Asymptotic normalization coefficients in nuclear reactions and nuclear astrophysics
AM Mukhamedzhanov, LD Blokhintsev - The European Physical Journal A, 2022 - Springer
The asymptotic normalization coefficient (ANC) is a fundamental nuclear characteristic of
bound states and resonances. The ANC plays an important role in low-energy elastic …
bound states and resonances. The ANC plays an important role in low-energy elastic …
Single-nucleon knockout cross sections for reactions producing resonance states at or beyond the drip line
RJ Charity, LG Sobotka, JA Tostevin - Physical Review C, 2020 - APS
Single-nucleon knockout cross sections from fast secondary beams of the proton-drip-line
nuclei C 9, O 13, and Ne 17 on a Be 9 target have been studied with emphasis on the …
nuclei C 9, O 13, and Ne 17 on a Be 9 target have been studied with emphasis on the …
Missing mass spectroscopy on oxygen isotopes beyond the proton-drip line: mirror symmetry of nuclear shell evolution
D Suzuki - The European Physical Journal A, 2012 - Springer
Missing mass spectroscopy of the proton-rich 12 O and 13 O nuclei was performed via the
neutron transfer (p, t and (p, d reactions, respectively, using a 14 O beam of 51 MeV/u at …
neutron transfer (p, t and (p, d reactions, respectively, using a 14 O beam of 51 MeV/u at …
Proton decay of excited states in N and O and the astrophysical C(,N reaction rate
LG Sobotka, WW Buhro, RJ Charity, JM Elson… - Physical Review C …, 2013 - APS
Using a 13 O beam, we have observed proton decays of 12 N and 13 O excited states
following proton-knockout and inelastic interactions on a 9 Be target. The excited states …
following proton-knockout and inelastic interactions on a 9 Be target. The excited states …
Using spin alignment of inelastically excited nuclei in fast beams to assign spins: The spectroscopy of as a test case
Excited states in O 13 were investigated using inelastic scattering of an E/A= 69.5 MeV O 13
beam off of a Be 9 target. The excited states were identified in the invariant-mass spectra of …
beam off of a Be 9 target. The excited states were identified in the invariant-mass spectra of …
Astrophysical factor for the radiative capture determined from the proton transfer reaction
The cross section of the radiative proton capture reaction on the drip line nucleus N 12 was
investigated using the asymptotic normalization coefficient (ANC) method. We have used the …
investigated using the asymptotic normalization coefficient (ANC) method. We have used the …
Determination of the astrophysical N(,)O reaction rate from the H(N,O) reaction and its astrophysical implications
B Guo, J Su, ZH Li, YB Wang, SQ Yan, YJ Li… - Physical Review C …, 2013 - APS
The evolution of massive stars with very low-metallicities depends critically on the amount of
CNO nuclides which they produce. The 12 N (p, γ) 13 O reaction is an important branching …
CNO nuclides which they produce. The 12 N (p, γ) 13 O reaction is an important branching …
Experimental study of the knockout reaction mechanism using at 60 MeV/nucleon
Background: For the deeply bound one-nucleon removal at intermediate energies using a
Be 9 or C 12 target, a strong reduction of cross section was observed relative to the …
Be 9 or C 12 target, a strong reduction of cross section was observed relative to the …
Internal and external radiative widths in the combined -matrix and potential-model formalism
By using the R-matrix approach we calculate the radiative width for a resonance decaying to
a bound state through electric-dipole E 1 transitions. The total radiative width is determined …
a bound state through electric-dipole E 1 transitions. The total radiative width is determined …
[HTML][HTML] Reaction rate of radiative p12N capture
The S-factor of radiative p 12 N capture at energies from 20 keV to 5 MeV was considered
within the modified potential cluster model with forbidden states, considering the first …
within the modified potential cluster model with forbidden states, considering the first …