Astrophysical Reaction Rates From Statistical Model Calculations
arXiv:astro-ph/0004059 · doi:10.1006/adnd.2000.0834
Abstract
Theoretical reaction rates in the temperature range 0.01*10^9<=T[K]<=10.*10^9 are calculated in the statistical model (Hauser-Feshbach formalism) for targets with 10<=Z<=83 (Ne to Bi) and for a mass range reaching the neutron and proton driplines. Reactions considered are (n,gamma), (n,p), (n,alpha), (p,gamma), (p,alpha),(alpha,gamma), and their inverse reactions. Reaction rates as a function of temperature for thermally populated targets are given by analytic seven parameter fits. To facilitate comparison with experimental rates, the stellar enhancement factors are also tabulated. Two complete sets of rates have been calculated, one of which includes a phenomenological treatment of shell quenching for neutron-rich nuclei. These extensive datasets are provided on-line as electronic files, while a selected subset from one calculation is given as printed tables. A summary of the theoretical inputs and advice on the use of the provided tabulations is included.
22 pages of text and 1 table; accepted by Atomic Data Nuclear Data Tables; a preprint is also available from http://quasar.physik.unibas.ch/~tommy/adndt.html
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- The Impact of Stellar Abundance Variations on Stellar Habitable Zone Evolution
- Calculation of excitation function of some structural fusion material for (n,p) reactions up to 25 MeV
- Endpoint of process using relativistic mean field approach and a new mass formula
- Determination of the Neutron-Capture Rate of 17C for the R-process Nucleosynthesis
- The Fe(n, γ)Fe Cross Section from the Surrogate Ratio Method and Its Effect on the Fe Nucleosynthesis
- Measurement of the Tb(n, ) cross section at the CSNS Back-n facility
- Temperature-dependent nuclear partition functions and abundances in stellar interior
- Low energy () reactions in Ni and Cu nuclei using microscopic optical model
- (n,) Cross Sections of Light p Nuclei -- Towards an Updated Database for the p Process
- Experimental determination of the He(,)Be reaction cross section above the Be proton separation threshold
- Cross section measurement of the 144Sm(alpha,n)147Gd reaction for studying the alpha-nucleus optical potential at astrophysical energies
- Evaluation of the K(,)Ca reaction rate using the Ca(,)Ca transfer reaction
- Examination and experimental constraints of the stellar reaction rate factor of the Ne(,)Na reaction at temperatures of X-Ray Bursts
- Measurement of the stellar NiNi cross section with AMS
- Impact of level densities and -strength functions on -process simulations
- Sensitivity of nuclear statistical equilibrium to nuclear uncertainties during stellar core collapse
- Low-energy proton capture reactions in the mass region 55-60
- Unexpected properties of the S(,p)Cl reaction cross section at low energies
- MONTAGE: AGB nucleosynthesis with full s-process calculations
- Direct capture in the Sn(n,)Sn and Sn(n,)Sn reactions under -process conditions
- Indirect measurement of the Sb cross section
- Astrophysical Rates for Explosive Nucleosynthesis: Stellar and Laboratory Rates for Exotic Nuclei
- Cross Sections of the Rb(p,Sr and Kr(p,Rb Reactions at Energies Characteristic of the Astrophysical Process
- Nuclear reactions in hot stellar matter and nuclear surface deformation
- Measurement of the 91Zr(p,gamma)92mNb cross section motivated by type Ia supernova nucleosynthesis
- Origin of the Chemical Elements
- Accurate stellar parameters and distance to two evolved eclipsing binary systems, OGLE-BLG-ECL-123903 and OGLE-BLG-ECL-296596, towards the Galactic bulge
- Nuclear level density of Zn from gamma gated particle spectrum and its implication on Zn(n, )Zn capture cross-section
- Thermonuclear 17O(n,gamma)18O reaction rate and its astrophysical implications
- Nuclear Ignition of White Dwarf Stars by Relativistic Encounters with Rotating Intermediate Mass Black Holes
- Thermonuclear 42Ti(p,gamma)43V rate in type I X-ray bursts
- The Importance of Parity-Dependence of the Nuclear Level Density in the Prediction of Astrophysical Reaction Rates
- Measurements of the Zr(,n)Mo cross section for astrophysics and applications
- -ray Strength Function for Barium Isotopes
- The role of low-lying resonances for Be(p,) reaction rate and implications for the formation of the Solar System
- Instantaneous Shape Sampling - a model for the -absorption cross section of transitional nuclei
- The Sensitivity of Nucleosynthesis in Type I X-ray Bursts to Thermonuclear Reaction-Rate Variations
- Coupling highly excited nuclei to the atomic shell in dense astrophysical plasmas
- Constraining the destruction rate of K in stellar nucleosynthesis through the study of the Ar(p,n)K reaction
- Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH
- Reaction rate weighted multilayer nuclear reaction network
- Improved Nuclear Physics Near Refines Urca Neutrino Luminosities in Accreted Neutron Star Crusts
- Reaction Rate Sensitivity of the gamma-Process Path
- Capitalizing on Nuclear Data Libraries' Comprehensiveness to Obtain Solar System r-process Abundances
- Impact of newly measured 26Al(n, p)26Mg and 26Al(n, α)23Na reaction rates on the nucleosynthesis of 26Al in stars
- Mass fractions in stellar interior during presupernova evolution
- Observing Nucleon Decay in Lead Perchlorate
- Nuclear reactions in hot astrophysical plasmas with K
- Experimental Evidence of Large Collective Enhancement of Nuclear Level Density and its Significance in Radiative Neutron Capture
- Neutron rich nuclei in a new binding energy formula and the astrophysical process
- Crucial inputs to nucleosynthesis calculations
- Explosive Nucleosynthesis: What we learned and what we still do not understand
- The Influence of Reaction Rates on the Final p-Abundances
- Tables of Neutron Thermal Cross Sections, Westcott Factors, Resonance Integrals, Maxwellian Averaged Cross Sections, Astrophysical Reaction Rates, and r-process Abundances Calculated from Evaluated Nuclear Data Libraries
- Study of Gamow-Teller strength and associated weak-rates on odd-A nuclei in stellar matter
- New 26P(p,γ)27S thermonuclear reaction rate and its astrophysical implication in rp-process
- Microscopic Study of (p,) Reactions in Mass Region A=110-125
- Cross sections of -induced reactions slightly below doubly-magic Ca from the statistical model
- Stellar Weak Rates and Mass Fractions of 20 Most Important -shell Nuclei with
- Allowed and unique first-forbidden stellar electron emission rates of neutron-rich copper isotopes
- The -processes nucleosynthesis during the formation of He-rich hot-subdwarf stars
- Coupling nuclear reaction rates with temperature in explosive conditions
- Microscopic folding model analysis of the radiative reactions near the shell-closure and the weak s-process
- Radiative neutron capture reaction rates for stellar nucleosynthesis
- New Ga(p,)Ge and Ge(p,)As reaction rates corresponding to the temperature regime of thermonuclear X-ray bursts
- Extension of the particle x-ray coincidence technique: The lifetimes and branching ratios apparatus
- Abundance Uncertainties Obtained With the PizBuin Framework For Monte Carlo Reaction Rate Variations
- Improved thermonuclear rate of Ti(,)V and its astrophysical implication in rp-process
- Capture Rates of Highly Degenerate Neutrons
- Astronomy with Radioactivities: Chapter 9, Nuclear Reactions
- Radiative proton capture cross sections in the mass range
- Radiative neutron capture reaction rates for r-process nucleosynthesis
- Nuclear Reactions For Nucleosynthesis Beyond Fe
- Nuclear Reactions in Evolving Stars
- The 2025 Evaluation of Experimental Thermonuclear Reaction Rates (ETR25)
- New experimental Na()Mg Reaction Rate for Massive Star and Type-Ia Supernova models
- Photo-nuclear reaction rates of Ho and Tm and their impact in the --process
- Extraction of neutron-capture cross sections on Zr using the charge-exchange Oslo method
- Machine-Learning-Enabled Measurements of Astrophysical (p,n) Reactions with the SECAR Recoil Separator
- Reevaluation of thermonuclear reaction rate of 50Fe(p,gamma)51Co
- Explicit Integration of Extremely-Stiff Reaction Networks: Quasi-Steady-State Methods
- Explosive nucleosynthesis in core-collapse supernovae
- Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
- Continuous Habitable Zones: Using Bayesian Methods to Prioritize Characterization of Potentially Habitable Worlds
- The Influence of a Shock on the Nucleosynthesis Developing during the Explosion of a Low-Mass Neutron Star
- Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs
- Around the Pair Instability Valley - Massive SN Progenitors
- Comment on "187Re(gamma,n) cross section close to and above the neutron threshold"
- Bare Collapse, Formation of Neutron Star Binaries and Fast Optical Transients
- Importance of -induced reactions and the inverse on -nuclei
- Astrophysical Reaction Rates for Charged-Particle Induced Reactions on Proton-Rich Nuclides
- Type Iax supernovae from deflagrations in Chandrasekhar mass white dwarfs
- Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates
- First strength measurements of low-energy resonances in the Sc()Ti reaction and its astrophysical implications