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This book summarizes the recent progress in the physics and astrophysics of neutron stars. It provides an overview of neutron star formation in supernovae, pulsars, equations of state of neutron stars, super dense matter, gravitational wave emission and alternative theories of gravity.
- Neutron Stars 1: Equation of State and Structure | SpringerLink
Neutron stars play a unique role in physics and...
- Neutron Stars 1: Equation of State and Structure | SpringerLink
publications devoted to neutron stars, and is designed first and foremost to present the author’s personal view of the problem. Fundamentals of neutron star physics are expounded in the excellent textbook by Shapiro and Teukolsky [24]. More detailed descriptions of develop-ments in selected branches of neutron star astrophysics
1 Μαΐ 2004 · Neutron stars are some of the densest manifestations of massive objects in the universe. They are ideal astrophysical laboratories for testing theories of dense matter physics and provide...
covers the astrophysical context where neutron stars are formed (core-collapse supernovae), discusses the impact of strong magnetic fields in neutron stars (mag-netars and transient phenomena),reviews tests of gravity with compact stars and the detection of gravitational waves, and studies the complexity of binary systems.
1 Ιαν 2017 · The main purpose of this book is to investigate processes, phenomena and reactions in neutron star physics with fundamental interactions described in a self-consistent manner to highlight...
Neutron stars play a unique role in physics and astrophysics. On the one hand, they contain matter under extreme physical conditions, and their theories are based on risky and far extrapolations of what we consider reliable physical theories of the structure of matter tested in laboratory.
When the existence of neutron stars was confirmed by the discovery of radio pul-sars in August 1967, there was general optimism that it should not be too difficult to explore and understand the physical properties of a rotating magnetised compact star with ∼10 km radius.
