'Nuclear burning' presentation slideshows

Reaction Rates

Reaction Rates. Marialuisa Aliotta. School of Physics University of Edinburgh. principles of stellar structure and evolution general features of thermonuclear reactions experimental approach. Second European Summer School on Experimental Nuclear Astrophysics

569 views • 48 slides

Nuclear-burning white dwarfs: Type Ia supernova progenitors?

Nuclear-burning white dwarfs: Type Ia supernova progenitors?. Theory and Observational Signatures. A tale in two parts: Rosanne Di Stefano and Jeno Sokoloski.

525 views • 43 slides

Superbursts: Nuclear Fury on Neutron Stars

Superbursts: Nuclear Fury on Neutron Stars. Sources of Thermonuclear Bursts: LMXBs Containing Neutron Stars. X-ray binaries near the Galactic center as seen with RXTE/PCA. Accreting neutron stars in low mass X-ray binaries. Roughly 70 burst sources known.

467 views • 30 slides

X-ray transients :

407 views • 28 slides

The Flash Code

The Flash Code. From Applications to Design. From Design to Applications. Tomek Plewa on behalf of almost countless contributors The ASCI Flash Center Dept. of Astronomy & Astrophysics The University of Chicago July 22, 2002. http://flash.uchicago.edu. What Is the Flash Center?.

366 views • 19 slides

FIVE REGIMES OF NUCLEAR BURNING IN DENSE STELLAR MATTER

FIVE REGIMES OF NUCLEAR BURNING IN DENSE STELLAR MATTER. D.G. Yakovlev. Ioffe Physical Technical Institute, St.-Petersburg, Russia. Physical conditions. Pycnonuclear burning. Thermonuclear burning. General outlook and applications. Screening in thermonuclear reactions. Summary.

318 views • 19 slides

9. Evolution of Massive Stars: Supernovae.

9. Evolution of Massive Stars: Supernovae. Evolution up to supernovae: the nuclear burning sequence; the iron catastrophe. Supernovae: photodisintigration; electron capture; neutron degeneracy. Nucleosynthesis in supernovae. 9.1 Evolution up to Supernovae.

192 views • 18 slides

171 views • 16 slides

ATON code for stellar evolution

254 views • 13 slides

nustarltech

117 views • 1 slides