P
Peng Wang
Researcher at Stanford University
Publications - 41
Citations - 3499
Peng Wang is an academic researcher from Stanford University. The author has contributed to research in topics: Dark matter & Adaptive mesh refinement. The author has an hindex of 17, co-authored 22 publications receiving 3197 citations. Previous affiliations of Peng Wang include Nvidia & Kavli Institute for Theoretical Physics.
Papers
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Journal ArticleDOI
Enzo: an adaptive mesh refinement code for astrophysics
Greg L. Bryan,Michael L. Norman,Brian W. O'Shea,Tom Abel,John H. Wise,Matthew J. Turk,Daniel R. Reynolds,David C. Collins,Peng Wang,Peng Wang,Samuel W. Skillman,Samuel W. Skillman,Britton D. Smith,Britton D. Smith,Robert P. Harkness,James Bordner,Ji-hoon Kim,Michael Kuhlen,Hao Xu,Nathan J. Goldbaum,Cameron Hummels,Alexei G. Kritsuk,Elizabeth J. Tasker,Stephen Skory,Christine M. Simpson,Oliver Hahn,Jeffrey S. Oishi,Geoffrey C. So,Fen Zhao,Renyue Cen,Yuan Li +30 more
TL;DR: Enzo as discussed by the authors uses block-structured adaptive mesh refinement to provide high spatial and temporal resolution for modeling astrophysical fluid flows, which can be run in one, two, and three dimensions, and supports a wide variety of physics, including hydrodynamics, ideal and non-ideal magnetohydrodynamic, N-body dynamics, primordial gas chemistry, optically thin radiative cooling of primordial and metal-enriched plasmas, and models for star formation and feedback in a cosmological context.
Journal ArticleDOI
Enzo: An Adaptive Mesh Refinement Code for Astrophysics
Greg L. Bryan,Michael L. Norman,Brian W. O'Shea,Tom Abel,John H. Wise,Matthew J. Turk,Daniel R. Reynolds,David C. Collins,Peng Wang,Samuel W. Skillman,Britton D. Smith,Robert P. Harkness,James Bordner,Ji-hoon Kim,Michael Kuhlen,Hao Xu,Nathan J. Goldbaum,Cameron Hummels,Alexei G. Kritsuk,Elizabeth J. Tasker,Stephen Skory,Christine M. Simpson,Oliver Hahn,Jeffrey S. Oishi,Geoffrey C. So,Fen Zhao,Renyue Cen,Yuan Li +27 more
TL;DR: Enzo as mentioned in this paper uses block-structured adaptive mesh refinement to provide high spatial and temporal resolution for modeling astrophysical fluid flows, which can be run in 1, 2, and 3 dimensions, and supports a wide variety of physics, including hydrodynamics, ideal and non-ideal magnetohydrodynamic, N-body dynamics, primordial gas chemistry, optically-thin radiative cooling of primordial and metal-enriched plasmas, and models for star formation and feedback.
Enzo: An Adaptive Mesh Refinement Code for Astrophysics
Greg L. Bryan,Michael L. Norman,Brian W. O'Shea,Tom Abel,John H. Wise,Matthew J. Turk,Daniel R. Reynolds,David C. Collins,Peng Wang,Samuel W. Skillman,Britton D. Smith,Robert P. Harkness,James Bordner,Ji-hoon Kim,Michael Kuhlen,Hao Xu,Nathan J. Goldbaum,Cameron Hummels,Alexei G. Kritsuk,Elizabeth J. Tasker,Stephen Skory +20 more
TL;DR: Enzo as discussed by the authors uses block-structured adaptive mesh refinement to provide high spatial and temporal resolution for modeling astrophysical fluid flows, which can be run in one, two, and three dimensions, and supports a wide variety of physics, including hydrodynamics, ideal and non-ideal magnetohydrodynamic, N-body dynamics, primordial gas chemistry, optically thin radiative cooling of primordial and metal-enriched plasmas, and models for star formation and feedback in a cosmological context.
Journal ArticleDOI
Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster-Forming Clumps
TL;DR: In this article, the authors investigate massive star formation in turbulent, magnetized, parsec-scale clumps of molecular clouds including protostellar outflow feedback using three dimensional numerical simulations.
Journal ArticleDOI
Fermi large area telescope observations of the vela pulsar
A. A. Abdo,A. A. Abdo,Markus Ackermann,W. B. Atwood,R. Bagagli,Luca Baldini,Jean Ballet,David L. Band,Guido Barbiellini,Guido Barbiellini,Matthew G. Baring,J. Bartelt,Denis Bastieri,Denis Bastieri,B. M. Baughman,Keith Bechtol,F. Bellardi,Ronaldo Bellazzini,B. Berenji,Dario Bisello,Dario Bisello,Roger Blandford,Elliott D. Bloom,J.R. Bogart,Emanuele Bonamente,Emanuele Bonamente,A. W. Borgland,A. Bouvier,J. Bregeon,Alessandro Brez,M. Brigida,M. Brigida,P. Bruel,T. H. Burnett,G. A. Caliandro,G. A. Caliandro,R. A. Cameron,Fernando Camilo,P. A. Caraveo,J. M. Casandjian,M. Ceccanti,Claudia Cecchi,Claudia Cecchi,E. Charles,A. Chekhtman,A. Chekhtman,C. C. Cheung,James Chiang,Stefano Ciprini,Stefano Ciprini,R. Claus,Ismaël Cognard,Johann Cohen-Tanugi,L. R. Cominsky,Jan Conrad,Jan Conrad,Robin H. D. Corbet,L. Corucci,S. Cutini,David S. Davis,David S. Davis,M. Deklotz,Charles D. Dermer,A. De Angelis,F. de Palma,F. de Palma,Seth Digel,M. Dormody,E. Do Couto E Silva,Persis S. Drell,Richard Dubois,D. Dumora,D. Dumora,Cristobal M. Espinoza,Christian Farnier,C. Favuzzi,C. Favuzzi,D. Flath,P. Fleury,W. B. Focke,M. Frailis,P. C C Friere,Yasushi Fukazawa,Stefan Funk,P. Fusco,P. Fusco,F. Gargano,Dario Gasparrini,Neil Gehrels,Neil Gehrels,S. Germani,S. Germani,R. Giannitrapani,B. Giebels,Nicola Giglietto,Nicola Giglietto,Francesco Giordano,Francesco Giordano,T. Glanzman,G.L. Godfrey,Eric V. Gotthelf,I. A. Grenier,M.-H. Grondin,M.-H. Grondin,J. E. Grove,L. Guillemot,L. Guillemot,S. Guiriec,Gunther Haller,Alice K. Harding,P. A. Hart,R. C. Hartman,Elizabeth Hays,George Hobbs,R. E. Hughes,Gudlaugur Johannesson,A. S. Johnson,R. P. Johnson,Tyrel J. Johnson,Tyrel J. Johnson,W. N. Johnson,Simon Johnston,T. Kamae,Gottfried Kanbach,Victoria M. Kaspi,Hideaki Katagiri,Jun Kataoka,A. Kavelaars,N. Kawai,H. Kelly,Matthew Kerr,Bulent Kiziltan,Wlodzimierz Klamra,Jürgen Knödlseder,Michael Kramer,F. Kuehn,M. Kuss,J. Lande,D. Landriu,Luca Latronico,B. Lee,Shiu-Hang Lee,Marianne Lemoine-Goumard,Marianne Lemoine-Goumard,Margaret A. Livingstone,Francesco Longo,Francesco Longo,F. Loparco,F. Loparco,Benoit Lott,Benoit Lott,M. N. Lovellette,P. Lubrano,P. Lubrano,Andrew Lyne,Grzegorz Madejski,A. Makeev,A. Makeev,R. N. Manchester,B. Marangelli,B. Marangelli,M. Marelli,M. N. Mazziotta,Julie McEnery,S. McGlynn,Maura McLaughlin,N. Menon,C. Meurer,Peter F. Michelson,Teresa Mineo,N. Mirizzi,N. Mirizzi,W. Mitthumsiri,Tsunefumi Mizuno,A. A. Moiseev,M. Mongelli,C. Monte,C. Monte,M. E. Monzani,Elena Moretti,Elena Moretti,A. Morselli,A. Morselli,Igor V. Moskalenko,S. Murgia,Takeshi Nakamori,P. L. Nolan,A. Noutsos,Eric Nuss,T. Ohsugi,Nicola Omodei,E. Orlando,J. F. Ormes,M. Ozaki,Alessandro Paccagnella,Alessandro Paccagnella,David Paneque,J. H. Panetta,D. Parent,D. Parent,Mark Pearce,M. Pepe,M. Pepe,M. Perchiazzi,Melissa Pesce-Rollins,L. Pieri,Michele Pinchera,F. Piron,T. A. Porter,S. Rainò,S. Rainò,Riccardo Rando,Riccardo Rando,Scott M. Ransom,E. Rapposelli,M. Razzano,A. Reimer,Olaf Reimer,T. Reposeur,T. Reposeur,L. C. Reyes,S. Ritz,S. Ritz,L.S. Rochester,A. Y. Rodriguez,Roger W. Romani,M. Roth,Felix Ryde,A. Sacchetti,Hartmut Sadrozinski,N. Saggini,David Sanchez,A. Sander,P. M. Saz Parkinson,K. N. Segal,A. Sellerholm,Carmelo Sgrò,E. J. Siskind,David A. Smith,David A. Smith,P. D. Smith,Gloria Spandre,P. Spinelli,P. Spinelli,M. Stamatikos,Jean-Luc Starck,Floyd W. Stecker,T. E. Stephens,M. S. Strickman,Andrew W. Strong,D. J. Suson,H. Tajima,Hiromitsu Takahashi,Tadayuki Takahashi,Takaaki Tanaka,A. Tenze,J. B. Thayer,J. G. Thayer,Gilles Theureau,D. J. Thompson,Stephen E. Thorsett,L. Tibaldo,L. Tibaldo,O. Tibolla,Diego F. Torres,Diego F. Torres,A. Tramacere,M. Turri,T. L. Usher,L. Vigiani,N. Vilchez,V. Vitale,V. Vitale,A. P. Waite,Peng Wang,Karen Watters,Patrick Weltevrede,Brian L Winer,K. S. Wood,T. Ylinen,M. Ziegler +280 more
TL;DR: In this paper, the Vela pulsar was used to verify Fermi timing and angular resolution, and the high energy behavior of the pulsed emission was examined; initial spectra suggest a phase-averaged power law index of Gamma=1.51{+0.05/-0.04} with an exponential cut-off at E_c=2.1 GeV.