High spin study of 104Ag nucleus

Kaushik Katre, P. V.Madhusudhan Rao, K. Suryanarayana, A. Tejaswi, M. Kumar Raju, M. Ratna Raju, D. Vijayal Lakshmi, T. Sashi Reddy, J. Matta, A. D. Ayangeakaa, U. Garg, R. Raut, S. S. Ghugre, R. Palit, S. Chakraborty, S. Muralithar, R. P. Singh

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

High spin states in 104Ag were populated via heavy-ion (32S) induced fusion evaporation reaction at a beam energy of 110 MeV. The de-exciting γ-rays were detected by 18 Compton suppressed HPGe clover detectors, placed in different (θ, φ) angles. Spin of several excited states were assigned firmly from the present angular correlation measurement.

Original languageEnglish
Title of host publicationECS Transactions
PublisherInstitute of Physics
Pages12577-12584
Number of pages8
Edition1
ISBN (Electronic)9781607685395
DOIs
StatePublished - 2022
Externally publishedYes
Event1st International Conference on Technologies for Smart Green Connected Society 2021, ICTSGS 2021 - Virtual, Online, United States
Duration: Nov 29 2021Nov 30 2021

Publication series

NameECS Transactions
Number1
Volume107
ISSN (Print)1938-6737
ISSN (Electronic)1938-5862

Conference

Conference1st International Conference on Technologies for Smart Green Connected Society 2021, ICTSGS 2021
Country/TerritoryUnited States
CityVirtual, Online
Period11/29/2111/30/21

Funding

We would like to acknowledge BARC-TIFR pelletron staff for delivering stable beam of 32S during the experiment. We acknowledge the help of all INGA collaboration. Authors gratefully acknowledge Department of Science and Technology (DST) for INGA project (No.IR/S2/PF-30/2003/I) and CSIR for financial support. We would also like to thanks R. Bhattacharjee, S. S. Bhattacharjee, S. Samanta, S. Das, N. Ghosh, A. K. Sinha, S. Mukhopadhyay, L. Dhanu, B. K. Nayak, D. C. Biswas, A. Y. Deo, S. K. Tandel, N. Kaur, Ashok Kumar, S. Saha, J. Sethi, S. Chattopadhyay for their help during the experiment. This work has been supported in part by the U. S. National Science Foundation (Grants No. PHY-1068192 and No. PHY-2011890).

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