The following is a list of over 1200 references for a wide range of topics in Nuclear Astrophysics. This list is meant to be complementary to the nuclear physics articles listed in the Nuclear Science References at the National Nuclear Data Center and to the astrophysics articles listed in NASA's NASA's Astrophysics Data System. The references are arranged alphabetically within subtopics, and the list of subtopics borrows heavily from the Wallerstein et al. review article and from other sources. Some references occur under multiple subtopics. The references were obtained from a variety of sources including the following:
Synthesis of Elements in Stars: 40 years of Progress, by G. Wallerstein et al., 1997, Reviews of Modern Physics 69, 995;
Solar Fusion Cross Sections, E.G. Adelberger et al., 1998, Reviews of Modern Physics 70, 1265;
Big-bang nucleosynthesis enters the precision era, D.N. Schramm and M.S. Turner, 1998, Reviews of Modern Physics 70, 303;
Experimental, Computational, and Observational Analysis of Primordial Nucleosynthesis, M.S. Smith, L.H. Kawano, R.A. Malaney, 1993, Astrophys. J. Suppl. 85, 219; and
Nuclear Astrophysics at the Beginning of the Twenty First Century, R.N. Boyd, in press.
Additional references were obtained from
W.R. Hix, A. Mezzacappa, and P.D. Parker.
Additions to this list are welcome; please contact Michael Smith at msmith@mail.phy.ornl.gov with suggestions.
0. General Nuclear Astrophysics References
1. Big Bang Nucleosynthesis
1.A. Overview
1.B. Evolution of abundances and primary reactions
1.C. Nuclear reaction rates and uncertainties
1.C.1. Overview
1.C.2. Reaction rate formalism
1.C.3. Reaction rate uncertainties
1.C.4. Individual reaction rates and uncertainties
1.C.4.a. The p(n,gamma)d reaction
1.C.4.b. The d(p,gamma)3He reaction
1.C.4.c. The d(d,n)3He reaction
1.C.4.d. The (d,p)t reaction
1.C.4.e. The 3He(n,p)t reaction
1.C.4.f. The t(d,n)4He reaction
1.C.4.g. The 3He(d,p)4He reaction
1.C.4.h. The 3He(alpha,gamma)7Be reaction
1.C.4.i. The t(alpha,gamma)7Li reaction
1.C.4.j. The 7Be(n,p)7Li reaction
1.C.4.k. The 7Li(p,alpha)4He reaction
1.C.4.l. Neutron Decay Lifetime
1.C.5. Comparison of new and previous rates
1.D. Numerical analysis and results
1.E. Inferred primordial abundances
1.E.1. Overview
1.E.2. Primoridal deuterium
1.E.3. Primordial 3He
1.E.4. Primordial D + 3He
1.E.5. Primordial 4He
1.E.6. Primordial lithium
1.E.6.a. Lithium in Population II stars
1.E.6.b. Lithium in Population I stars
1.F. Comparison of observed and predicted
primordial abundances
2. Neutrino Astrophysics
2.A. The Solar Neutrino Problem
2.B. Other Aspects of Neutrino Astrophysics
3. Stellar Evolution
3.A. Historical Overview
3.B. Evolution of single stars that become white dwarfs
3.B.1. Overview
3.B.2. Nucleosynthesis and dredge-up prior to the AGB phase
3.B.3. Nucleosynthesis and dredge-up during the AGB phase
3.B.4. The born-again AGB phase
3.B.5. Other mixing processes, and wind-mass loss, which affect surface composition
3.C. Evolution of massive single stars that produce neutron stars or black holes
3.D. Close binary star evolution
3.D.1. Modes of mass transfer and of orbital angular momentum loss
3.D.2. Scenario modeling
3.D.2.a. Cataclysmic variables and novae
3.D.2.b. White dwarf mergers: R CrB stars and type Ia supernovae
3.D.2.c. X-ray binaries and pulsars
4. Hydrogen Burning in the pp Chain and
CN Cycle
4.A. The p(p,e+nue)d reaction
4.B. The 3He(3He,2p)4He reaction
4.C. The 3He(alpha,gamma)7Be reaction
4.D. The 7Be(p,gamma)8Be reaction
4.E. The 7Li(n,gamma)8Li reaction
4.F. The 14N(p,gamma)15O reaction
4.G. The 17O(p,alpha)14N reaction
4.H. The Hot CNO cycle
5. The x Process
5.A. Introduction and Retrospective
5.B. Abundances
5.B.1. Lithium
5.B.2. Beryllium
5.B.3. Boron
5.C. Nonlocal thermodynamic-equilibrium effects
5.D. Production mechanisms
5.D.1. Big Bang
5.D.2. Spallation
5.D.3. Asymptotic giant branch stars
5.D.4. Supernovae
6. Helium Burning
6.A. Triple-alpha capture
6.B. alpha+12C capture
6.B.1. E1 capture
6.B.1.a. Direct measurements
6.B.1.b. beta-delayed alpha spectrum from the decay of 16N
6.B.2. E2 capture
6.B.3. Other analyses and recommended values
7. H Burning in the NeSi Region: Laboratory
Studies
7.A. Introduction
7.B. Experimental approaches
7.C. The neon-sodium cycle at low temperatures
7.C.1. Reaction rates
7.C.1.a. The 20Ne(p,gamma)21Na reaction
7.C.1.b. The 21Ne(p,gamma)23Na reaction
7.C.1.c. The 22Na(p,gamma)23Mg reaction
7.C.1.d. The 22Ne(p,gamma)23Na reaction
7.C.1.e. The 23Na(p,gamma)24Mg and 23Na(p,alpha)20Ne reactions
7.C.2. Network calculations
7.D. The magnesium-aluminum cycle at low temperatures
7.D.1. Reaction rates
7.D.1.a. The 24Mg(p,gamma)25Al reaction
7.D.1.b. The 25Mg(p,gamma)26Al reaction
7.D.1.c. The 26Mg(p,gamma)27Al reaction
7.D.1.d. The 26Al(p,gamma)27Si reaction
7.D.1.e. The 27Al(p,gamma)28Si reaction and 27Al(p,alpha)24Mg reaction
7.E. High-temperature behavior
7.E.1. Reaction rates
7.E.2. Network calculations
8. Observational Evidence of Hydrogen Burning
8.A. CN cycle and mixing
8.B. O depletion and the enhancement of Na and Al
8.C. Origin of the Na and Al enhancements
9. Carbon, Neon, Oxygen, and Silicon Burning
9.A. Introduction
9.B. Carbon burning
9.C. Neon burning
9.D. Oxygen burning
9.E. Silicon burning
10. s Process: Laboratory Studies
and Stellar Models
10.A. The s process since B2FH
10.B. Laboratory experiments
10.B.1. Neutron capture cross sections
10.B.2. Stellar beta decay
10.C. The canonical s process
10.C.1. The sigma*N curve
10.C.2. Branchings
11. Observations of the s process
11.A. Brief history
11.B. Observations of nucleosynthesis and mixing in CH, Ba, S, and C stars
11.C. The s process as a function of metallicity
11.D. Rubidium and the s-process neutron density
11.E. Recent models: Radiative buring of 13C during the AGB interpulse phase
12. The r process
12.A. Introduction
12.B. A search for the astrophysical site
12.C. Early model results, from conflict to clarity
12.D. High-Entropy winds
13. Observations of the r process
13.A. Defining the r-process elements
13.B. Early r-process discoveries
13.C. Recent r-process surveys
13.D. Thorium and the age of the halo and disk
13.E. Filling out the picture
14. The p process
14.A. The p process
14.B. Early p-process models
14.C. The gamma process
14.D. The rp process
14.E. The nu process
14.F. Recent developments
15. The e process and the
iron-group nuclei
15.A. Energetics and equilibria
15.B. Statistical equilibrium
15.C. A brief history of the ideas of iron-group element synthesis
15.D. Significance for astrophysics
16. Carbon Stars
16.A. Prologue
16.B. Carbon stars--An observer's view
16.B.1. What is a carbon-rich star?
16.B.2. What makes a carbon-rich star?
16.B.3. The principle types of carbon-rich stars
16.B.3.a. R-type carbon stars
16.B.3.b. N-type carbon stars
16.B.3.c. Barium and related stars
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