Rodríguez D, Kolhinen V S, Audi G, Aystö J, Beck D, Blaum K, Bollen G, Herfurth F, Jokinen A, Kellerbauer A, Kluge H-J, Oinonen M, Schatz H, Sauvan E, Schwarz S
GSI, Darmstadt, Germany.
Phys Rev Lett. 2004 Oct 15;93(16):161104. doi: 10.1103/PhysRevLett.93.161104. Epub 2004 Oct 14.
The mass of one of the three major waiting points in the astrophysical rp process 72Kr was measured for the first time with the Penning trap mass spectrometer ISOLTRAP. The measurement yielded a relative mass uncertainty of deltam/m=1.2x10(-7) (deltam=8 keV). (73,74)Kr, also needed for astrophysical calculations, were measured with more than 1 order of magnitude improved accuracy. We use the ISOLTRAP masses of 72-74Kr to reanalyze the role of 72Kr (T(1/2)=17.2 s) in the rp process during x-ray bursts and conclude that 72Kr is a strong waiting point delaying the burst duration with at least 80% of its beta-decay half-life.
利用潘宁阱质谱仪ISOLTRAP首次测量了天体物理rp过程中三个主要等待点之一的72Kr的质量。测量得到的相对质量不确定度为δm/m = 1.2×10⁻⁷(δm = 8 keV)。天体物理计算中也需要的(73,74)Kr,测量精度提高了一个多数量级。我们利用72 - 74Kr的ISOLTRAP质量重新分析了72Kr(T(1/2)=17.2 s)在X射线暴期间rp过程中的作用,并得出结论:72Kr是一个强大的等待点,将暴持续时间延迟至少80%的β衰变半衰期。