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Related papers: Imploding ignition waves: I. one dimensional analy…

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The decay of a detonation wave from its initial CJ velocity to its final, steady state velocity upon encountering a finite thickness or diameter charge is investigated numerically and theoretically. The numerical simulations use an ideal…

Fluid Dynamics · Physics 2014-07-09 Jianling Li , XiaoCheng Mi , Andrew J. Higgins

When designing high-efficiency spark-ignition (SI) engines to operate at high compression ratios, one of the main issues that have to be addressed is detonation development from a pre-ignition front. In order to control this phenomenon, it…

Lipid interfaces not only compartmentalize but also connect different reaction centers within a cell architecture. These interfaces have well defined specific heats and compressibilities, hence energy can propagate along them analogous to…

Biological Physics · Physics 2018-11-19 Shamit Shrivastava

In this paper, we use large reaction networks to find ignition conditions of single-zone nuclear fuel with compositions typical of white dwarf (WD) matter. The necessary but, possibly not sufficient condition for initiation of detonation is…

Solar and Stellar Astrophysics · Physics 2020-04-06 Rahul Kashyap

We analyze the sensitivity of the flame propagation in a Chandrasekhar mass white dwarf to initial conditions during the subsonic burning phase, using 2D simulations of the full WD. Results are presented for a wide variety of initial flame…

Astrophysics · Physics 2009-11-11 Eli Livne , Shimon M. Asida , Peter Hoeflich

This paper investigates the initiation of a deflagration in a premixed boundary-layer stream by continuous heat deposition from a line energy source placed perpendicular to the flow on the wall surface, a planar flow configuration relevant…

Fluid Dynamics · Physics 2022-02-09 Mario Sanchez Sanz , Eduardo Fernandez Tarrazo , Antonio L. Sanchez

Double detonations of sub-Chandrasekhar-mass white dwarfs (WDs) in unstably mass-transferring double WD binaries have become one of the leading contenders to explain most Type Ia supernovae. However, past theoretical studies of the…

Solar and Stellar Astrophysics · Physics 2024-09-11 Ken J. Shen , Samuel J. Boos , Dean M. Townsley

The design of inertial confinement fusion (ICF) ignition targets requires radiation-hydrodynamics simulations with accurate models of the fundamental material properties (i.e., equation of state, opacity, and conductivity). Validation of…

We have studied double-detonation explosions in double-degenerate (DD) systems with different companion white dwarfs (WD) for modeling type Ia supernovae (SNe Ia) by means of high-resolution smoothed particle hydrodynamics (SPH)…

High Energy Astrophysical Phenomena · Physics 2019-11-26 Ataru Tanikawa , Ken'ichi Nomoto , Naohito Nakasato , Keiichi Maeda

We present a detonating failed deflagration model of Type Ia supernovae. In this model, the thermonuclear explosion of a massive white dwarf follows an off-center deflagration. We conduct a survey of asymmetric ignition configurations…

Astrophysics · Physics 2008-11-26 Tomasz Plewa

The thermonuclear explosion of a C/O white dwarf as a Type Ia supernova (SN Ia) generates a kinetic energy comparable to that released by a massive star during a SN II event. Current observations and theoretical models have established that…

High Energy Astrophysical Phenomena · Physics 2015-03-17 David Falta , Robert T. Fisher , Gaurav Khanna

Using 2D and 3D simulation, we study the "robustness" of the double detonation scenario for Type Ia supernovae, in which a detonation in the helium shell of a carbon-oxygen white dwarf induces a secondary detonation in the underlying core.…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Rainer Moll , Stanford E. Woosley

Ignition delay times of cyclopentene-oxygen-argon mixtures were measured behind reflected shock waves. Mixtures contained 0.5 or 1 % of hydrocarbons for equivalence ratios ranging from 0.5 to 1.5. Reflected shock waves conditions were:…

Detonations in helium-rich envelopes surrounding white dwarfs have garnered attention as triggers of faint thermonuclear ".Ia" supernovae and double detonation Type Ia supernovae. However, recent studies have found that the minimum size of…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Ken J. Shen , Kevin Moore

The interaction of a shock wave with a spherical density inhomogeneity leads to the development of a vortex ring through the impulsive deposition of baroclinic vorticity. The present fluid dynamics videos display this phenomenon and were…

Fluid Dynamics · Physics 2009-10-19 N. Haehn , C. Weber , J. Oakley , M. Anderson , D. Rothamer , R. Bonazza

High temperature radiating Air is produced experimentally by focusing a shock wave with the help of a spherically converging test section attached to a shock tube. The converging section concentrates the shock to a point with minimum…

Fluid Dynamics · Physics 2022-07-25 Saranyamol V. S. , Mohammed Ibrahim S

We use the Chandra X-ray Observatory to analyze interactions of the blast wave and the inhomogeneous interstellar medium on the western limb of the Cygnus Loop supernova remnant. This field of view includes an initial interaction between…

Astrophysics · Physics 2008-11-26 N. A. Levenson , J. R. Graham , J. L. Walters

Relativistic fluid dynamics and the theory of relativistic detonation fronts are used to estimate the space-time dynamics of the burning of the D-T fuel in Laser driven pellet fusion experiments. The initial "High foot" heating of the fuel…

Plasma Physics · Physics 2015-06-03 L. P. Csernai , D. D. Strottman

We discuss the results of 3D simulations of tidal disruptions of white dwarfs by moderate-mass black holes as they may exist in the cores of globular clusters or dwarf galaxies. Our simulations follow self-consistently the hydrodynamic and…

Astrophysics · Physics 2009-07-22 S. Rosswog , E. Ramirez-Ruiz , W. R. Hix

The present paper deals with the following hyperbolic--elliptic coupled system, modelling dynamics of a gas in presence of radiation, $u_{t}+ f(u)_{x} +Lq_{x}=0, -q_{xx} + Rq +G\cdot u_{x}=0,$ where $u\in\R^{n}$, $q\in\R$ and $R>0$, $G$,…

Analysis of PDEs · Mathematics 2019-07-25 Corrado Lattanzio , Corrado Mascia , Denis Serre
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