J. E. 1990,J. Comp. Phys.,87, 161.
Bertschinger, E. 1998,ARA & A,36, 599.
Bode, P., Ostriker, J. 2003,ApJL,145, 1.
Bouchet, F. R., Kandrup, H. E. 1985,ApJ,299, 1.
Dehnen, W. 2001,MNRAS,324, 273.
Dubinski, J., Kim, J., Park, C., Humble, R. 2004,New Astronomy,9, 111.
Efstathiou, G., Davis, M., Frenk, C. S., White, S. D. M. 1985,ApJS,57, 241.
Ewald, P. P. 1921,Ann. Physik,64, 253.
Filmore, J. A., Goldreich, P. 1984,ApJ,281, 1.
Hamilton, A. J. S., Kumar, P., Edward, L., Matthews, A. 1991,ApJ,374, L1.
Hernquist, L., Bouchet, F. R., Suto, Y. 1991,ApJS,75, 231.
Hockney, R. W., Eastwood, J. W. 1988,Computer Simulation using Particles (New York: McGraw Hill).
Monaghan, J. J. 1992,Annu. Rev. Astron. Astrophys.,30, 543.
Munshi, D., Coles, P. 1998,MNRAS,293, L68.
Nityananda, R., Padmanabhan, T. 1994,MNRAS,271, 976.
Padmanabhan, T. 1996,MNRAS,278, L29.
Ray, S., Bagla, J. 2004, astro-ph/0405220.
Springel, V., Yoshida, N., White, S. D. M. 2001,New Astronomy,6, 79S.
Xu, G. 1995,ApJS,98, 355.
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Ray, S. TreePM method for two-dimensional cosmological simulations. J Astrophys Astron 25, 103–113 (2004). https://doi.org/10.1007/BF02702367
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DOI: https://doi.org/10.1007/BF02702367