IMPROTANCE OF PHOTO-BETA PROCESS FOR SYNTHESIS OF P ELEMENTS IN STELLAR CONDITIONS

被引：8

作者：

ARNOULD, M

机构：

来源：

关键词：

D O I：

10.1016/0375-9474(67)90129-7

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：

引用

页码：657 / &

共 12 条

[1] BAHCALL JN, 1963, AP J, V138, P437
[2] BLATT JM, 1952, THEORETICAL NUCLEAR, P670
[3] SYNTHESIS OF THE ELEMENTS IN STARS
BURBIDGE, EM
BURBIDGE, GR
FOWLER, WA
HOYLE, F
[J]. REVIEWS OF MODERN PHYSICS, 1957, 29 (04) : 547 - 650
[4] FOWLER WA, 1964, AP J S9
[5] Frank-Kamenetskii D. A., 1961, SOV ASTRON, V5, P66
[6] STELLAR SYNTHESIS OF THE PROTON-RICH HEAVY ELEMENTS
ITO, K
[J]. PROGRESS OF THEORETICAL PHYSICS, 1961, 26 (06): : 990 - 1004
[7] MALKIEL GS, 1963, SOV ASTRON, V7, P207
[8] POSITRON-CAPTURE PROCESSES AS A POSSIBLE SOURCE OF P ELEMENTS
REEVES, H
STEWART, P
[J]. ASTROPHYSICAL JOURNAL, 1965, 141 (04) : 1432 - &
[9] Rose M. E., 1955, BETA GAMMA RAY SPECT
[10] SHAW PB, 1965, PHYS REV, V140, P1433