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Introduces the physics behind single and binary stellar evolution, assuming no prior knowledge of astronomy
Focuses on the evolution of stars to the end point of white dwarf, neutron star, and black hole binary systems
Fills the niche between more-and-less advanced books, currently available on the topic
An Introduction to the Evolution of Single and Binary Stars provides physicists with an understanding of binary and single star evolution, beginning with a background and introduction of basic astronomical concepts. Although a general treatment of stellar structure and evolution is included, the text stresses the physical processes that lead to stellar mass compact object binaries that may be sources of observable gravitational radiation.
Basic concepts of astronomy, stellar structure and atmospheres, single star evolution, binary systems and mass transfer, compact objects, and dynamical systems are covered in the text. Readers will understand the astrophysics behind the populations of compact object binary systems and have sufficient background to delve deeper into specific areas of interest. In addition, derivations of important concepts and worked examples are included. No previous knowledge of astronomy is assumed, although a familiarity with undergraduate quantum mechanics, classical mechanics, and thermodynamics is beneficial.
Content Level »Upper undergraduate
Keywords »compact binaries - evolution of stars - single and binary stars - star cluster dynamics - star formation - stellar birth - stellar evolution - stellar evolution explained - undergraduate text