Measurement of the 13C(α, n0)16O Differential Cross Section from 0.8 to 6.5 MeV

被引：2

作者：

deBoer, R. J. ^{[1
]}

Febbraro, M. ^{[2
]}

Bardayan, D. W. ^{[1
]}

Boomershine, C. ^{[1
]}

Brandenburg, K. ^{[3
]}

Brune, C. ^{[3
]}

Coil, S. ^{[1
]}

Couder, M. ^{[1
]}

Derkin, J. ^{[3
]}

Dede, S. ^{[1
]}

Fang, R. ^{[1
]}

Fritsch, A. ^{[4
]}

Gula, A. ^{[1
]}

Gyurky, Gy. ^{[5
]}

Hackett, B. ^{[6
]}

Hamad, G. ^{[3
]}

Jones-Alberty, Y. ^{[3
]}

Kelmar, R. ^{[1
]}

Manukyan, K. ^{[1
]}

Matney, M. ^{[1
]}

McDonaugh, J. ^{[1
]}

Meisel, Z. ^{[3
]}

Moylan, S. ^{[1
]}

Nattress, J. ^{[2
]}

Odell, D. ^{[3
]}

O'Malley, P. ^{[1
]}

Paris, M. W. ^{[7
]}

Robertson, D. ^{[1
]}

Shahina ^{[1
]}

Singh, N. ^{[3
]}

Smith, K. ^{[8
]}

Smith, M. S. ^{[2
]}

Stech, E. ^{[1
]}

Tan, W. ^{[1
]}

Wiescher, M. ^{[1
]}

机构：

[1] Univ Notre Dame, Dept Phys & Astron, Notre Dame, IN 46556 USA

[2] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA

[3] Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA

[4] Gonzaga Univ, Dept Phys, Spokane, WA 99258 USA

[5] Inst Nucl Res Atomki, POB 51, H-4001 Debrecen, Hungary

[6] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA

[7] Los Alamos Natl Lab, Theoret Div, Los Alamos, NM 87545 USA

[8] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

来源：

PHYSICAL REVIEW LETTERS | 2024年 / 132卷 / 06期

基金：

美国国家科学基金会;

关键词：

S-PROCESS; PROCESS NUCLEOSYNTHESIS; ANGULAR-DISTRIBUTIONS; ENERGIES; OXYGEN; NEUTRONS; O-17; IRON;

D O I：

10.1103/PhysRevLett.132.062702

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The cross section of the 13C(alpha, n)16O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of approximate to 15%. Using a state-of-the-art neutron detection array, we have performed a high resolution differential cross section study covering a broad energy range. These measurements result in a dramatic improvement in the extrapolation of the cross section to stellar energies potentially reducing the uncertainty to approximate to 5% and resolving long standing discrepancies in higher energy data.

引用

页数：7

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