Investigating the 16O + 12C reaction over a wide range of energies

被引：1

作者：

Gridnev K.A. ^{[1
]}

Burtebayev N. ^{[2
]}

Maltsev N.A. ^{[1
]}

Amangeldi N. ^{[3
]}

Hamada S. ^{[4
]}

机构：

[1] St. Petersburg State University, St. Petersburg

[2] Institute of Nuclear Physics, National Nuclear Center, Almaty

[3] Eurasia National University, Astana

[4] Kazakh National University, Almaty

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2011年 / 75卷 / 7期

关键词：

Elastic Scattering; Nuclear Matter; Optical Model; Optical Potential; Distorted Wave;

D O I：

10.3103/S1062873811070173

中图分类号：

学科分类号：

摘要：

The main aim of this work was to describe the reactions of elastic scattering of 16O + 12C over a wide range of energies in an optical model with an l-dependent core. We obtained a value for the compress- ibility coefficient that agreed with the one found from data on the giant monopole resonance. We considered the elastic transfer of an α particle to reproduce the cross section in the reverse hemisphere. © 2011 Allerton Press, Inc.

引用

页码：961 / 963

页数：2

共 50 条

[1] The 12C(α,γ)16O reaction at astrophysical energies
Braizinha, B
Eiró, AM
Santos, FD
NUCLEAR PHYSICS A, 2001, 689 (1-2) : 369C - 372C
[2] Role of the inelastic transfer channel in elastic 16O + 12C scattering over a wide range of energies
K. A. Gridnev
N. A. Mal’tsev
N. Burtebaev
N. Amangel’dy
Sh. Hamada
Bulletin of the Russian Academy of Sciences: Physics, 2012, 76 (8) : 934 - 937
[3] Impact of 16O(γ, α)12C measurements on the 12C(α, γ)16O astrophysical reaction rate
Holt, R. J.
Filippone, B. W.
Pieper, Steven C.
PHYSICAL REVIEW C, 2019, 99 (05)
[4] A new study for 16O(γ,α)12C at the energies of nuclear astrophysics interest:: The inverse of key nucleosynthesis reaction 12C(α,γ)16O
Xu, Y.
Xu, W.
Ma, Y. G.
Guo, W.
Chen, J. G.
Cai, X. Z.
Wang, H. W.
Wang, C. B.
Lu, G. C.
Shen, W. Q.
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2007, 581 (03): : 866 - 873
[5] α-Spectroscopic factor of 16Ogs from the 12C(16O,12C)16O reaction
Morais, M. C.
Lichtenthaeler, R.
NUCLEAR PHYSICS A, 2011, 857 (01) : 1 - 8
[6] 16O(e,e′α)12C measurements and the 12C(α,γ)16O astrophysical reaction rate
Potterveld, D. H.
Filippone, B. W.
Holt, R. J.
Friscic, I.
PHYSICAL REVIEW C, 2024, 110 (03)
[7] Impact of 16O(e, e′ α)12C measurements on the 12C(α, γ)16O astrophysical reaction rate
Holt, R. J.
Filippone, B. W.
PHYSICAL REVIEW C, 2019, 100 (06)
[8] Comments on the 12C(α, γ)16O reaction rate
Buchmann, L
NUCLEAR PHYSICS A, 2005, 758 : 355C - 362C
[9] Astrophysical reaction rate of 12C(α, γ)16O
Kunz, R
Fey, M
Jaeger, M
Mayer, A
Hammer, JW
Staudt, G
Harissopulos, S
Paradellis, T
ASTROPHYSICAL JOURNAL, 2002, 567 (01): : 643 - 650
[10] The 12C(α,γ)16O reaction, in the laboratory and in the stars
de Boer, R. J.
Best, A.
Brune, C. R.
Chieffi, A.
Hebborn, C.
Imbriani, G.
Liu, W. P.
Shen, Y. P.
Timmes, F. X.
Wiescher, M.
EUROPEAN PHYSICAL JOURNAL A, 2025, 61 (04):

← 1 2 3 4 5 →