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Titlebook: An Introduction to the Evolution of Single and Binary Stars; Matthew Benacquista Textbook 2013 Springer Science+Business Media New York 20

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期刊全称An Introduction to the Evolution of Single and Binary Stars
影响因子2023Matthew Benacquista
视频video
发行地址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 h
学科分类Undergraduate Lecture Notes in Physics
图书封面Titlebook: An Introduction to the Evolution of Single and Binary Stars;  Matthew Benacquista Textbook 2013 Springer Science+Business Media New York 20
影响因子.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.
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,Einleitung – zum Anliegen der Arbeit,is contained within ∼ 60 . of the radius. For lower-mass stars, this extends out to about 80 % of the radius. Naturally, the energy production is significantly higher in high-mass stars and extends out to larger radii.
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https://doi.org/10.1007/978-3-476-03840-1 baryon structure changes, altering their cooling process. Neutron stars are frequently born with high magnetic fields that slowly decay and spin down the neutron star. Black holes, however, will not change much for eons. In this chapter, we will look at the properties and continued evolution of these exotic objects.
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