4.5 Article

Benchmark on neutron capture extracted from (d, p) reactions

期刊

PHYSICAL REVIEW C
卷 77, 期 5, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.77.051601

关键词

-

向作者/读者索取更多资源

Direct neutron capture reactions play an important role in nuclear astrophysics and applied physics. Since for most unstable short-lived nuclei it is not possible to measure the (n, gamma) cross sections, (d, p) reactions have been used as an alternative indirect tool. We analyze simultaneously Ca-48(d, P)Ca-49 reactions at deuteron energies of 2, 13, 19, and 56 MeV and the thermal (n, gamma) reaction at 25 meV. We include results for the ground state and the first excited state of Ca-49. From the low-energy (d, p) reaction, the neutron asymptotic normalization coefficient (ANC) is determined. Using this ANC, we extract the spectroscopic factor (SF) from the higher energy (d, p) data and the (n, gamma) data. The SF obtained through the 56-MeV (d, p) data are less accurate but consistent with those from the thermal capture. We show that to have a similar dependence on the single-particle parameters as in the (n, gamma), the (d, p) reaction should be measured at 30 MeV.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.5
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

Article Physics, Nuclear

Cross-sections at sub-Coulomb energies: Full optical model versus barrier transmission for 40Ca + α

Peter Mohr

INTERNATIONAL JOURNAL OF MODERN PHYSICS E (2019)

Article Physics, Nuclear

Yrast band in the heavy N = Z nucleus 88Ru: α-cluster approach

Peter Mohr

EUROPEAN PHYSICAL JOURNAL A (2020)

Article Physics, Multidisciplinary

Successful Prediction of Total α-Induced Reaction Cross Sections at Astrophysically Relevant Sub-Coulomb Energies Using a Novel Approach

P. Mohr, Zs Fulop, Gy Gyurky, G. G. Kiss, T. Szucs

PHYSICAL REVIEW LETTERS (2020)

Article Physics, Atomic, Molecular & Chemical

Astrophysical reaction rates of α-induced reactions for nuclei with 26 ≤ Z ≤ 83 from the new Atomki-V2 α-nucleus potential

P. Mohr, Zs Fulop, Gy Gyurky, G. G. Kiss, T. Szucs, A. Arcones, M. Jacobi, A. Psaltis

Summary: The new Atomki-V2 alpha-nucleus potential is used to calculate astrophysical reaction rates for intermediate mass and heavy target nuclei from iron to bismuth, covering a wide range of neutron-deficient and extremely neutron-rich target nuclei. These calculations include all relevant exit channels, with a focus on the dominating (alpha, xn) reactions for neutron-rich target nuclei, unlike previous rate compilations.

ATOMIC DATA AND NUCLEAR DATA TABLES (2021)

Article Astronomy & Astrophysics

The 59Fe (n,γ) 60Fe Cross Section from the Surrogate Ratio Method and Its Effect on the 60Fe Nucleosynthesis

S. Q. Yan, X. Y. Li, K. Nishio, M. Lugaro, Z. H. Li, H. Makii, M. Pignatari, Y. B. Wang, R. Orlandi, K. Hirose, K. Tsukada, P. Mohr, G. S. Li, J. G. Wang, B. S. Gao, Y. L. Han, B. Guo, Y. J. Li, Y. P. Shen, T. K. Sato, Y. Ito, F. Suzaki, J. Su, Y. Y. Yang, J. S. Wang, J. B. Ma, P. Ma, Z. Bai, S. W. Xu, J. Ren, Q. W. Fan, S. Zeng, Z. Y. Han, W. Nan, W. K. Nan, C. Chen, G. Lian, Q. Hu, F. F. Duan, S. Y. Jin, X. D. Tang, W. P. Liu

Summary: In this study, the Fe-59(n,gamma)Fe-60 cross sections were experimentally determined using the surrogate ratio method for the first time, yielding values roughly 10%-20% higher than previous estimates. The analysis showed that uncertainties in stellar physics play a major role in the accurate evaluation of Fe-60 production, with uncertainties in the Fe-59(n,gamma)Fe-60 rate being at most 25%.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Constraining Nucleosynthesis in Neutrino-driven Winds: Observations, Simulations, and Nuclear Physics

A. Psaltis, A. Arcones, F. Montes, P. Mohr, C. J. Hansen, M. Jacobi, H. Schatz

Summary: This study investigates the impact of nuclear reactions on the synthesis of lighter heavy elements. Using a Monte Carlo approach and improved (alpha, xn) rates, the study identifies the effects of (alpha, xn) reaction rates on elemental ratios in different astrophysical conditions. The study calls for more nuclear physics experiments and observational studies of metal-poor stars.

ASTROPHYSICAL JOURNAL (2022)

Article Physics, Nuclear

a-decay half-life of 212Po at stellar temperatures

Peter Mohr

Summary: This study analyzes how the decay properties of atomic nuclei can be altered in stellar environments. Contrary to a recent study claiming a significant reduction in the half-life of Po-212 by up to five orders of magnitude, this study shows a moderate reduction of less than one order of magnitude up to 2 GK.

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS (2023)

Editorial Material Physics, Nuclear

Comment on 'Alpha decay of thermally excited nuclei'

Peter Mohr

Summary: In a recent study, Perez Velasquez, Caballero, and Kelkar found a significant enhancement in the decay rate of the nucleus Po-212 at a temperature of 2 Giga-Kelvin, reaching almost five orders of magnitude. However, in the present comment based on a careful study of the properties of excited states in Po-212, only a moderate enhancement by a factor of three is observed.

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS (2023)

Article Physics, Nuclear

Fusion cross section of α-induced reactions for heavy target nuclei

Raj Kumar, Shilpa Rana, M. Bhuyan, P. Mohr

Summary: This study investigates the effects of different nuclear density distributions and effective nucleon-nucleon interaction potentials on the fusion cross section of He-4-induced reactions on heavy target nuclei. The results show that the relativistic R3Y NN potential folded with RMF densities provides a better fit to the experimental data.

PHYSICAL REVIEW C (2022)

Article Physics, Nuclear

First direct measurement of 59Cu(p, α) 56Ni: A step towards constraining the Ni-Cu cycle in the cosmos

J. S. Randhawa, R. Kanungo, J. Refsgaard, P. Mohr, T. Ahn, M. Alcorta, C. Andreoiu, S. S. Bhattacharjee, B. Davids, G. Christian, A. A. Chen, R. Coleman, P. E. Garrett, G. F. Grinyer, E. Gyabeng Fuakye, G. Hackman, J. Hollett, R. Jain, K. Kapoor, R. Krucken, A. Laffoley, A. Lennarz, J. Liang, Z. Meisel, B. Nikhil, A. Psaltis, A. Radich, M. Rocchini, N. Saei, M. Saxena, M. Singh, C. Svensson, P. Subramaniam, A. Talebitaher, S. Upadhyayula, C. Waterfield, J. Williams, M. Williams

Summary: Reactions on proton-rich nuclides play a crucial role in nucleosynthesis in core collapse supernovae and x-ray bursts. However, the Ni-Cu cycle may pose a challenge for the production of heavier elements during the Cu-59(p, alpha) Ni-56 reaction. New research suggests that the vp process could operate at higher temperatures, making it a viable pathway for synthesizing heavier elements.

PHYSICAL REVIEW C (2021)

Article Astronomy & Astrophysics

The 95Zr(n, γ)96Zr Cross Section from the Surrogate Ratio Method and Its Effect on s-process Nucleosynthesis

S. Q. Yan, Z. H. Li, Y. B. Wang, K. Nishio, M. Lugaro, A. I. Karakas, H. Makii, P. Mohr, J. Su, Y. J. Li, I. Nishinaka, K. Hirose, Y. L. Han, R. Orlandi, Y. P. Shen, B. Guo, S. Zeng, G. Lian, Y. S. Chen, W. P. Liu

ASTROPHYSICAL JOURNAL (2017)

Article Physics, Nuclear

α scattering and α-induced reaction cross sections of 64Zn at low energies

A. Ornelas, P. Mohr, Gy. Gyurky, Z. Elekes, Zs. Fulop, Z. Halasz, G. G. Kiss, E. Somorjai, T. Szuecs, M. P. Takacs, D. Galaviz, R. T. Guray, Z. Korkulu, N. Ozkan, C. Yalcin

PHYSICAL REVIEW C (2016)

Article Astronomy & Astrophysics

RE-EVALUATION OF THE 16O(N, γ)17O CROSS SECTION AT ASTROPHYSICAL ENERGIES AND ITS ROLE AS A NEUTRON POISON IN THE s-PROCESS

Peter Mohr, Christian Heinz, Marco Pignatari, Iris Dillmann, Alberto Mengoni, Franz Kaeppeler

ASTROPHYSICAL JOURNAL (2016)

暂无数据