Enzo primary references

The Enzo method paper is not yet complete. However, there are several papers that describe the numerical methods used in Enzo. Two general references (that should be considered to stand in for the method paper) are:

• Introducing Enzo, an AMR Cosmology Application by O'Shea et al. In "Adaptive Mesh Refinement - Theory and Applications," Eds. T. Plewa, T. Linde & V. G. Weirs, Springer Lecture Notes in Computational Science and Engineering, 2004. Bibtex entry

• Simulating Cosmological Evolution with Enzo by Norman et al. In "Petascale Computing: Algorithms and Applications," Ed. D. Bader, CRC Press LLC, 2007. Bibtex entry

Three somewhat older conferences proceedings are also relevant:

• Simulating X-Ray Clusters with Adaptive Mesh Refinement by Bryan and Norman. In "Computational Astrophysics; 12th Kingston Meeting on Theoretical Astrophysics;" proceedings of meeting held in Halifax; Nova Scotia; Canada October 17-19; 1996, ASP Conference Series #123, edited by D. A. Clarke and M. J. West., p. 363. Bibtex entry

• A Hybrid AMR Application for Cosmology and Astrophysics by Bryan and Norman. In "Workshop on Structured Adaptive Mesh Refinement Grid Methods", Mar. 1997, ed. N. Chrisochoides. Bibtex entry

• Cosmological Adaptive Mesh Refinement by Norman and Bryan. In "Numerical Astrophysics : Proceedings of the International Conference on Numerical Astrophysics 1998 (NAP98)," held at the National Olympic Memorial Youth Center, Tokyo, Japan, March 10-13, 1998. Edited by Shoken M. Miyama, Kohji Tomisaka, and Tomoyuki Hanawa. Boston, Mass. : Kluwer Academic, 1999. (Astrophysics and space science library ; v. 240), p.19 Bibtex entry

The primary hydrodynamics methods are PPM and ZEUS, as described in the following two papers:

• The Piecewise Parabolic Method (PPM) for Gas-Dynamical Simulations by Colella, P.; Woodward, Paul R. Journal of Computational Physics (ISSN 0021-9991), vol. 54, April 1984, p. 174-201. Bibtex entry

• ZEUS-2D: A radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. I - The hydrodynamic algorithms and tests. by Stone and Norman Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 80, no. 2, June 1992, p. 753-790. Bibtex Entry

The extension of PPM to cosmology can be found here:

• A piecewise parabolic method for cosmological hydrodynamics. by Bryan et al. Comput. Phys. Commun., Vol. 89, No. 1 - 3, p. 149 - 168 Bibtex entry

The AMR method used in Enzo can be found here:

• Local adaptive mesh refinement for shock hydrodynamics by Berger, M. J. and Colella, P. Journal of Computational Physics (ISSN 0021-9991), vol. 82, May 1989, p. 64-84. Bibtex Entry

The YT introduction paper can be found here:

• M Turk, Analysis and Visualization of Multi-Scale Astrophysical Simulations Using Python and NumPy in Proceedings of the 7th Python in Science conference (SciPy 2008), G Varoquaux, T Vaught, J Millman (Eds.), pp. 46-50