Proposed s = ± 1 octupole bands in Xe 140

doi:10.1103/PhysRevC.93.064321

Title: Proposed $s = \pm 1$ octupole bands in ${}^{140}{Xe}$

Article Details
Other Related Research

Authors:: Huang, Y. ; Zhu, S. J. ; Hamilton, J. H. ; Wang, E. H. ; Ramayya, A. V. ; Xiao, Z. G. ; Li, H. J. ; Luo, Y. X. ; Rasmussen, J. O. ; Ter-Akopian, G. M. ; Oganessian, Yu. Ts.

Publication Date:: 2016-06-20

Grant/Contract Number:: FG05-88ER40407; AC03-76SF00098

Type:: Publisher's Accepted Manuscript

Journal Name:: Physical Review C

Additional Journal Information:: Journal Name: Physical Review C Journal Volume: 93 Journal Issue: 6; Journal ID: ISSN 2469-9985

Publisher:: American Physical Society

Sponsoring Org:: USDOE

Country of Publication:: United States

Language:: English

OSTI Identifier:: 1258307


                    Huang, Y., Zhu, S. J., Hamilton, J. H., Wang, E. H., Ramayya, A. V., Xiao, Z. G., Li, H. J., Luo, Y. X., Rasmussen, J. O., Ter-Akopian, G. M., and Oganessian, Yu. Ts.. Proposed s = ± 1 octupole bands in Xe 140.  United States: N. p.,  
        Web.  doi:10.1103/PhysRevC.93.064321.

Copy to clipboard


                    Huang, Y., Zhu, S. J., Hamilton, J. H., Wang, E. H., Ramayya, A. V., Xiao, Z. G., Li, H. J., Luo, Y. X., Rasmussen, J. O., Ter-Akopian, G. M., & Oganessian, Yu. Ts.. Proposed s = ± 1 octupole bands in Xe 140.  United States.  doi:10.1103/PhysRevC.93.064321.

Copy to clipboard


                    Huang, Y., Zhu, S. J., Hamilton, J. H., Wang, E. H., Ramayya, A. V., Xiao, Z. G., Li, H. J., Luo, Y. X., Rasmussen, J. O., Ter-Akopian, G. M., and Oganessian, Yu. Ts.. 2016.  
        "Proposed s = ± 1 octupole bands in Xe 140".  United States.  
        doi:10.1103/PhysRevC.93.064321.

Copy to clipboard


                    
@article{osti_1258307,

  title        = {Proposed s = ± 1 octupole bands in Xe 140},

  author       = {Huang, Y. and Zhu, S. J. and Hamilton, J. H. and Wang, E. H. and Ramayya, A. V. and Xiao, Z. G. and Li, H. J. and Luo, Y. X. and Rasmussen, J. O. and Ter-Akopian, G. M. and Oganessian, Yu. Ts.},

  abstractNote = {},

  doi          = {10.1103/PhysRevC.93.064321},

  journal      = {Physical Review C},

  number       = 6,

  volume       = 93,

  place        = {United States},

  year         = {2016},

  month        = {6}

}

Copy to clipboard

Free Publicly Accessible Full Text
Accepted Manuscript (Publisher)
Publisher's Version of Record
10.1103/PhysRevC.93.064321
https://doi.org/10.1103/PhysRevC.93.064321

Citation Metrics
Cited by: 4works
Citation information provided by
Web of Science

Save / Share this Record
Export Metadata
- Endnote
- RIS
- Excel
- CSV
- XML
Save to My Library
Send to Email

Send to Email

Email address:

Content:

Similar Records

Similar records in DOE PAGES and OSTI.GOV collections:

New measurement of the $α$ asymptotic normalization coefficient of the ${1 / 2}^{+}$ state in ${}^{17}O$ at 6.356 MeV that dominates the ${}^{13}C (α, n) {}^{16}O$ reaction rate at temperatures relevant for the $s$ process

Journal Article Avila, M. L. ; Rogachev, G. V. ; Koshchiy, E. ; ... April 2015 - Physical Review C

Cited by 8Full Text Available
Comprehensive sets of ${}^{124}{Xe} (n, γ) {}^{125}{Xe}$ and ${}^{124}{Xe} (n, 2 n) {}^{123}{Xe}$ cross-section data for assessment of inertial-confinement deuterium-tritium fusion plasma

Journal Article Bhike, Megha ; Fallin, B. ; Gooden, M. E. ; ... January 2015 - Physical Review C

Cited by 2Full Text Available
Measurement of the relative yields of $ψ (2 S)$ to $ψ (1 S)$ mesons produced at forward and backward rapidity in $p + p$ , $p + Al$ , $p + Au$ , and ${}^{3}{He} + Au$ collisions at $\sqrt{s_{NN}} = 200$ GeV

Journal Article Adare, A. ; Aidala, C. ; Ajitanand, N. N. ; ... March 2017 - Physical Review C

The PHENIX Collaboration has measured the ratio of the yields of ψ(2S) to ψ(1S) mesons produced in p+p, p+Al, p+Au, and ³He+Au collisions at √ ^sNN = 200 GeV over the forward and backward rapidity intervals 1.2 < |y| < 2.2. We find that the ratio in p+p collisions is consistent with measurements at other collision energies. In collisions with nuclei, we find that in the forward (p-going or ³He-going) direction, the relative yield of ψ(2S) mesons to ψ(1S) mesons is consistent with the value measured in p+p collisions. However, in the backward (nucleus-going) direction, the ψ(2S) meson is preferentiallymore »« less
Cited by 4Full Text Available
Measurement of the relative yields of $ψ (2 S)$ to $ψ (1 S)$ mesons produced at forward and backward rapidity in $p + p$ , $p + Al$ , $p + Au$ , and ${}^{3}{He} + Au$ collisions at $\sqrt{s_{NN}} = 200$ GeV

Journal Article Adare, A. ; Aidala, C. ; Ajitanand, N. N. ; ... March 2017 - Physical Review C

The PHENIX Collaboration has measured the ratio of the yields of ψ(2S) to ψ(1S)mesons produced in p + p, p + Al, p + Au, and 3He+Au collisions at √ sNN = 200 GeV over the forward and backward rapidity intervals 1.2 < |y| < 2.2. We find that the ratio in p + p collisions is consistent with measurements at other collision energies. In collisions with nuclei, we find that in the forward (p-going or 3He-going) direction, the relative yield of ψ(2S) mesons to ψ(1S) mesons is consistent with the value measured in p + p collisions. However, inmore »« less
Cited by 4Full Text Available
Measurement of the relative yields of $ψ (2 S)$ to $ψ (1 S)$ mesons produced at forward and backward rapidity in $p + p$ , $p + Al$ , $p + Au$ , and ${}^{3}{He} + Au$ collisions at $\sqrt{s_{NN}} = 200$ GeV

Journal Article Adare, A. ; Aidala, C. ; Ajitanand, N. N. ; ... March 2017 - Physical Review C

The PHENIX Collaboration has measured the ratio of the yields of ψ(2S) to ψ(1S) mesons produced in p+p, p+Al, p+Au, and 3He+Au collisions at sNN√=200 GeV over the forward and backward rapidity intervals 1.2<|y|<2.2. We find that the ratio in p+p collisions is consistent with measurements at other collision energies. In collisions with nuclei, we find that in the forward (p-going or 3He-going) direction, the relative yield of ψ(2S) mesons to ψ(1S) mesons is consistent with the value measured in \pp collisions. However, in the backward (nucleus-going) direction, the ψ(2S) is preferentially suppressed by a factor of ~2. This suppressionmore »« less
Cited by 4Full Text Available

Access journal articles and accepted manuscripts resulting from DOE research funding

Title: Proposed s = ± 1 octupole bands in Xe 140

Access journal articles and accepted manuscripts
resulting from DOE research funding

Title: Proposed $s = \pm 1$ octupole bands in ${}^{140}{Xe}$