C. Cardall

发表

TURBULENT MAGNETIC FIELD AMPLIFICATION FROM SPIRAL SASI MODES: IMPLICATIONS FOR CORE-COLLAPSE SUPERNOVAE AND PROTO-NEUTRON STAR MAGNETIZATION

E. Endeve, C. Cardall, R. Budiardja, 2012, 1203.3108.

Fully threaded transport engine: new method for multi-scale radiative transfer

C. Cardall, A. Razoumov, 2005, astro-ph/0505172.

GenASiS: General Astrophysical Simulation System. II. Nonrelativistic Hydrodynamics

E. Endeve, C. Cardall, R. Budiardja, 2012, 1207.3393.

Supernova neutrinos

C. Cardall, 2007, astro-ph/0703334.

Intermediate baseline appearance experiments and three-neutrino mixing schemes

C. Cardall, D. Cline, G. Fuller, 1997, hep-ph/9706426.

NewtonPlus: Approximate Relativity for Supernova Simulations

C. Cardall, A. Mezzacappa, M. Liebendoerfer, 2001, astro-ph/0106105.

NewtonPlus: Approximating Relativistic Effects in Supernova Simulations

C. Cardall, A. Mezzacappa, 2001, astro-ph/0106287.

General Relativistic Effects in the Neutrino-driven Wind and r-Process Nucleosynthesis

C. Cardall, G. Fuller, 1997, astro-ph/9701178.

Three-generation neutrino mixing and LSND dark matter neutrinos

C. Cardall, G. Fuller, 1996, astro-ph/9606024.

The deuteron confronts big bang nucleosynthesis

C. Cardall, G. Fuller, 1996, astro-ph/9606025.

Turbulent magnetic field amplification from spiral SASI modes in core-collapse supernovae

E. Endeve, C. Cardall, R. Budiardja, 2012, 1203.3385.

MHD models of stellar core collapse with GenASiS

E. Endeve, C. Cardall, R. Budiardja, 2007 .

Effects of Strong Magnetic Fields on Neutron Star Structure

C. Cardall, J. Lattimer, M. Prakash, 2000, astro-ph/0011148.

The deuteron confronts big bang nucleosynthesis

C. Cardall, G. Fuller, 1996, astro-ph/9606025.

Supernova neutrinos, from back of the envelope to supercomputer

C. Cardall, 2007, astro-ph/0701831.

A Finite Difference Representation of Neutrino Radiation Hydrodynamics in Spherically Symmetric General Relativistic Spacetime

O. E. Bronson Messer, C. Cardall, A. Mezzacappa, 2002, astro-ph/0207036.

Three-generation neutrino mixing and LSND dark matter neutrinos

C. Cardall, G. Fuller, 1996, astro-ph/9606024.

Supernova neutrinos

C. Cardall, 2007, astro-ph/0703334.

Intermediate baseline appearance experiments and three-neutrino mixing schemes

C. Cardall, D. Cline, G. Fuller, 1997, hep-ph/9706426.

Effects of Strong Magnetic Fields on Neutron Star Structure

C. Cardall, J. Lattimer, M. Prakash, 2000, astro-ph/0011148.

NewtonPlus: Approximate Relativity for Supernova Simulations

C. Cardall, A. Mezzacappa, M. Liebendoerfer, 2001, astro-ph/0106105.

J un 2 00 1 NewtonPlus : Approximate Relativity for Supernova Simulations

C. Cardall, A. Mezzacappa, M. Liebendörfer, 2001 .

Ju n 20 01 NewtonPlus : Approximating Relativistic Effects in Supernova Simulations

C. Cardall, A. Mezzacappa, 2001 .

Theory of Neutrino Flavor Mixing

C. Cardall, 2001, hep-ph/0107004.

0 Ju n 20 01 Theory of Neutrino Flavor Mixing

C. Cardall, 2001 .

01 07 00 4 v 1 30 J un 2 00 1 Theory of Neutrino Flavor Mixing

C. Cardall, 2022 .

Conservative formulations of general relativistic kinetic theory

Knoxville, C. Cardall, U. Tennessee, 2002, astro-ph/0212460.

Big Bang Nucleosynthesis in Light of Discordant Deuterium Measurements

C. Cardall, G. Fuller, 1996, astro-ph/9603071.

Fully threaded transport engine: new method for multi-scale radiative transfer

C. Cardall, A. Razoumov, 2005, astro-ph/0505172.

Conservative special relativistic radiative transfer for multidimensional astrophysical simulations: motivation and elaboration

Knoxville, C. Cardall, E. Lentz, 2005, astro-ph/0510702.

An Approach to Neutrino Radiative Transfer in Supernova Simulations

C. Cardall, 2004, astro-ph/0404401.

Supernova neutrino challenges

C. Cardall, 2005, astro-ph/0502232.

MSW effect in quantum field theory

C. Cardall, D. Chung, 1999, hep-ph/9904291.

Accelerating our understanding of supernova explosion mechanism via simulations and visualizations with GenASiS

Reuben D. Budiardja, Christian Y. Cardall, Eirik Endeve, 2015, XSEDE.

GenASiS: GENERAL ASTROPHYSICAL SIMULATION SYSTEM. I. REFINABLE MESH AND NONRELATIVISTIC HYDRODYNAMICS

Reuben D. Budiardja, Christian Y. Cardall, Eirik Endeve, 2012, 1207.3392.

Liouville equations for neutrino distribution matrices

C. Cardall, 2007, 0712.1188.

Neutrino oscillations in curved spacetime: A heuristic treatment

C. Cardall, G. Fuller, 1996, hep-ph/9610494.

Conservative 3+1 general relativistic variable Eddington tensor radiation transport equations

E. Endeve, C. Cardall, A. Mezzacappa, 2012, 1209.2151.

Conservative 3 + 1 general relativistic Boltzmann equation

Christian Y. Cardall, Eirik Endeve, Anthony Mezzacappa, 2013, 1305.0037.

Coherence of neutrino flavor mixing in quantum field theory

C. Cardall, 1999, hep-ph/9909332.

On Steady State Neutrino-heated Ultrarelativistic Winds from Compact Objects

C. Cardall, G. Fuller, J. Pruet, 2001, astro-ph/0103455.

Parallel FFT-based Poisson solver for isolated three-dimensional systems

Reuben D. Budiardja, Christian Y. Cardall, C. Cardall, 2011, Comput. Phys. Commun..

Convection- and SASI-driven flows in parametrized models of core-collapse supernova explosions

E. Endeve, C. Cardall, R. Budiardja, 2016 .

Supernova Modeling: Progress and Challenges

C. Cardall, 2012 .

GenASiS: General Astrophysical Simulation System. I. Fundamentals pdf

Reuben D. Budiardja, Christian Y. Cardall, Eirik Endeve, 2012, ArXiv.

Turbulence and magnetic field amplification from spiral SASI modes in core-collapse supernovae

E. Endeve, C. Cardall, R. Budiardja, 2012, 1203.3748.

Core-collapse supernova explosion simulations

C. Cardall, 2011 .

GENERATION OF MAGNETIC FIELDS BY THE STATIONARY ACCRETION SHOCK INSTABILITY

Reuben D. Budiardja, Christian Y. Cardall, Eirik Endeve, 2008, 0811.3385.

Core-collapse supernovae and gravitational waves

C. Cardall, 2004, astro-ph/0401060.

A Finite Difference Representation of Neutrino Radiation Hydrodynamics for Spherically Symmetric General Relativistic Supernova Simulations

O. E. Bronson Messer, C. Cardall, A. Mezzacappa, 2002 .

Magnetic field generation by the stationary accretion shock instability

R. D. Budiardja, E. Endeve, C. Cardall, 2008, 0806.3104.

TURBULENT MAGNETIC FIELD AMPLIFICATION FROM SPIRAL SASI MODES: IMPLICATIONS FOR CORE-COLLAPSE SUPERNOVAE AND PROTO-NEUTRON STAR MAGNETIZATION

E. Endeve, C. Cardall, R. Budiardja, 2012, 1203.3108.

STOCHASTICITY AND EFFICIENCY IN SIMPLIFIED MODELS OF CORE-COLLAPSE SUPERNOVA EXPLOSIONS

C. Cardall, R. Budiardja, 2015, 1509.02494.

Relativistic analogue of the Newtonian fluid energy equation with nucleosynthesis

C. Cardall, 2017, 1802.05590.

Minkowski and Galilei/Newton Fluid Dynamics: A Geometric 3 + 1 Spacetime Perspective

C. Cardall, 2018, Fluids.

Degeneracy, the virial theorem, and stellar collapse

C. Cardall, 2008, 0812.0114.

Fluid Dynamics in Curvilinear Coordinates without Fictitious Forces

C. Cardall, 2021, Fluids.

Combining 3-Momentum and Kinetic Energy on Galilei/Newton Spacetime

C. Cardall, 2019, Symmetry.

GenASiS Mathematics : Object-oriented manifolds, operations, and solvers for large-scale physics simulations

Reuben D. Budiardja, Christian Y. Cardall, C. Cardall, 2017, Comput. Phys. Commun..

GenASiS Basics: Object-oriented utilitarian functionality for large-scale physics simulations

Reuben D. Budiardja, Christian Y. Cardall, C. Cardall, 2015, Comput. Phys. Commun..