Further Reading — Chapter 22

Textbooks

Clayton, D. D. Principles of Stellar Evolution and Nucleosynthesis (University of Chicago Press, 1983). The classic textbook. Chapters 4–7 cover hydrogen, helium, and advanced burning stages in rigorous detail. Despite its age, it remains the most pedagogically complete treatment of stellar nucleosynthesis at the advanced undergraduate / graduate level.
Iliadis, C. Nuclear Physics of Stars, 2nd ed. (Wiley-VCH, 2015). The modern standard reference for nuclear astrophysics. Chapters 5–7 cover thermonuclear reaction rates, hydrogen burning, and helium burning with full derivations and up-to-date experimental data. Highly recommended as a companion to this chapter.
Rolfs, C. E. and Rodney, W. S. Cauldrons in the Cosmos: Nuclear Astrophysics (University of Chicago Press, 1988). An accessible introduction that emphasizes the experimental aspects of nuclear astrophysics. The treatment of the pp chain and CNO cycle is particularly clear.
Krane, K. S. Introductory Nuclear Physics (Wiley, 1988). Chapter 17 provides a concise introduction to nuclear astrophysics at the advanced undergraduate level, including stellar energy generation and nucleosynthesis.
Phillips, A. C. The Physics of Stars, 2nd ed. (Wiley, 1999). A stellar astrophysics textbook that complements the nuclear physics perspective. Chapters 5–7 cover the pp chain, CNO cycle, and advanced burning stages from the stellar structure viewpoint.

Bethe, H. A. "Energy Production in Stars." Physical Review 55, 434 (1939). The paper that identified the CNO cycle as the dominant hydrogen-burning mechanism in massive stars. Awarded the Nobel Prize in 1967.
Burbidge, E. M., Burbidge, G. R., Fowler, W. A., and Hoyle, F. "Synthesis of the Elements in Stars." Reviews of Modern Physics 29, 547 (1957). The B$^2$FH paper — the foundational document of stellar nucleosynthesis theory. Still worth reading for its clarity and scope.
Hoyle, F. "On Nuclear Reactions Occurring in Very Hot STARS. I. The Synthesis of Elements from Carbon to Nickel." Astrophysical Journal Supplement 1, 121 (1954). The paper that predicted the Hoyle state and outlined the advanced burning stages.
Salpeter, E. E. "Nuclear Reactions in Stars Without Hydrogen." Astrophysical Journal 115, 326 (1952). The first quantitative treatment of the triple-alpha process.
Cameron, A. G. W. "Stellar Evolution, Nuclear Astrophysics, and Nucleogenesis." Chalk River Report CRL-41 (1957). Published independently of B$^2$FH, this comprehensive report reached many of the same conclusions. Cameron's contributions are sometimes underappreciated.

Woosley, S. E., Heger, A., and Weaver, T. A. "The Evolution and Explosion of Massive Stars." Reviews of Modern Physics 74, 1015 (2002). Comprehensive review of massive star evolution, including detailed nucleosynthesis yields and pre-supernova structures.
deBoer, R. J. et al. "The ${}^{12}$C$(\alpha,\gamma){}^{16}$O Reaction and Its Implications for Stellar Helium Burning." Reviews of Modern Physics 89, 035007 (2017). The definitive review of the most important reaction rate in nuclear astrophysics.
Freer, M., Horiuchi, H., Kanada-En'yo, Y., Lee, D., and Meissner, U.-G. "Microscopic Clustering in Light Nuclei." Reviews of Modern Physics 90, 035004 (2018). Includes a thorough discussion of the Hoyle state and alpha-clustering in ${}^{12}$C.
Adelberger, E. G. et al. "Solar Fusion Cross Sections. II. The pp Chain and CNO Cycles." Reviews of Modern Physics 83, 195 (2011). The community standard for solar nuclear reaction rates. Essential reference for all S-factor values cited in this chapter.
Jose, J. and Iliadis, C. "Nuclear Astrophysics: The Unfinished Quest for the Origin of the Elements." Reports on Progress in Physics 74, 096901 (2011). Accessible review covering nucleosynthesis from the Big Bang through stellar evolution.

Dunbar, D. N. F., Pixley, R. E., Wenzel, W. A., and Whaling, W. "The 7.68-MeV State in ${}^{12}$C." Physical Review 92, 649 (1953). The experimental discovery of the Hoyle state.
Epelbaum, E., Krebs, H., Lee, D., and Meissner, U.-G. "Ab Initio Calculation of the Hoyle State." Physical Review Letters 106, 192501 (2011). Lattice effective field theory calculation reproducing the Hoyle state energy.
Kibedi, T. et al. "Radiative Width of the Hoyle State from Gamma-Ray Spectroscopy." Physical Review Letters 125, 182701 (2020). Precision measurement of the Hoyle state radiative width.
Fynbo, H. O. U. et al. "Revised Rates for the Stellar Triple-Alpha Process from Measurement of ${}^{12}$C Nuclear Resonances." Nature 433, 136 (2005). Updated triple-alpha rate based on improved measurements.

Bahcall, J. N. Neutrino Astrophysics (Cambridge University Press, 1989). The definitive treatment of solar neutrino physics by its principal architect.
Borexino Collaboration. "Experimental Evidence of Neutrinos Produced in the CNO Fusion Cycle in the Sun." Nature 587, 577 (2020). First direct detection of CNO neutrinos from the Sun.
Ahmad, Q. R. et al. (SNO Collaboration). "Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in SNO." Physical Review Letters 89, 011301 (2002). Resolution of the solar neutrino problem.

JINA REACLIB: https://reaclib.jinaweb.org/ — The standard thermonuclear reaction rate library used in astrophysical simulations.
NACRE/NACRE-II: Nuclear Astrophysics Compilation of REaction Rates. Angulo et al., Nuclear Physics A 656, 3 (1999), and Xu et al., Nuclear Physics A 918, 61 (2013).
STARLIB: Sallaska et al., Astrophysical Journal Supplement 207, 18 (2013). Monte Carlo-based reaction rate library with uncertainties.

MESA (Modules for Experiments in Stellar Astrophysics): http://mesa.sourceforge.net/ — Open-source stellar evolution code. Paxton et al., Astrophysical Journal Supplement 192, 3 (2011) and subsequent papers.
NuGrid: http://nugridstars.org/ — Open-source nucleosynthesis and stellar evolution data, including pre-supernova composition profiles.