Astrophysical factors of fusion from Trojan horse method
arXiv:1806.08828 · doi:10.1103/PhysRevC.99.064618
Abstract
Carbon-carbon burning plays an important role in many stellar environments. Recently, using the indirect Trojan horse method A. Tumino {\em et al.} reported [Nature {\bf 557} 687 (2018)] a strong rise of the astrophysical factor for the carbon-carbon fusion at low resonance energies. In this paper, we demonstrate that this rise is the artifact of using an invalid plane-wave approximation. It is shown that the calculated renormalization factor decreases the astrophysical factor from [A. Tumino {\em et al.}, Nature {\bf 557} 687 (2018)] at the resonance energies of MeV by as much as times.
arXiv comment11 pages, 10 figures
References in corpus (3)
Cited by in corpus (18)
- New measurement of C+C fusion reaction at astrophysical energies
- Status on fusion at deep subbarrier energies: impact of resonances on astrophysical factors
- Constraining the C+C astrophysical S-factors with the C+C measurements at very low energies
- Fusion -factor from a Full-microscopic Nuclear Model
- The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics?
- The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
- The study of key reactions shaping the post main-sequence evolution of massive stars in underground facilities
- Massive stars evolution with new C12+C12 nuclear reaction rate -- the core carbon-burning phase
- The modified astrophysical S-factor of the C+C fusion reaction at sub-barrier energies
- Trojan horse method as surrogate indirect approach to study resonant reactions in nuclear astrophysics
- The Intrinsic Stochasticity of the Ni Distribution of Single-Degenerate Type Ia Supernovae
- Refining the deep sub-barrier 12C+12C excitation function with STELLA
- Constraining Accreted Neutron Star Crust Shallow Heating with the Inferred Depth of Carbon Ignition in X-ray Superbursts
- Re-examination of fusion hindrance in astrophysical C+C and C+C reactions
- Asymptotic normalization coefficient method for two-proton radiative capture
- Indirect Measurement of the Factor for at Gamow Energies via the Trojan Horse Method with Near-0 degree Spectator Detection
- Clusters in light stable and exotic nuclei
- measurement of the reaction at astrophysical energies via the Trojan horse method with quasi-free breakup