MARC Record from marc_columbia

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001 15130597
005 20220627133323.0
006 m o d
007 cr |n|---|||||
008 180217s2018 xx o 000 0 eng d
035 $a(OCoLC)on1023550503
035 $a(NNC)15130597
040 $aEBLCP$beng$epn$cEBLCP$dCRCPR$dCOO$dYDX$dN$T$dCNCGM$dOCLCF$dNLE$dOCLCQ$dOCLCO$dMERER$dQCL$dOCLCQ$dEZ9$dU3W$dOCLCQ$dOTZ$dTYFRS$dOCLCQ$dS2H$dOCLCO$dUKAHL$dOCLCQ$dOCLCO
019 $a1023612923
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020 $z1138588164
020 $z9781138588165
035 $a(OCoLC)1023550503$z(OCoLC)1023612923
050 4 $aQB464
072 7 $aSCI$x004000$2bisacsh
082 14 $aSCPC19
049 $aZCUA
100 1 $aKhan, Md A.
245 10 $aNuclear Astrophysics :$ba Course of Lectures.
260 $aMilton :$bCRC Press,$c2018.
300 $a1 online resource (220 pages)
336 $atext$btxt$2rdacontent
337 $acomputer$bc$2rdamedia
338 $aonline resource$bcr$2rdacarrier
588 0 $aPrint version record.
505 0 $aIntro; Halftitle; Title Page; Copyright Page; Table of Contents; 1 Basics of Nuclear Astrophysics; 1.1 Introduction; 1.2 Nuclear Physics; 1.2.1 Branching of Radioactivity; 1.2.2 Binding energy; 1.2.3 Nuclear Reactions; 1.2.4 Reaction Qâ#x80;#x90;value; 1.2.5 α decay; 1.2.6 βâ#x80;#x90;decay and electron capture; 1.2.7 γâ#x80;#x90;decay; 1.2.8 Nuclear fusion; 1.2.9 The Coulomb barrier; 1.2.10 Reaction rate in a medium; 1.2.11 Compound nuclear hypothesis; 1.2.12 Breit-Wigners one-level formula; 1.2.13 Crossâ#x80;#x90;sections and their derivations; 1.3 Particle physics; 1.4 Astrophysics; 1.5 Scopes of nuclear astrophysics.
505 8 $a2 Nucleosynthesis2.1 Introduction; 2.2 Primordial nucleosynthesis; 2.3 Stellar nucleosynthesis up to iron (A â#x89;Þ 60); 2.4 Stellar nucleosynthesis beyond iron; 3 Sources of Energy in Stars; 3.1 Introduction; 3.2 Hydrogen burning and pâ#x80;#x90;p (protonâ#x80;#x90;proton) chain; 3.3 CNO Cycles; 3.4 The Hot CNO Cycle and the Rapid Proton Process; 3.5 The Early rpâ#x80;#x90;Process and Bottleneck Reactions; 3.6 Helium (4He) Burning; 3.7 TheTriple - αProcess; 3.8 Heavier Elementαâ#x80;#x90;Burning; 3.8.1 Neutron Production in (\alpha, n) Reactions; 3.9 The s and râ#x80;#x90;Neutron Processes.
505 8 $a4 Opportunities in Nuclear Astrophysics4.1 Introduction; 4.2 Thermonuclear rates and reaction networks; 4.2.1 Thermonuclear Reaction Rates; 4.2.2 Nuclear Reaction Networks; 4.2.3 Burning Processes in Stellar Environments; 4.3 Experimental Techniques in Nuclear Astrophysics; 4.3.1 Choice of Target; 4.3.2 Choice of detectors; 4.3.3 Recoil separators; 4.3.4 Ground State Properties; 4.3.5 Resonances Properties; 4.3.6 Transfer Reactions; 4.4 Experimental Nuclear Astrophysics; 4.4.1 Energy ranges for measurement of cross-sections; 4.4.2 Radioactive Beams; 4.4.3 In-Flight Separators.
505 8 $a4.5 Cross Section Predictions and Reaction Rates4.5.1 Thermonuclear Rates from Statistical Model Calculations; 4.5.2 Astrophysical S-factors of radiative capture reactions; 4.5.3 Sub-barrier fusion and selective resonant tunneling cross section; 4.6 Weak-Interaction Rates; 4.6.1 Electron Capture and β-Decay; 4.6.2 Neutrino-Induced Reactions; 5 Explosive Burning Processes; 5.1 Introduction; 5.2 Explosive Hâ#x80;#x90;Burning; 5.3 Explosive Heâ#x80;#x90;Burning; 5.4 Explosive C - and Neâ#x80;#x90;Burning; 5.5 Explosive â#x80;#x90;Burning; 5.6 Explosive Siâ#x80;#x90;Burning; 5.7 The â#x80;#x90;Process; 6 Core Collapse Supernovae.
505 8 $a6.1 Introduction6.2 General Scenario; 6.3 Role of weak-Interaction rates in presupernova evolution; 6.4 The Role of Electron Capture During Collapse; 6.5 Neutrino-Induced Processes During a Supernova Collapse; 6.6 Type II Supernovae Nucleosynthesis; 7 Basic Components Of Astrophysical râ#x80;#x90;Process; 7.1 Role of Nuclear Physics in the râ#x80;#x90;process; 7.2 Parameters controlling the râ#x80;#x90;process; 7.3 râ#x80;#x90;Process Sites; 7.3.1 Type II Supernovae; 7.3.2 Neutron Star Mergers; 7.3.3 râ#x80;#x90;Process Overview; 8 Nuclear processes in explosive binary stars; 8.1 Introduction; 8.2 Nova explosions; 8.3 X-ray bursts.
500 $a8.4 Thermonuclear runaway.
520 2 $a"In this volume the physics involved in various astrophysical processes like the synthesis of light and heavier elements, explosive burning processes, core collapse supernova etc have been critically addressed with minimum mathematical derivations so as to suit all faculties of the readers. For graduate students there are solved problems with exercises at the end of each chapter, for researchers some recent works on the calculation of physical parameters of astrophysical importance like the calculation of Sfactors at low energies have been included, and for amateur readers there are lot of history, information and discussion on the astronuclear phenomenon. Please note: Taylor & Francis does not sell or distribute the Hardback in India, Pakistan, Nepal, Bhutan, Bangladesh and Sri Lanka."--Provided by publisher.
650 0 $aNuclear astrophysics.
650 6 $aAstrophysique nucléaire.
650 7 $aSCIENCE$xAstronomy.$2bisacsh
650 7 $aNuclear astrophysics.$2fast$0(OCoLC)fst01039896
655 0 $aElectronic books.
655 4 $aElectronic books.
776 08 $iPrint version:$aKhan, Md A.$tNuclear Astrophysics : A Course of Lectures.$dMilton : CRC Press, ©2018$z9781138588165
856 40 $uhttp://www.columbia.edu/cgi-bin/cul/resolve?clio15130597$zTaylor & Francis eBooks
852 8 $blweb$hEBOOKS