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Nucleosynthesis during a Thermonuclear Supernova Explosion

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Artificial neural network approach to large-eddy simulation of compressible isotropic turbulence

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Algorithmic comparisons of decaying, isothermal, supersonic turbulence

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Gasoline2: a modern smoothed particle hydrodynamics code

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Compression of turbulent magnetized gas in giant molecular clouds

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Turbulence production and turbulent pressure support in the intergalactic medium

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Reynolds number effects on Rayleigh–Taylor instability with possible implications for type Ia supernovae

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Black hole formation in the early Universe

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High-resolution studies of massive primordial haloes

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An observational method to measure the relative fractions of solenoidal and compressible modes in interstellar clouds

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The characteristic black hole mass resulting from direct collapse in the early Universe

M. A. Latif, D. R. G. Schleicher, W. Schmidt and J. C. Niemeyer
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3D deflagration simulations leaving bound remnants: a model for 2002cx-like Type Ia supernovae★

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MODELING THE POLLUTION OF PRISTINE GAS IN THE EARLY UNIVERSE

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Treating Unresolvable Flame Physics in Simulations of Thermonuclear Supernovae

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Recovery from Population III supernova explosions and the onset of second-generation star formation

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Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae

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GRAVITATIONALLY UNSTABLE FLAMES: RAYLEIGH-TAYLOR STRETCHING VERSUS TURBULENT WRINKLING

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Three‐Dimensional Simulations of the Deflagration Phase of the Gravitationally Confined Detonation Model of Type Ia Supernovae

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The Astrophysical Journal 681 (2) 1448 (2008)
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A semi-analytic model of the turbulent multi-phase interstellar medium

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Three-dimensional simulations of gravitationally confined detonations compared to observations of SN 1991T

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Carbon Detonation Initiation in Turbulent Electron-degenerate Matter

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A subgrid-scale model for deflagration-to-detonation transitions in Type Ia supernova explosion simulations

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Pulsating instability and self-acceleration of fast turbulent flames

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A new hydrodynamics code for Type Ia supernovae

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Large Eddy Simulations in Astrophysics

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Rapid filamentary accretion as the origin of extended thin discs

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A modified optimal LES model for highly compressible isotropic turbulence

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Constraining the Single-degenerate Channel of Type Ia Supernovae with Stable Iron-group Elements in SNR 3C 397

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Rayleigh–Taylor unstable flames at higher Reynolds number

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EVALUATING SYSTEMATIC DEPENDENCIES OF TYPE Ia SUPERNOVAE: THE INFLUENCE OF CENTRAL DENSITY

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A fluid-dynamical subgrid scale model for highly compressible astrophysical turbulence

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EVOLUTION OF SHOCKS AND TURBULENCE IN MAJOR CLUSTER MERGERS

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POWER-LAW WRINKLING TURBULENCE-FLAME INTERACTION MODEL FOR ASTROPHYSICAL FLAMES

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The Astrophysical Journal 784 (2) 174 (2014)
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A Three‐Dimensional Deflagration Model for Type Ia Supernovae Compared with Observations

F. K. Ropke, W. Hillebrandt, W. Schmidt, et al.
The Astrophysical Journal 668 (2) 1132 (2007)
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The Astrophysical Journal 704 (1) 255 (2009)
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Type Ia supernova diversity: white dwarf central density as a secondary parameter in three-dimensional delayed detonation models

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Large-Scale Structure Formation: From the First Non-linear Objects to Massive Galaxy Clusters

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Hydrodynamical adaptive mesh refinement simulations of turbulent flows - I. Substructure in a wind

L. Iapichino, J. Adamek, W. Schmidt and J. C. Niemeyer
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Viscosity, pressure and support of the gas in simulations of merging cool-core clusters

W. Schmidt, C. Byrohl, J. F. Engels, C. Behrens and J. C. Niemeyer
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On the applicability of the level set method beyond the flamelet regime in thermonuclear supernova simulations

W. Schmidt
Astronomy & Astrophysics 465 (1) 263 (2007)
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Cosmological fluid mechanics with adaptively refined large eddy simulations

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Three-dimensional hydrodynamic simulations of the combustion of a neutron star into a quark star

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THREE-DIMENSIONAL SIMULATIONS OF PURE DEFLAGRATION MODELS FOR THERMONUCLEAR SUPERNOVAE

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FOLLOWING THE COSMIC EVOLUTION OF PRISTINE GAS. I. IMPLICATIONS FOR MILKY WAY HALO STARS

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Hydrodynamical adaptive mesh refinement simulations of turbulent flows - II. Cosmological simulations of galaxy clusters

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TURBULENCE IN A THREE-DIMENSIONAL DEFLAGRATION MODEL FOR TYPE Ia SUPERNOVAE. I. SCALING PROPERTIES

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On Simulating Type Ia Supernovae

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SUPERMASSIVE BLACK HOLE FORMATION AT HIGH REDSHIFTS VIA DIRECT COLLAPSE: PHYSICAL PROCESSES IN THE EARLY STAGE

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Large-scale simulations of buoyancy-driven turbulent nuclear burning

D M Townsley, R A Bair, A Dubey, et al.
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TYPE Ia SUPERNOVA EXPLOSIONS FROM HYBRID CARBON–OXYGEN–NEON WHITE DWARF PROGENITORS

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Off‐Center Ignition in Type Ia Supernovae. I. Initial Evolution and Implications for Delayed Detonation

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ADAPTIVELY REFINED LARGE EDDY SIMULATIONS OF A GALAXY CLUSTER: TURBULENCE MODELING AND THE PHYSICS OF THE INTRACLUSTER MEDIUM

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Combustion of a neutron star into a strange quark star: The neutrino signal

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THE DEFLAGRATION STAGE OF CHANDRASEKHAR MASS MODELS FOR TYPE Ia SUPERNOVAE. I. EARLY EVOLUTION

C. M. Malone, A. Nonaka, S. E. Woosley, et al.
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Turbulence in the ICM from mergers, cool-core sloshing, and jets: results from a new multi-scale filtering approach

F. Vazza, E. Roediger and M. Brüggen
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CARBON DEFLAGRATION IN TYPE Ia SUPERNOVA. I. CENTRALLY IGNITED MODELS

H. Ma, S. E. Woosley, C. M. Malone, A. Almgren and J. Bell
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Adaptive mesh refinement simulations of a galaxy cluster merger – I. Resolving and modelling the turbulent flow in the cluster outskirts

L. Iapichino, C. Federrath and R. S. Klessen
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STUDY OF THE DETONATION PHASE IN THE GRAVITATIONALLY CONFINED DETONATION MODEL OF TYPE Ia SUPERNOVAE

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The Astrophysical Journal 693 (2) 1188 (2009)
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Modeling and simulation of turbulent nuclear flames in Type Ia supernovae

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Modeling subgrid-scale force and divergence of heat flux of compressible isotropic turbulence by artificial neural network

Chenyue Xie, Ke Li, Chao Ma and Jianchun Wang
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Modelling turbulent effects of stellar feedback in cosmological simulations

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High Performance Computing in Science and Engineering, Garching/Munich 2007

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High Performance Computing in Science and Engineering, Garching/Munich 2007

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High Performance Computing in Science and Engineering, Garching/Munich 2009

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High Performance Computing in Science and Engineering, Garching/Munich 2009

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Interdisciplinary Aspects of Turbulence

F. Röpke and W. Schmidt
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Morphology of radio relics – I. What causes the substructure of synchrotron emission?

P Domínguez-Fernández, M Brüggen, F Vazza, et al.
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SN Ia Explosions from Hybrid Carbon–Oxygen–Neon White Dwarf Progenitors that Have Mixed during Cooling

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THE FORMATION OF MASSIVE POPULATION III STARS IN THE PRESENCE OF TURBULENCE

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Dynamic one-equation-based subgrid model for large-eddy simulation of stratified turbulent flows

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Amplification and generation of turbulence during self-gravitating collapse

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On the origin of surprisingly cold gas discs in galaxies at high redshift

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Radiative mixing layers: insights from turbulent combustion

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Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies

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