Expressions for the O-14(alpha,p)F-17 and F-17(p,gamma)Ne-18 astrophysical reaction rates

被引：16

作者：

Bardayan, DW ^{[1
]}

Smith, MS ^{[1
]}

机构：

[1] OAK RIDGE NATL LAB, DIV PHYS, OAK RIDGE, TN 37831 USA

来源：

PHYSICAL REVIEW C | 1997年 / 56卷 / 03期

关键词：

D O I：

10.1103/PhysRevC.56.1647

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The O-14(alpha,p)F-17 and F-17(p,gamma)Ne-18 astrophysical reaction rates are needed to determine the breakout conditions from the hot CNO cycle into the rapid proton capture process in hot stellar environments. We have examined recent indirect experimental measurements of these reactions and generated analytical expressions for the reaction rates as a function of temperature. We also present a correction to the previously reported calculation of the F-17(p,gamma) rate.

引用

页码：1647 / 1650

页数：4

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