Trojan horse method as surrogate indirect approach to study resonant reactions in nuclear astrophysics
arXiv:2007.13331 · doi:10.1140/epja/s10050-020-00214-9
Abstract
We review the Trojan horse method and its applications to resonant reactions in nuclear astrophysics.
References in corpus (33)
- Microscopic Clustering in Light Nuclei
- Study of the 12C+12C fusion reactions near the Gamow energy
- s-Process Nucleosynthesis in Carbon Stars
- Frontiers in Nuclear Astrophysics
- The reaction 13C(alpha,n)16O: a background for the observation of geo-neutrinos
- New measurement of C+C fusion reaction at astrophysical energies
- First direct measurement of the total cross section of 12C(alpha,gamma)16O
- Effects of mutual excitations in the fusion of carbon isotopes
- New determination of the 13C(a, n)16O reaction rate and its influence on the s-process nucleosynthesis in AGB stars
- Trojan Horse as an indirect technique in nuclear astrophysics. Resonance reactions
- Constraining the 6.05 MeV 0 and 6.13 MeV 3 cascade transitions in the C(,)O reaction using the Asymptotic Normalization Coefficients
- Suppression of the centrifugal barrier effects in the off-energy-shell neutron+O interaction
- Theory of deuteron stripping. From surface integrals to generalized -matrix approach
- Characterizing the astrophysical S-factor for C+C with wave-packet dynamics
- An Optical Readout TPC (O-TPC) for Studies in Nuclear Astrophysics With Gamma-Ray Beams at HIgS
- Astrophysical factors of fusion from Trojan horse method
- Concurrent application of ANC and THM to assess the absolute cross section at astrophysical energies and possible consequences for neutron production in low-mass AGB stars
- Broad levels in O and their relevance for the astrophysical s-process
- Primordial reaction and second Lithium puzzle
- Status on fusion at deep subbarrier energies: impact of resonances on astrophysical factors
- New ANC measurement of the 1/2 state in O at 6.356 MeV, that dominates the C(,n)O reaction rate at temperatures relevant for the s-process
- Astrophysical factor for the reaction from -matrix analysis and asymptotic normalization coefficient for . Is any fit acceptable?
- Ambiguities of the Rate of Oxygen Formation During Stellar Helium Burning in the 12C(a,g) Reaction
- Coulomb renormalization and ratio of proton and neutron asymptotic normalization coefficients for mirror nuclei
- Subthreshold resonances and resonances in the -matrix method for binary reactions and in the Trojan Horse method
- Assessing the foundation of the Trojan Horse Method
- Connection between asymptotic normalization coefficients and resonance widths of mirror states
- Internal and external radiative widths in the combined R-matrix and potential model formalism
- Surface-integral formalism of deuteron stripping
- Nuclear Structure and the Fate of Core Collapse (Type II) Supernova
- Theory of surrogate nuclear and atomic reactions with three charged particles in the final state proceeding through a resonance in the intermediate subsystem
- Radiative capture reactions via indirect method
- On the sensitivity of extracting the astrophysical cross section factor of the 12C(a,g) reaction from existing data [Comment on Schuermann et al. Phys. Lett. B711(2012)35]