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.
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