Cauldrons in the Cosmos: Nuclear Astrophysics
University of Chicago Press, 1988 - 561 من الصفحات
Nuclear astrophysics is, in essence, a science that attempts to understand and explain the physical universe beyond the Earth by studying its smallest particles. Cauldrons in the Cosmos, by Claus E. Rolfs and William S. Rodney, serves as a basic introduction to these endeavors. From the major discoveries in the field to a discussion of the makeup of stars to an explanation of standard lab techniques, this text provides students and scientists alike a thorough and fascinating survey of the accomplishments, goals, and methods of nuclear astrophysics. A classic in its field, Cauldrons in the Cosmos will surely remain an important reference in nuclear astrophysics for years to come.
"One could not wish for a better account of the current state of knowledge (and uncertainty) about nuclear reactions in stars."—B. E. J. Pagel, Nature
"Written in an informal style that those uninitiated into the jargon of nuclear astrophysics and astronomy will find readable and illuminating. . . . A useful and long-awaited introduction to nuclear astrophysics."—G. J. Mathews, Science
ما يقوله الناس - كتابة مراجعة
لم نعثر على أي مراجعات في الأماكن المعتادة.
AstronomyObserving the Universe
AstrophysicsExplaining the Universe
Definitions and General Characteristics
Determination of Stellar Reaction Rates
Laboratory Equipment and Techniques
Advanced and Explosive Burning
طبعات أخرى - عرض جميع المقتطفات
a-particles abundances accelerator angular astronomers astrophysics atoms baryon beam energy big bang calculations capture reaction chap CNO cycles collapse compound nucleus core cosmic Coulomb barrier cross section cycle decay density detection detector determined distribution effects electrons elements emitted energy dependence equation equilibrium evolution example excited experimental factor function galaxies Gamow gas target gravitational helium hydrogen burning interaction interstellar involved ion beam ion source ionization isotopes lifetime luminosity magnetic field mass massive stars material matter measurements nebulae neutrinos neutron capture neutron star nuclear reactions nuclei nucleosynthesis observed p-p chain partial width photodisintegration pressure production projectile protons pulse quasars r-process radiation radioactive radius range ratio reaction rate red giant region relative resonance result shown in Figure solar system stable stellar evolution stellar temperature supernova surface synthesis telescope thermal tion velocity voltage white dwarfs Wien filter y-ray yield