= 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 a page that gives a [wiki:Tutorials/EnzoAlgorithms#EnzoAlgorithms brief outline of the essential physics in enzo].  Two general references (that should be considered to stand in for the method paper) are:

 * [http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0403044 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.  [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004astro.ph..3044O&data_type=BIBTEX&db_key=PRE&nocookieset=1 Bibtex entry]

 * [http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:0705.1556 Simulating Cosmological Evolution with Enzo] by '''Norman et al.'''  In "Petascale Computing: Algorithms and Applications," Ed. D. Bader, CRC Press LLC, 2007.  [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2007arXiv0705.1556N&data_type=BIBTEX&db_key=PRE&nocookieset=1 Bibtex entry]

Three somewhat older conferences proceedings are also relevant:

 * [http://adsabs.harvard.edu/abs/1997ASPC..123..363B 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. [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1997ASPC..123..363B&data_type=BIBTEX&db_key=AST&nocookieset=1 Bibtex entry]

 * [http://adsabs.harvard.edu/abs/1997astro.ph.10187B 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. [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1997astro.ph.10187B&data_type=BIBTEX&db_key=PRE&nocookieset=1 Bibtex entry]

 * [http://adsabs.harvard.edu/abs/1999ASSL..240...19N 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 [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1999ASSL..240...19N&data_type=BIBTEX&db_key=AST&nocookieset=1 Bibtex entry]

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

 * [http://adsabs.harvard.edu/abs/1984JCoPh..54..174C 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. [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1984JCoPh..54..174C&data_type=BIBTEX&db_key=AST&nocookieset=1 Bibtex entry]

 * [http://adsabs.harvard.edu/abs/1992ApJS...80..753S 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. [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1992ApJS...80..753S&data_type=BIBTEX&db_key=AST&nocookieset=1 Bibtex Entry]

The extension of PPM to cosmology can be found here:

 * [http://adsabs.harvard.edu/abs/1995CoPhC..89..149B A piecewise parabolic method for cosmological hydrodynamics.] by '''Bryan et al.''' Comput. Phys. Commun., Vol. 89, No. 1 - 3, p. 149 - 168 [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1995CoPhC..89..149B&data_type=BIBTEX&db_key=AST&nocookieset=1 Bibtex entry]

The AMR method used in Enzo can be found here:

 * [http://adsabs.harvard.edu/abs/1989JCoPh..82...64B 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. [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1989JCoPh..82...64B&data_type=BIBTEX&db_key=PHY&nocookieset=1 Bibtex Entry]

The YT introduction paper can be found here:

 * M Turk,  [http://conference.scipy.org/proceedings/SciPy2008/paper_11/ 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 ([http://yt.enzotools.org/wiki/Citation BibTeX entry])