Add to ORKGWe discuss the challenges of modeling X-ray bursts in multi-dimensions, review the different calculations done to date, and discuss our new set of ongoing simulations. We also describe algorithmic improvements that may help in the future to offset some of the expense of these simulations, and describe what may be possible with exascale computing
Regular bursts have been observed in binary systems containing a neutron star with an accretion flow...
Type I X-ray bursts are thermonuclear explosions that occur in the envelopes of accreting neutron st...
We describe efforts to model the formation and evolution of X-ray clusters. After summarizing the cu...
We discuss the challenges of modeling X-ray bursts in multi-dimensions, review the different calcula...
We discuss the challenges of modeling X-ray bursts in multi-dimensions, review the different calcula...
We investigate the structure of laterally propagating flames through the highly stratified burning l...
Presentation at the TACC Workshop on Future Directions in Extreme Scale Computing for Scientific Gra...
AbstractGamma-ray bursts are a complex, non-linear system that evolves very rapidly through stages o...
Type I X-ray bursts are thermonuclear explosions on the surfaces of neutron stars that can be used t...
Type I X-ray bursts are thermonuclear burning events which occur on the surface of accreting neutron...
We continue to investigate two-dimensional laterally propagating flames in type I X-ray bursts using...
Type I X-ray Bursts (XRBs) are thermonuclear explosions of accreted mate-rial on the surfaces of a n...
Faculty Advisor: Professor Alexander HegerThe goal of my project was to develop an optimized linear ...
Regular X-ray bursts are the most prevalent thermonuclear stellar explosions observed in the Galaxy....
We perform the first detailed three-dimensional simulation of low Mach num-ber convection preceding ...
Regular bursts have been observed in binary systems containing a neutron star with an accretion flow...
Type I X-ray bursts are thermonuclear explosions that occur in the envelopes of accreting neutron st...
We describe efforts to model the formation and evolution of X-ray clusters. After summarizing the cu...
We discuss the challenges of modeling X-ray bursts in multi-dimensions, review the different calcula...
We discuss the challenges of modeling X-ray bursts in multi-dimensions, review the different calcula...
We investigate the structure of laterally propagating flames through the highly stratified burning l...
Presentation at the TACC Workshop on Future Directions in Extreme Scale Computing for Scientific Gra...
AbstractGamma-ray bursts are a complex, non-linear system that evolves very rapidly through stages o...
Type I X-ray bursts are thermonuclear explosions on the surfaces of neutron stars that can be used t...
Type I X-ray bursts are thermonuclear burning events which occur on the surface of accreting neutron...
We continue to investigate two-dimensional laterally propagating flames in type I X-ray bursts using...
Type I X-ray Bursts (XRBs) are thermonuclear explosions of accreted mate-rial on the surfaces of a n...
Faculty Advisor: Professor Alexander HegerThe goal of my project was to develop an optimized linear ...
Regular X-ray bursts are the most prevalent thermonuclear stellar explosions observed in the Galaxy....
We perform the first detailed three-dimensional simulation of low Mach num-ber convection preceding ...
Regular bursts have been observed in binary systems containing a neutron star with an accretion flow...
Type I X-ray bursts are thermonuclear explosions that occur in the envelopes of accreting neutron st...
We describe efforts to model the formation and evolution of X-ray clusters. After summarizing the cu...