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arXiv 2004.14101nucl-exnucl-th
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核质量测量绘制原子核和吸积中子星的结构

Nuclear Mass Measurements Map the Structure of Atomic Nuclei and Accreting Neutron Stars

Z. Meisel, S. George, S. Ahn, D. Bazin, B. A. Brown, J. Browne, J. F. Carpino, H. Chung, R. H. Cyburt, A. Estradé, M. Famiano, A. Gade, C. Langer, M. Matoš, W. … 展开作者

Z. Meisel, S. George, S. Ahn, D. Bazin, B. A. Brown, J. Browne, J. F. Carpino, H. Chung, R. H. Cyburt, A. Estradé, M. Famiano, A. Gade, C. Langer, M. Matoš, W. Mittig, F. Montes, D. J. Morrissey, J. Pereira, H. Schatz, J. Schatz, M. Scott, D. Shapira, K. Smith, J. Stevens, W. Tan, O. Tarasov, S. Towers, K. Wimmer, J. R. Winkelbauer, J. Yurkon, R. G. T. Zegers

摘要:

我们目前的质量过剩(ME)的富中子同位素的Ar通过Fe,通过TOF- $Bρ$质谱在国家超导回旋加速器实验室。我们的新结果显着降低了系统的不确定性相对于先前的分析,使第一次确定ME为$^{58,59}{\rm Ti}$,$^{62}{\rm V}$,$^{65}{\rm Cr}$,$^{67,68}{\rm Mn}$,和$^{69,70}{\rm Fe}$。结果表明,$N=34$亚壳层在Sc处减弱,Ti处消失,Mn处没有$N=40$亚壳层.这导致了一个较冷的中子星外壳,突出了原子核和中子星结构之间的联系。

英文摘要:

We present mass excesses (ME) of neutron-rich isotopes of Ar through Fe, obtained via TOF-$Bρ$ mass spectrometry at the National Superconducting Cyclotron Laboratory. Our new results have significantly reduced systematic uncertainties relative to a prior analysis, enabling the first determination of ME for $^{58,59}{\rm Ti}$, $^{62}{\rm V}$, $^{65}{\rm Cr}$, $^{67,68}{\rm Mn}$, and $^{69,70}{\rm Fe}$. Our results show the $N=34$ subshell weaken at Sc and vanish at Ti, along with the absence of an $N=40$ subshell at Mn. This leads to a cooler accreted neutron star crust, highlighting the connection between the structure of nuclei and neutron stars.

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