.. _EnzoPrimaryReferences: Enzo Primary References ======================= The Enzo method paper is not yet complete. However, there are several papers that describe the numerical methods used in Enzo, and this documentation contains a brief outline of the essential physics in Enzo, in :ref:`EnzoAlgorithms`. 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 papers 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 (`Bibtex entry `_) * `yt: A Multi-code Analysis Toolkit for Astrophysical Simulation Data `_, by Turk, M. J.; Smith, B. D.; Oishi, J. S.; Skory, S.; Skillman, S. W.; Abel, T.; and Norman, M. L. The Astrophysical Journal Supplement, Volume 192, Issue 1, article id. 9 (2011) `Bibtex Entry `_.