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Supernovae, neutron star physics and nucleosynthesis

Record Type:	Electronic resources : Monograph/item
Title/Author:	Supernovae, neutron star physics and nucleosynthesisby Debades Bandyopadhyay, Kamales Kar.
Author:	Bandyopadhyay, Debades.
other author:	Kar, Kamales.
Published:	Cham :Springer International Publishing :2022.
Description:	xvii, 207 p. :ill. (some col.), digital ;24 cm.
Contained By:	Springer Nature eBook
Subject:	Supernovae.
Online resource:	https://doi.org/10.1007/978-3-030-95171-9
ISBN:	9783030951719$q(electronic bk.)

Supernovae, neutron star physics and nucleosynthesis
Bandyopadhyay, Debades.

Supernovae, neutron star physics and nucleosynthesis[electronic resource] /by Debades Bandyopadhyay, Kamales Kar. - Cham :Springer International Publishing :2022. - xvii, 207 p. :ill. (some col.), digital ;24 cm. - Astronomy and astrophysics library,2196-9698. - Astronomy and astrophysics library..

1. Introduction -- 2. Theory of Supernova Explosions -- 3. Neutron Stars -- 4. Binary Neutron Star Mergers -- 5. Synthesis of Heavy Elements in the Universe.

This book deals with the interdisciplinary areas of nuclear physics, supernovae and neutron star physics. It addresses the physics and astrophysics of the spectacular supernova explosions, starting with the collapse of massive stars and ending with the birth of neutron stars or black holes. Recent progress in the understanding of core collapse supernova (CCSN) and observational aspects of future detections of neutrinos from CCSN explosions are discussed. The other main focus in this text is the novel phases of dense nuclear matter, its compositions and equation of state (EoS) from low to very high baryon density relevant to supernovae and neutron stars. The multi-messenger astrophysics of binary neutron star merger GW170817 and its relation to EoS through tidal deformability are also presented in detail. The synthesis of elements heavier than iron in the supernova and neutron star environment by the rapid (r)-process are treated here with special emphasis on the nucleosynthesis in the ejected material from GW170817. This monograph is written for graduate students and researchers in the field of nuclear astrophysics.

ISBN: 9783030951719$q(electronic bk.)

Standard No.: 10.1007/978-3-030-95171-9doiSubjects--Topical Terms:

266973
Supernovae.

LC Class. No.: QB843.S95 / B35 2022

Dewey Class. No.: 523.84465

Supernovae, neutron star physics and nucleosynthesis
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300 $a xvii, 207 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Astronomy and astrophysics library, $x 2196-9698
505 0 $a 1. Introduction -- 2. Theory of Supernova Explosions -- 3. Neutron Stars -- 4. Binary Neutron Star Mergers -- 5. Synthesis of Heavy Elements in the Universe.
520 $a This book deals with the interdisciplinary areas of nuclear physics, supernovae and neutron star physics. It addresses the physics and astrophysics of the spectacular supernova explosions, starting with the collapse of massive stars and ending with the birth of neutron stars or black holes. Recent progress in the understanding of core collapse supernova (CCSN) and observational aspects of future detections of neutrinos from CCSN explosions are discussed. The other main focus in this text is the novel phases of dense nuclear matter, its compositions and equation of state (EoS) from low to very high baryon density relevant to supernovae and neutron stars. The multi-messenger astrophysics of binary neutron star merger GW170817 and its relation to EoS through tidal deformability are also presented in detail. The synthesis of elements heavier than iron in the supernova and neutron star environment by the rapid (r)-process are treated here with special emphasis on the nucleosynthesis in the ejected material from GW170817. This monograph is written for graduate students and researchers in the field of nuclear astrophysics.
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