The 18O(p, α)15N reaction at stellar energies☆
References (22)
- et al.
Ann. Rev. Astr. and Astrophys.
(1975) - M. Wiescher, K. U. Kettner, H. P. Trautvetter, R. E. Azuma, W. E. Kieser, K. P. Jackson, J. W. Hammer and C. Rolfs, to...
- et al.
- et al.
Nucl. Data Tables
(1970) - et al.
Thin Solid Films
(1973) - et al.
Nucl. Phys.
(1978) - et al.
Astrophys. J. Lett.
(1974)et al.Nucl. Phys.
(1975) Nucl. Phys.
(1978)- et al.
J. of Phys.
(1978)K. W. Allen, private... Phil. Mag.
(1951)
Phil. Mag.
Cited by (94)
Improved astrophysical rate for the <sup>18</sup>O(p,α)<sup>15</sup>N reaction by underground measurements
2019, Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy PhysicsCitation Excerpt :Furthermore, the 0.3 keV uncertainty in the energy of each data point of this work was converted into an uncertainty in the corresponding cross-section and added in quadrature to the other statistical uncertainties. The authors acknowledge A.I. Karakas for providing the stellar structure of the 5 M⊙ Monash model, and R.J. deBoer for a digitization of data from [11]. This work was supported in part by INFN, STFC UK (grant no. ST/L005824/1), NKFIH (grant no. K120666), HAS Lendület (grant no. LP2014-17), and DFG (grant no. BE 4100/4-1).
Monte Carlo simulation of the LENA detector system
2013, Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated EquipmentCitation Excerpt :The simulated two-dimensional histogram of the energy deposited in the HPGe detector (x-axis) versus the energy deposited in the NaI(Tl) annulus (y-axis) is shown in Fig. 7. The known decay scheme and Q-value are taken from Refs. [12–16] and are built into the simulation. Fig. 8 shows the comparison between the data and simulation with the condition for Gate 1 applied.
ANC From Experimental Perspective
2020, Frontiers in Astronomy and Space SciencesIndirect Measurements of n- and p-Induced Reactions of Astrophysical Interest on Oxygen Isotopes
2020, Frontiers in Astronomy and Space Sciences
- ☆
Supported in part by the Deutsche Forschungsgemeinschaft [Ro 429/2-5].