Revised rates for the stellar triple-α process from measurement of 12C nuclear resonances

By H. Fynbo, C. Diget, U. Bergmann, M. Borge, J. Cederkäll, P. Dendooven, L. Fraile, S. Franchoo, V. Fedosseev, B. Fulton and 21 more. Nature, 2005

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Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/ee19863ae5bfecc5a2a510a8167abc527097da24

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CONVECTIVE–REACTIVE PROTON–12C COMBUSTION IN SAKURAI'S OBJECT (V4334 SAGITTARII) AND IMPLICATIONS FOR THE EVOLUTION AND YIELDS FROM THE FIRST GENERATIONS OF STARS (2010, background): “…for basic energetic nuclear reactions, i.e., 14N(p,γ)15O, 3-α and 12C(α,γ)16O. Notice that the use of more recent rates (e.g., Imbriani et al. 2005; Fynbo et al. 2005; Kunz et al. 2002, respectively) would not change our results, where uncertainties related to physics processes and mixing…”
NUGRID STELLAR DATA SET. I. STELLAR YIELDS FROM H TO BI FOR STARS WITH METALLICITIES Z = 0.02 and Z = 0.01 (2013, methodology): “These include triple-α and 12C(α,γ)16O reactions from Fynbo et al. (2005) and Kunz et al. (2002), respectively, as well as the 14N(p,γ)15O reaction (Imbriani et al. 2005).”
Yields of AGB and SAGB models with chemistry of low- and high-metallicity globular clusters (2013, background): “…relevant cross-sections are taken from the recommended values in the NACRE compilation (Angulo et al. 1999), with only the following exceptions: 3α (Fynbo et al. 2005); 12C(α,γ)16O (Kunz et al. 2002); 14N(p,γ)15O (Formicola et al. 2004); 22Ne(p,γ)23Na (Hale et al. 2002); 23Na(p,γ)24Mg (Hale et…”
s-process production in rotating massive stars at solar and low metallicities (2015, methodology): “The charged particle reaction rates from Angulo, Arnould & Rayet (NACRE compilation, 1999) were used except for the following reactions: 22Ne(α,n) and the 3α-rate were taken from Jaeger et al. (2001) and from Fynbo et al. (2005), respectively.”
Thermohaline instability and rotation-induced mixing - III. Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars of various metallicities (2012, unknown): “The following reactions rates are computed by: – 3He(D, p)4He (Descouvemont et al. 2004); – 3He(αα, γ)12C (Fynbo et al. 2005); – 8B(β, ν)24He; 13N(β, ν)13C; 22Na(β, ν)22Ne; 26Alm(β, ν)26Mg; 26Alg(β, ν)26Mg (Horiguchi et al. 1996); – 14C(p, γ)15N (Wiescher et al. 1990); – 14C(p, n)14N (Koehler &…”
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS (2016, background): “For example, the 15N(p,α)12C reaction rate comes from Angulo et al. (1999), while the triple-α reaction rate comes from Fynbo et al. (2005).”
THE JINA REACLIB DATABASE: ITS RECENT UPDATES AND IMPACT ON TYPE-I X-RAY BURSTS (2010, methodology): “The differences between the Fynbo et al. (2005) and the NACRE rate (Angulo et al. 1999) are negligible for X-ray burst temperatures.”
CHARGED-PARTICLE AND NEUTRON-CAPTURE PROCESSES IN THE HIGH-ENTROPY WIND OF CORE-COLLAPSE SUPERNOVAE (2010, methodology): “In addition, test calculations with Fynbo’s triple-alpha reaction rates (Fynbo et al. 2005) have been performed for two entropies S = 100 and 250 kB/baryon, although in several (A color version of this figure is available in the online journal.) recent publications the data analysis with respect to…”
Non-standard s process in low metallicity massive rotating stars (2011, methodology): “The charged particle reaction rates from Angulo et al. (1999) were used except for the following reactions: 22Ne(α,n) was taken from Jaeger et al. (2001) and the 3α-rate from Fynbo et al. (2005).”
Radioactive decays at limits of nuclear stability (2011, background): “…beta-delayed decays can be illustrated with the case of 12N (and 12B) whose decay into the 3α continuum has recently been studied in detail (Diget et al., 2009; Hyldegaard et al., 2010, 2009) motivated by the importance of this continuum for the astrophysical triple-α process (Fynbo et al., 2005).”
MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA) (2010, unknown): “Signiﬁcant updates to the NACRE rates have been included for 14 N( p , γ ) 15 O (Imbriani et al. 2004), triple-α (Fynbo et al. 2005), 14 N( α, γ ) 18 F (G¨orres et al. 2000), and 12 C( α, γ ) 16 O (Kunz et al. 2002).”