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??In this paper, we compare the smallest order statistics arising from multiple-outlier models when the numbers of independent and identically distributed random variables are different. Let and denote the smallest order statistics among, and, respectively, whereand. We then prove that $ and are ordered in terms of the usual stochastic order, hazard rate order and likelihood ratio order under the majorization relationship between and.  相似文献   
2.
The proton resonant properties in 18Ne, which determine the reaction rate of the key stellar 14O(α,p)17F reaction, have been studied by using a technique of proton resonant elastic scattering of 17F+p. A 4.22 MeV/nucleon 17F radioactive ion (RI) beam was produced via a projectile-fragmentation reaction, and separated by a Radioactive Ion Beam Line in Lanzhou (RIBLL). By bombarding a thick (CH2)n target, the energy spectra of the recoiled protons were measured by two ΔE-E silicon telescopes at the center-of-...  相似文献   
3.
He  JianJun  Hu  Jun  Xu  ShiWei  Chen  ZhiQiang  Zhang  XueYing  Wang  JianSong  Yu  XiangQing  Zhang  LiYong  Li  Long  Yang  YanYun  Ma  Peng  Zhang  XueHeng  Hu  ZhengGuo  Guo  ZhongYan  Xu  Xing  Yuan  XiaoHua  Lu  Wan  Yu  YuHong  Zang  YongDong  Tang  ShuWen  Ye  RuiPing  Chen  JinDa  Jin  ShiLun  Du  ChengMing  Wang  ShiTao  Ma  JunBing  Liu  LongXiang  Bai  Zhen  Lei  XiangGuo  Sun  ZhiYu  Zhang  YuHu  Zhou  XiaoHong  Xu  HuShan  Su  Jun  Li  ErTao  Wang  HongWei  Tian  WenDong  Li  XiangQing 《中国科学:物理学 力学 天文学(英文版)》2011,54(1):32-36
The proton resonant properties in 18Ne, which determine the reaction rate of the key stellar 14O(α,p)17F reaction, have been studied by using a technique of proton resonant elastic scattering of 17F+p. A 4.22 MeV/nucleon 17F radioactive ion (RI) beam was produced via a projectile-fragmentation reaction, and separated by a Radioactive Ion Beam Line in Lanzhou (RIBLL). By bombarding a thick (CH2) n target, the energy spectra of the recoiled protons were measured by two ΔE-E silicon telescopes at the center-of-mass scattering angles of θ c.m.≈175°±5°, θ c.m.≈152°±8°, respectively. Several proton resonances in 18Ne were observed clearly. A further R-matrix analysis of the experimental data is under way to determine the resonant parameters. The present work reports the preliminary results briefly.  相似文献   
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