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The study of QCD in the confinement regime poses some of the most difficult problems of fundamental physics at present. The mechanism of confinement is not yet understood, and it is hard to investigate the properties of the fundamental theory in the determination of the structures and interactions of hadronic systems. As a consequence of these difficulties, the frontier between effective and fundamental theories has been intensively investigated in the last few years, and progress has been achieved in several directions. The 'Hadron Physics' workshop gathered together experts who have been taking the lead in these developments in recent years. Four sets of lectures were presented, providing a pedagogical and updated basis that gives support to research work in frontier problems. This book puts together the main current methods in the study of the properties of hadrons. The perspective of future developments based on different approaches can then be more clearly perceived.
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Section-I: Solid State Physics| Section-Ii Electronics | Section-Iii: Nuclear And Particle Physics
Neutron stars are the collapsed cores of some massive stars. They pack roughly the mass of our Sun into a region the size of a city. Neutron stars are believed to form in supernovae such as the one that formed the Crab Nebula. The stars that eventually become neutron stars are thought to start out with about 15 to 30 times the mass of our sun. It appears that for initial masses much less than 15 solar masses the star becomes a white dwarf, whereas for initial masses a lot higher than 30 solar masses a black hole results instead. It is estimated that there are 108 neutron stars in our galaxy. About 1000 of these have actually been observed by astronomers so far. This new book presents recent and important research results in the field.
Neutron stars are the densest observable bodies in our universe. Born during the gravitational collapse of luminous stars - a birth heralded by spectacular supernova explosions - they open a window on a world where the state of the matter and the strengths of the fields are anything but ordinary. This book is a collection of pedagogical lectures on the theory of neutron stars, and especially their interiors, at the forefront of current research. It addresses graduate students and researchers alike, and should be particularly suitable as a text bridging the gap between standard textbook material and the research literature.