Mass measurements for nuclear astrophysics with JYFLTRAP

被引：2

作者：

Kankainen, A. ^{[1
]}

机构：

[1] Univ Jyvaskyla, Dept Phys, Jyvaskyla 40014, Finland

来源：

HYPERFINE INTERACTIONS | 2011年 / 199卷 / 1-3期

基金：

芬兰科学院;

关键词：

Atomic masses; Penning traps; Explosive hydrogen burning in novae; rp process; nu p process; RP-PROCESS; PENNING TRAPS; RAMSEY METHOD; NUCLEOSYNTHESIS; SPECTROMETRY; EXCITATION; ENERGIES;

D O I：

10.1007/s10751-011-0317-5

中图分类号：

O64 [物理化学（理论化学）、化学物理学]; O56 [分子物理学、原子物理学];

学科分类号：

070203 ; 070304 ; 081704 ; 1406 ;

摘要：

Over 90 neutron-deficient nuclides between C-10 and I-111 have been measured at the JYFLTRAP mass spectrometer with a precision of better than 10 keV. Masses of these nuclides are important for modeling astrophysical rp and nu p processes and nucleosynthesis occurring in novae. Here, a review of the mass measurement programme of the neutron-deficient nuclides performed at JYFLTRAP for nuclear astrophysics studies is given.

引用

页码：221 / 230

页数：10

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