Possible wobbling phenomenon in Xe 125

Mamta Prajapati; Somnath Nag; A. K. Singh; A. Al-Khatib; H. Hübel; A. Neußer-Neffgen; G. B. Hagemann; G. Sletten; B. Herskind; C. R. Hansen; G. Benzoni; A. Bracco; R. V.F. Janssens; M. P. Carpenter; P. Chowdhury

doi:10.1103/PhysRevC.109.034301

Possible wobbling phenomenon in Xe 125

Mamta Prajapati
, Somnath Nag^*
, A. K. Singh
, A. Al-Khatib
, H. Hübel
, A. Neußer-Neffgen
, G. B. Hagemann
, G. Sletten
, B. Herskind
, C. R. Hansen
, G. Benzoni
, A. Bracco
, R. V.F. Janssens
, M. P. Carpenter
, P. Chowdhury

^*Kontaktforfatter

Indian Institute of Technology (BHU) Varanasi
Indian Institute of Technology Kharagpur
Damascus University
University of Bonn
Wagner & Albiger Patent Attorneys
Københavns Universitet
Sezione di Milano
University of North Carolina at Chapel Hill
Triangle Universities Nuclear Laboratory
Argonne National Laboratory
University of Massachusetts Lowell

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › peer review

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Abstract

In the present paper, negative-parity bands based on the νh11/2 configuration in Xe125 have been revisited. This nucleus was populated through the reaction Se82(Ca48,5n)Xe125 at a beam energy of 205 MeV and the corresponding γ rays were observed using the Gammasphere spectrometer. Evidence for first and second phonon wobbling excitations has been established by measurements of directional correlation ratios and angular distributions of the involved γ rays. The observed wobbling energy of the bands involved were compared with the recently published results obtained within the framework of triaxial projected shell-model calculations.

Originalsprog	Engelsk
Artikelnummer	034301
Tidsskrift	Physical Review C
Vol/bind	109
Udgave nummer	3
Antal sider	7
ISSN	2469-9985
DOI	https://doi.org/10.1103/PhysRevC.109.034301
Status	Udgivet - mar. 2024

Finansiering

The authors thank the ANL operations staff at Gammasphere and, in particular, J.P. Greene for help in the target preparation. M.P. acknowledges the fellowship support from the Department of Science and Technology (No. DST/INSPIRE fellowship/2019/IF190275). S.N. acknowledges the financial support from the SERB-DST India under CRG (File No.: CRG/2021/006671). M.P. would also like to thank S. Bhattacharya for his support and valuable advice. The help received from R. M. Clark, P. Fallon, T. L. Khoo, T. Lauritsen, F. Camera, P. Bringel, and C. Engelhardt in this work is gratefully acknowledged. This work is supported by the German BMBF (06 BN 109), the Alexander von Humboldt foundation, Germany, the Danish FNU Council for Natural Sciences, the US Department of Energy, Office of Science, Office of Nuclear Physics, under Contracts No. DE-AC02-06CH11357 (ANL) and DE-AC02-05CH11231 (LBNL), and Grants No. DE-FG02-97ER41041 (UNC), DE-FG02-97ER41033 (TUNL), and DE-FG02-94ER40848 (UML).

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Citationsformater

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title = "Possible wobbling phenomenon in Xe 125",

abstract = "In the present paper, negative-parity bands based on the νh11/2 configuration in Xe125 have been revisited. This nucleus was populated through the reaction Se82(Ca48,5n)Xe125 at a beam energy of 205 MeV and the corresponding γ rays were observed using the Gammasphere spectrometer. Evidence for first and second phonon wobbling excitations has been established by measurements of directional correlation ratios and angular distributions of the involved γ rays. The observed wobbling energy of the bands involved were compared with the recently published results obtained within the framework of triaxial projected shell-model calculations.",

author = "Mamta Prajapati and Somnath Nag and Singh, \{A. K.\} and A. Al-Khatib and H. H{\"u}bel and A. Neu{\ss}er-Neffgen and Hagemann, \{G. B.\} and G. Sletten and B. Herskind and Hansen, \{C. R.\} and G. Benzoni and A. Bracco and Janssens, \{R. V.F.\} and Carpenter, \{M. P.\} and P. Chowdhury",

year = "2024",

month = mar,

doi = "10.1103/PhysRevC.109.034301",

language = "English",

volume = "109",

journal = "Physical Review C",

issn = "2469-9985",

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TY - JOUR

T1 - Possible wobbling phenomenon in Xe 125

AU - Prajapati, Mamta

AU - Nag, Somnath

AU - Singh, A. K.

AU - Al-Khatib, A.

AU - Hübel, H.

AU - Neußer-Neffgen, A.

AU - Hagemann, G. B.

AU - Sletten, G.

AU - Herskind, B.

AU - Hansen, C. R.

AU - Benzoni, G.

AU - Bracco, A.

AU - Janssens, R. V.F.

AU - Carpenter, M. P.

AU - Chowdhury, P.

PY - 2024/3

Y1 - 2024/3

N2 - In the present paper, negative-parity bands based on the νh11/2 configuration in Xe125 have been revisited. This nucleus was populated through the reaction Se82(Ca48,5n)Xe125 at a beam energy of 205 MeV and the corresponding γ rays were observed using the Gammasphere spectrometer. Evidence for first and second phonon wobbling excitations has been established by measurements of directional correlation ratios and angular distributions of the involved γ rays. The observed wobbling energy of the bands involved were compared with the recently published results obtained within the framework of triaxial projected shell-model calculations.

AB - In the present paper, negative-parity bands based on the νh11/2 configuration in Xe125 have been revisited. This nucleus was populated through the reaction Se82(Ca48,5n)Xe125 at a beam energy of 205 MeV and the corresponding γ rays were observed using the Gammasphere spectrometer. Evidence for first and second phonon wobbling excitations has been established by measurements of directional correlation ratios and angular distributions of the involved γ rays. The observed wobbling energy of the bands involved were compared with the recently published results obtained within the framework of triaxial projected shell-model calculations.

U2 - 10.1103/PhysRevC.109.034301

DO - 10.1103/PhysRevC.109.034301

M3 - Journal article

AN - SCOPUS:85186919303

SN - 2469-9985

VL - 109

JO - Physical Review C

JF - Physical Review C

IS - 3

M1 - 034301

ER -

Possible wobbling phenomenon in Xe 125

Abstract

Finansiering

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