001445670 000__ 03480cam\a2200577Ii\4500
001445670 001__ 1445670
001445670 003__ OCoLC
001445670 005__ 20230310003843.0
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001445670 007__ cr\un\nnnunnun
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001445670 019__ $$a1306527893$$a1308393323$$a1308798706
001445670 020__ $$a9783030951719$$q(electronic bk.)
001445670 020__ $$a3030951715$$q(electronic bk.)
001445670 020__ $$z9783030951702$$q(print)
001445670 020__ $$z3030951707
001445670 0247_ $$a10.1007/978-3-030-95171-9$$2doi
001445670 035__ $$aSP(OCoLC)1308977106
001445670 040__ $$aGW5XE$$beng$$erda$$epn$$cGW5XE$$dEBLCP$$dOCLCO$$dYDX$$dOCLCF$$dN$T$$dUKAHL$$dOCLCQ
001445670 049__ $$aISEA
001445670 050_4 $$aQB843.S95
001445670 08204 $$a523.8/4465$$223
001445670 1001_ $$aBandyopadhyay, Debades,$$eauthor.$$0(orcid)0000-0003-0616-4367$$1https://orcid.org/0000-0003-0616-4367
001445670 24510 $$aSupernovae, neutron star physics and nucleosynthesis /$$cDebades Bandyopadhyay, Kamales Kar.
001445670 264_1 $$aCham, Switzerland :$$bSpringer,$$c2022.
001445670 300__ $$a1 online resource (xvii, 207 pages) :$$billustrations (some color).
001445670 336__ $$atext$$btxt$$2rdacontent
001445670 337__ $$acomputer$$bc$$2rdamedia
001445670 338__ $$aonline resource$$bcr$$2rdacarrier
001445670 4901_ $$aAstronomy and astrophysics library,$$x2196-9698
001445670 504__ $$aIncludes bibliographical references and index.
001445670 5050_ $$a1. Introduction -- 2. Theory of Supernova Explosions -- 3. Neutron Stars -- 4. Binary Neutron Star Mergers -- 5. Synthesis of Heavy Elements in the Universe.
001445670 506__ $$aAccess limited to authorized users.
001445670 520__ $$aThis book deals with the interdisciplinary areas of nuclear physics, supernovae and neutron star physics. It addresses the physics and astrophysics of the spectacular supernova explosions, starting with the collapse of massive stars and ending with the birth of neutron stars or black holes. Recent progress in the understanding of core collapse supernova (CCSN) and observational aspects of future detections of neutrinos from CCSN explosions are discussed. The other main focus in this text is the novel phases of dense nuclear matter, its compositions and equation of state (EoS) from low to very high baryon density relevant to supernovae and neutron stars. The multi-messenger astrophysics of binary neutron star merger GW170817 and its relation to EoS through tidal deformability are also presented in detail. The synthesis of elements heavier than iron in the supernova and neutron star environment by the rapid (r)-process are treated here with special emphasis on the nucleosynthesis in the ejected material from GW170817. This monograph is written for graduate students and researchers in the field of nuclear astrophysics.
001445670 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed April 5, 2022).
001445670 650_0 $$aSupernovae.
001445670 650_0 $$aNeutron stars.
001445670 650_0 $$aAstrophysics.
001445670 650_6 $$aSupernovae.
001445670 650_6 $$aÉtoiles à neutrons.
001445670 650_6 $$aAstrophysique.
001445670 655_0 $$aElectronic books.
001445670 7001_ $$aKar, Kamales,$$eauthor.$$0(orcid)0000-0002-3313-2072$$1https://orcid.org/0000-0002-3313-2072
001445670 77608 $$iPrint version:$$z3030951707$$z9783030951702$$w(OCoLC)1289366368
001445670 830_0 $$aAstronomy and astrophysics library,$$x2196-9698
001445670 852__ $$bebk
001445670 85640 $$3Springer Nature$$uhttps://univsouthin.idm.oclc.org/login?url=https://link.springer.com/10.1007/978-3-030-95171-9$$zOnline Access$$91397441.1
001445670 909CO $$ooai:library.usi.edu:1445670$$pGLOBAL_SET
001445670 980__ $$aBIB
001445670 980__ $$aEBOOK
001445670 982__ $$aEbook
001445670 983__ $$aOnline
001445670 994__ $$a92$$bISE