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- Oneworld Publications 2014; US$ 14.99
Before the Higgs boson, there was a maddening search for another particle the ghostly neutrino. First detected in 1956, its fleeting appearances have teased answers to many mysteries: How did the Big Bang happen? Why is antimatter so rare? What might dark matter be made of? And could faster-than-light travel be possible, overturning Einstein?s theory... more...
- Elsevier Science 2013; US$ 31.95
Introduction to Stellar Statistics discusses the fundamental concepts that are essential in utilizing statistical methods in quantifying the variables present in celestial bodies. The title emphasizes detailing a conceptual system that aids in the organization of collected data. The text first introduces stellar statistics, and then proceeds to covering... more...
- Elsevier Science 2013; US$ 72.95
Plasma Astrophysics is a translation from the Russian language; the topics discussed are based on lectures given by V.N. Tsytovich at several universities. The book describes the physics of the various phenomena and their mathematical formulation connected with plasma astrophysics. This book also explains the theory of the interaction of fast particles... more...
- Springer International Publishing 2014; US$ 129.00
This prize-winning thesis deals with the observation and modeling of the spectral evolution of blazars. Based on single-dish light curves, a model of shock-shock interaction is tested and confirmed using multi-frequency high resolution Very Long Baseline Observations. He presents state-of-the art numerical relativistic hydrodynamic simulations and... more...
- Wiley 2015; US$ 103.95
Most elements are synthesized, or "cooked", by thermonuclear reactions in stars. The newly formed elements are released into the interstellar medium during a star's lifetime, and are subsequently incorporated into a new generation of stars, into the planets that form around the stars, and into the life forms that originate on the planets. Moreover,... more...
- Komplett Media GmbH 2011; US$ 5.60
Sterne werden seit 13 Milliarden Jahren kontinuierlich in Molekülwolken durch Gravitationsinstabilitäten geboren. Wenn im Inneren dieser kollabierenden Gaskugeln Druck und Temperatur hoch genug sind, setzt Energieproduktion durch Kernfusion ein - das normale Leben der Sterne beginnt. Je größer die Sterne sind, desto kürzer leben sie. Wenn durch Fusion... more...
- De Gruyter 2015; US$ 112.00
Astroparticle physics employs a range of theories to model the sources of cosmic radiation ? but until now, it has not fully captured the relevant connections between these theories. Using Scheibe?s method for the reconstruction and reduction of physical theories, Raphael Bolinger demonstrates the uses and limitations of formal strategies... more...
- Springer Berlin Heidelberg 2006; US$ 109.00
This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale... more...