Muutke küpsiste eelistusi

E-raamat: Astrophysics with Radioactive Isotopes

Edited by , Edited by , Edited by
  • Formaat - EPUB+DRM
  • Hind: 135,23 €*
  • * hind on lõplik, st. muud allahindlused enam ei rakendu
  • Lisa ostukorvi
  • Lisa soovinimekirja
  • See e-raamat on mõeldud ainult isiklikuks kasutamiseks. E-raamatuid ei saa tagastada.

DRM piirangud

  • Kopeerimine (copy/paste):

    ei ole lubatud

  • Printimine:

    ei ole lubatud

  • Kasutamine:

    Digitaalõiguste kaitse (DRM)
    Kirjastus on väljastanud selle e-raamatu krüpteeritud kujul, mis tähendab, et selle lugemiseks peate installeerima spetsiaalse tarkvara. Samuti peate looma endale  Adobe ID Rohkem infot siin. E-raamatut saab lugeda 1 kasutaja ning alla laadida kuni 6'de seadmesse (kõik autoriseeritud sama Adobe ID-ga).

    Vajalik tarkvara
    Mobiilsetes seadmetes (telefon või tahvelarvuti) lugemiseks peate installeerima selle tasuta rakenduse: PocketBook Reader (iOS / Android)

    PC või Mac seadmes lugemiseks peate installima Adobe Digital Editionsi (Seeon tasuta rakendus spetsiaalselt e-raamatute lugemiseks. Seda ei tohi segamini ajada Adober Reader'iga, mis tõenäoliselt on juba teie arvutisse installeeritud )

    Seda e-raamatut ei saa lugeda Amazon Kindle's. 

Dealing with astrophysics derived from the radiation emitted by radioactive atomic nuclei, this book describes the different methods used to measure cosmic radio-isotopes. It demonstrates how this astronomical window has contributed to the understanding of the sources and the chemical evolution of cosmic gas. Reference materials and explanations are included for students in advanced stages of their education.

Nuclear reactions in different sites across the universe lead to the production of stable and unstable nuclei. Their abundances can be measured through different methods, allowing to study the various nuclear processes taking place in cosmic environments. Nucleosynthesis is the cosmic formation of new nuclear species, starting from hydrogen and helium resulting from the big bang origins. Stars create and eject synthesized nuclei during their evolution and explosions. Incorporation of the new interstellar composition into next-generation stars characterises the compositional (chemical) evolution of cosmic gas in and between galaxies. Radioactive species have unique messages about how this occurs.

Since the first Edition of this book published in 2011 with the title Astronomy with Radioactivities, long-awaited new direct observations of supernova radioactivity have been made and are now addressed in two updated chapters dealing with supernovae. In this second Edition, the advances of recent years beyond one-dimensional treatments of stellar structure and stellar explosions towards 3-dimensional models have been included, and led to significant re-writings in Chapters 3-5. The sections on the Solar System origins have been re-written to account for new insights into the evolution of giant molecular clouds. The chapter on diffuse radioactivities now also includes material measurements of radioactivities in the current solar system, and their interpretations for recent nucleosynthesis activity in our Galaxy. Significant new results on gamma-rays from positron annihilations have been accounted for in that chapter, and led to new links with nucleosynthesis sources as well as interstellar transport processes. A new chapter now provides a description of interstellar processes often called 'chemical evolution', thus linking the creation of new nuclei to their abundance observations in gas and stars. The experimental / instrumental chapters on nuclear reaction measurements, on gamma-ray telescopes, and pre-solar grain laboratories have been updated. Moreover, new windows of astronomy that have been opened up in recent years have been included in the discussions of the multi-messenger approach that broadens the basis for astrophysical insights.



This comprehensive and coherent book introduces the reader to the field of nuclear astrophysics. The authors explain the role of radioactivities in astrophysics, discuss specific sources of cosmic isotopes and in which special regions they can be observed.

Arvustused

The entire volume should surely find a place on a reading list for a graduate course on nucleosynthesis and related matters. Moreover, the volume under review deserves to be read by young and old astrophysicists. (David L. Lambert, The Observatory, Vol. 139 (1273), December, 2019)

Part I The Role of Radioactivities in Astrophysics
1 Astrophysics with Radioactive Isotopes
3(26)
Roland Diehl
1.1 Origin of Radioactivity
3(6)
1.2 Processes of Radioactivity
9(7)
1.3 Radioactivity and Cosmic Nucleosynthesis
16(4)
1.4 Observing Radioactive Isotopes in the Universe
20(9)
References
26(3)
2 The Role of Radioactive Isotopes in Astrophysics
29(62)
Donald D. Clayton
2.1 History of Nucleosynthesis and Radioactivity
30(13)
2.1.1 Two Very Different Pioneers
30(4)
2.1.2 The Second Decade
34(6)
2.1.3 New Astronomy with Radioactivity
40(1)
2.1.4 Interpreting Exponential Decay
41(2)
2.2 Disciplines of Astronomy with Radioactivity
43(48)
2.2.1 Nuclear Cosmochronology
43(13)
2.2.2 Gamma-Ray Lines from Galactic Radioactivity
56(8)
2.2.3 Radiogenic Luminosity
64(4)
2.2.4 Extinct Radioactivity and Immediate Pre-solar Nucleosynthesis
68(9)
2.2.5 Stardust: Radioactivity in Solid Samples of Pre-solar Stars
77(8)
References
85(6)
Part II Specific Sources of Cosmic Isotopes
3 Low- and Intermediate-Mass Stars
91(82)
Maria Lugaro
Alessandro Chieffi
3.1 The Missing Element
92(1)
3.2 The Production of Radioactive Nuclei in Stellar Interiors
92(12)
3.2.1 The Stellar Energy Source and Radioactive Isotopes
93(7)
3.2.2 The Sun: Neutrinos and the Nuclear Origin of Starlight
100(3)
3.2.3 Solar Flares and Radioactivities
103(1)
3.3 Evolution After the Main Sequence: The First Giant Branch
104(10)
3.3.1 The First Giant Branch
105(5)
3.3.2 The Production of Li
110(4)
3.4 Evolution in the Double Shell Burning Phase
114(13)
3.4.1 Asymptotic Giant Branch (AGB) Stars
115(7)
3.4.2 Super-AGB Stars
122(1)
3.4.3 Winds from AGB Stars
123(1)
3.4.4 Dust from Giant Stars and the Origin of Stardust
124(3)
3.5 Neutron Capture Nucleosynthesis in AGB Stars
127(18)
3.5.1 Neutron Sources in AGB Stars
127(4)
3.5.2 The eProcess in AGB Stars
131(5)
3.5.3 Branchings and the s-Process in AGB Stars
136(2)
3.5.4 Signatures of k-Process Branching Points: Rb, Zr, Eu
138(2)
3.5.5 SiC Grains from AGB Stars and Branching Points
140(4)
3.5.6 The Intermediate Neutron-Capture Process
144(1)
3.6 Nucleosynthesis of Long-Lived Isotopes in AGB Stars
145(14)
3.6.1 26Al
145(4)
3.6.2 Evidence of 26Al in AGB Stars
149(3)
3.6.3 60Fe
152(2)
3.6.4 36Cl and 41Ca
154(2)
3.6.5 Long-Lived Radioactive Isotopes Heavier than Fe
156(3)
3.7 Conclusions
159(14)
References
160(13)
4 Massive Stars and Their Supernovae
173(114)
Friedrich-Karl Thielemann
Roland Diehl
Alexander Heger
Raphael Hirschi
Matthias Liebendorfer
4.1 The Cosmic Significance of Massive Stars
174(3)
4.2 Hydrostatic and Explosive Burning
177(10)
4.2.1 Nuclear Burning During Hydrostatic Evolution
178(6)
4.2.2 Nuclear Burning During the Explosion
184(3)
4.3 Evolution up to Core Collapse
187(18)
4.3.1 Complexities of Post-Main-Sequence Evolution
188(12)
4.3.2 Late Burning Stages and the Onset of Core Collapse
200(5)
4.4 Core Collapse and Supernova Explosions
205(17)
4.4.1 Physics of Core Collapse, and Numerical Simulations
205(4)
4.4.2 Early Spherically-Symmetric Modeling
209(3)
4.4.3 Multi-D Simulations: A Short Survey
212(3)
4.4.4 Spherically-Symmetric Simulations, New Generation
215(7)
4.5 Exotic Explosions: Hypernovae, Gamma-Ray Bursts, Neutron Star Mergers
222(10)
4.5.1 Hypernovae/Long Duration Gamma-Ray Bursts/Collapsars
225(1)
4.5.2 MHD-Driven Supernovae/Magnetars
226(2)
4.5.3 Pair-Instability Supernovae (PISNe)
228(2)
4.5.4 Neutron Star Mergers
230(2)
4.6 Nucleosynthesis in Explosions from Massive Stars
232(18)
4.6.1 Nuclear Burning During Explosions
232(8)
4.6.2 Production of Long-Lived Radioactivities 44Ti, 26Al and 60Fe
240(4)
4.6.3 Explosive Burning Off the Regime of Nuclear Stability
244(6)
4.7 The Aftermath of Explosions
250(37)
4.7.1 Overall Nucleosynthesis Yields
250(2)
4.7.2 Spectroscopic Observations of Nucleosynthesis Products
252(6)
4.7.3 Radiogenic Luminosity and Late Lightcurves
258(4)
4.7.4 Material Deposits on Earth and Moon
262(2)
References
264(23)
5 Binary Systems and Their Nuclear Explosions
287(92)
Jordi Isern
Margarita Hernanz
Jordi Jose
5.1 Accretion onto Compact Objects and Thermonuclear Runaways
287(11)
5.1.1 Evolution of Degenerate Cores Before Ignition
289(2)
5.1.2 The Thermonuclear Runaway
291(2)
5.1.3 Physics of the Burning Front
293(3)
5.1.4 Scenarios Leading to a Thermonuclear Runaway
296(2)
5.2 Classical Novae
298(12)
5.2.1 Observational Properties
300(3)
5.2.2 Modeling Classical Novae
303(3)
5.2.3 Nucleosynthesis in Classical Novae
306(4)
5.3 SNIa Explosions
310(12)
5.3.1 Chandrasekhar-Mass Models
316(3)
5.3.2 Super-Chandrasekhar Models, Sub-Chandrasekhar, and White Dwarf-White Dwarf Collisions
319(2)
5.3.3 Nucleosynthesis in Thermonuclear Supernovae
321(1)
5.4 X-ray Bursts and Superbursts
322(11)
5.4.1 The Nature of Type I X-ray Bursts
324(3)
5.4.2 Modeling X-ray Bursts
327(1)
5.4.3 Nucleosynthesis in Type I X-ray Bursts
328(3)
5.4.4 Superbursts
331(2)
5.5 Observational Diagnostics of Binary-Systems
333(18)
5.5.1 Gamma-Rays from Radioactivity
333(12)
5.5.2 Dust from Novae and Thermonuclear Supernovae
345(6)
5.6 Accretion in Binaries: Special Cases
351(28)
References
354(25)
Part III Special Places to Observe Cosmic Isotopes
6 The Early Solar System
379(48)
Maurizio Busso
6.1 The Age of the Solar System
380(4)
6.1.1 The Beginnings
380(1)
6.1.2 Long-Lived Nuclei for Solar System Dating
381(3)
6.2 Short-Lived Radioactive Nuclei in the ESS
384(6)
6.3 The Galactic Inheritance
390(4)
6.4 Expected Conditions in the ESS and Its Environment
394(6)
6.4.1 Processes in Star-Forming Clouds and Protostellar Disks
395(2)
6.4.2 Local Contamination, I: An Individual Star?
397(1)
6.4.3 Local Contamination, II: Sequential Episodes in a Molecular Cloud?
398(2)
6.5 Arguments Left for a Single Close Stellar Encounter?
400(10)
6.5.1 Short-Lived Nuclei: A Late Supernova Origin?
401(5)
6.5.2 Contributions from a Nearby AGB Star?
406(4)
6.6 Short-Lived Nuclei: Production Inside the ESS
410(3)
6.6.1 Radioactivities from the Bombardment of Early Solids
410(1)
6.6.2 Solar Activity and the Production of 7Be
411(2)
6.7 Lessons from the Early Solar System
413(14)
References
415(12)
7 Distributed Radioactivities
427(74)
Roland Diehl
Dieter H. Hartmann
Nikos Prantzos
7.1 Radioactivities in the Interstellar Medium
427(4)
7.2 26Al
431(24)
7.2.1 Nuclear Reactions, Candidate Sources, and Observability
431(4)
7.2.2 Observations of 26Al
435(2)
7.2.3 26Al Throughout the Galaxy
437(7)
7.2.4 26Al from Specific Regions
444(11)
7.3 60Fe
455(7)
7.3.1 Nuclear Reactions, Candidate Sources, and Observability
455(2)
7.3.2 Observations Throughout the Galaxy
457(2)
7.3.3 Observations of 60Fe in Solar-System Material
459(3)
7.4 Radioactivities in Cosmic Rays
462(10)
7.4.1 Sources, Acceleration, and Propagation of Cosmic Rays
462(4)
7.4.2 Observations of Cosmic Rays
466(6)
7.5 Positrons and Their Annihilation
472(29)
7.5.1 Candidate Sources and Expected Observables
473(4)
7.5.2 Observations of Positrons
477(10)
7.5.3 Assessment of Candidate Positron Sources
487(6)
References
493(8)
Part IV Tools for the Study of Radioactivities in Astrophysics
8 Computer-Modeling of Stars
501(22)
Matthias Liebendorfer
8.1 Models of Core-Collapse Supernovae
505(11)
8.1.1 Basic Physical Description
505(1)
8.1.2 Basic Mathematical Description
506(2)
8.1.3 Scales and Challenges
508(3)
8.1.4 Solution Strategies
511(5)
8.2 Models of Ejecta for Nucleosynthetic Yield Prediction
516(7)
8.2.1 The Dynamics of the Ejection Process
516(1)
8.2.2 The Thermodynamic Conditions of the Ejecta
517(1)
8.2.3 The Exposure of the Ejecta to Neutrinos
518(1)
References
519(4)
9 Nuclear Reactions
523(32)
Michael Wiescher
Thomas Rauscher
9.1 Nuclear Reactions in Astrophysical Environments
524(7)
9.1.1 Reaction Networks and Thermonuclear Reaction Rates
525(5)
9.1.2 Reaction Equilibria
530(1)
9.2 Relevant Energy Range of Astrophysical Cross Sections
531(2)
9.3 Nuclear Reaction Models
533(5)
9.3.1 Resonance and Potential Models
533(4)
9.3.2 Statistical Model
537(1)
9.4 Experimental Facilities and Techniques
538(9)
9.4.1 Low-Energy Facilities, Underground Techniques
539(3)
9.4.2 Laboratory Neutron Sources
542(2)
9.4.3 Accelerator Mass Spectroscopy
544(1)
9.4.4 Radioactive Beam Techniques
545(2)
9.5 Specific Experiments
547(8)
9.5.1 Experiments with Stable Beams
547(2)
9.5.2 Experiments with Neutron Beams
549(1)
9.5.3 Experiments with Radioactive Beams or Targets
550(2)
References
552(3)
10 Instruments for Observations of Radioactivities
555(26)
Gottfried Kanbach
Larry Nittler
10.1 Astronomical Telescopes
556(10)
10.1.1 Measuring Radiation from Cosmic Radioactivity
556(3)
10.1.2 Photon Collectors
559(1)
10.1.3 Imaging Instruments
560(2)
10.1.4 Current Spectrometry and Imaging: INTEGRAL/SPI, NuSTAR, and COSI
562(2)
10.1.5 Perspectives of Cosmic Gamma-Ray Imaging and Spectroscopy
564(2)
10.2 Analyzing Material Samples from and Within Meteorites
566(8)
10.2.1 Measurement Principles and Techniques
566(3)
10.2.2 Bulk Techniques
569(2)
10.2.3 In Situ Techniques
571(2)
10.2.4 Perspectives for Astronomy with Meteorite Samples
573(1)
10.3 Detection and Analysis of Cosmic Rays
574(7)
10.3.1 Ground-Based Observations
575(1)
10.3.2 High-Altitude and Space-Based Observations
575(3)
References
578(3)
11 Cosmic Evolution of Isotopic Abundances: Basics
581(62)
Roland Diehl
Nikos Prantzos
11.1 Modeling Compositional Evolution of Cosmic Gas
581(30)
11.1.1 The Concept and Formalism
583(4)
11.1.2 The Role of Stars
587(14)
11.1.3 The Roles of Gas and Dust
601(10)
11.2 The Milky Way Galaxy
611(13)
11.2.1 Stellar Populations
611(2)
11.2.2 Supernova Rates in the Galaxy
613(3)
11.2.3 Interstellar Matter
616(1)
11.2.4 Spiral Arm Structures
617(2)
11.2.5 Interstellar Magnetic Fields
619(3)
11.2.6 Dark Matter
622(2)
11.3 Applications and the Solar Neighborhood
624(19)
11.3.1 Chemical Evolution of the Local Disk
624(1)
11.3.2 Observables
625(1)
11.3.3 The Local Metallicity Distribution in Stars
626(4)
11.3.4 A Brief History of the Solar Neighbourhood
630(4)
References
634(9)
12 Branching Points on the Path of the Slow Neutron-Capture Process
643(12)
Maria Lugaro
Alessandro Chieffi
References
650(5)
Part V Epilogue
13 Perspectives
655(6)
Roland Diehl
Dieter H. Hartmann
Nikos Prantzos
A Science of Cosmic Radioactivities: Milestones 661(4)
B Glossary 665(8)
Index 673
Roland Diehl is research scientist at the Max Planck Institut für extraterrestrische Physik (MPE). He holds a doctoral degree in physics from the Technische Universität München (1988) and is Professor (apl.) in the Physics Department at the Technische Universität München. He started his career from nuclear physics, joining the staff of the gamma-ray astronomy group at MPE in 1979. Experimental nuclear physics determined his early work. This evolved into taking part in development of pioneering telescopes for the MeV regime of astronomy at MPE, specifically the COMPTEL telescope, which was operated 1991-2000 in space aboard NASA's Compton Gamma-Ray Observatory, and the SPI imaging spectrometer aboard ESA's INTEGRAL satellite observatory launched in 2002 and operating successfully since. After leading the calibrations of the COMPTEL telescope, he has been guiding different teams to advance analysis methods required for these complex measurements with gamma-ray telescopes, which involved telescope projects COMPTEL, INTEGRAL/SPI, GRIPS, and eAstrogam. He is Co-Principal Investigator of the INTEGRAL SPI telescope, and head of MPEs science team on cosmic gamma-ray spectroscopy. He has been member of several international and national science advisory boards, and of the Senate of the Max-Planck Society. His astrophysical interest is centered on nuclear astrophysics, interpreting gamma-ray line measurements in their context of nucleosynthesis in stars and supernovae, and related cosmic ray physics. He pioneered the imaging of the sky in the radioactive-decay gamma-ray line from 26Al, and is currently involved in studies of supernovae, massive stars, novae, and how these energise and shape the interstellar medium, employing a broad range of astronomical measurements.





Dieter H. Hartmann is a Professor of Astrophysics on the faculty of the Department of Physics and Astronomy at Clemson University, South Carolina, USA. He holds a Ph.D. from the Universityof California Santa Cruz (1989). He had studied Physics Engineering in Lübeck / Germany, then found his interest in astrophysics at the Gauss Observatory in Göttingen, where he obtained his Diploma (1982) on the nuclear equation of state of supernova matter. Studies of nucleosynthesis in neutron-rich environments to explain isotopic anomalies in meteorites, and -ray properties of core-collapse supernovae continued this early work. Gamma Ray Bursts (GRBs) and their afterglows were subject of his Ph.D. time under the mentorship of Prof. S. E. Woosley, whereafter a postdoctoral research position at the Lawrence Livermore National Laboratory focused on galactic dynamics and GRB counterparts. Since 1991 he pursued nuclear and -ray astrophysics in the group of Prof. Donald D. Clayton at Clemson University. He worked as member of the LOTIS Team (GRB counterparts), and then in the Compton Gamma Ray Observatory (CGRO) Team for many years, including many summer visits working with the gamma-ray group at the MPE. He has been member of the User Groups of NASA's Swift- and Fermi-missions, as well as ESAs INTEGRAL User Group, and also serves as a Scientific Editor of The Astrophysical Journal, and in committees such as the Astronomy and Astrophysics Advisory Committee and NASAs roadmap study "Enduring Quests - Daring Visions". His current research includes the general area of Time Domain Astrophysics, with a focus on explosive phenomena (novae, supernovae, GRBs) and their use as cosmic probes for galactic and cosmic chemical evolution.





Nikos Prantzos is Director of research in the Paris Institute of Astrophysics. He holds a PhD in nuclear astrophysics from Paris VII University (1986). His main scientific interests are on stellar evolution and nucleosynthesis, with an emphasis on galactic chemical evolution and high energy astrophysics, in particular gamma-ray line astronomy and the composition of galactic cosmic rays. He coordinated various international teams doingtheoretical work on these topics, and on interpretations of the variety of astronomical observations, including high-energy data on gamma rays and cosmic rays. He served as member of the time allocation committee of ESAs gamma-ray satellite INTEGRAL. He was representative of Greece in the Board of Directors of the European journal "Astronomy and Astrophysics" and he served as member of the Councils of the Greek Astronomical Society, the French Astronomical Society and the French Society of Physics. He was awarded the annual distinction of the French Astronomical Society in 1994. He is also author of science popularisation books, which have been translated into several other languages.