In-beam gamma-ray and electron spectroscopy following the 75As(p, n)75Se reaction

Agarwal, Y. K. ; Baba, C. V. K. ; Bharathi, S. M. ; Bhattacherjee, S. K. ; Lal, B. ; Sahai, Baldev (1974) In-beam gamma-ray and electron spectroscopy following the 75As(p, n)75Se reaction Pramana - Journal of Physics, 3 (4). pp. 243-260. ISSN 0304-4289

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Official URL: http://www.ias.ac.in/j_archive/pramana/3/4/243-260...

Related URL: http://dx.doi.org/10.1007/BF02872243

Abstract

The level scheme of75Se has been studied through the75As (p, n) reaction at proton energies from 1.5 to 5.0 MeV.γ-ray and internal conversion electron measurements were made using NaI (T1) and Ge(Li) detectors and a six-gap electron spectrometer. A proportional counter and a thin window NaI(T1) detector were used to detect γ-rays with energies less than 30 keV. The level scheme has been established by observing the thresholds of various γ-rays and by γ-γ and e--γ coincidence measurements. New levels at 133.0, 293.2, 790.0, 953.0, 1020.8, 1184.3, 1198.5 and 1258.2 keV not observed in earlier (p, n) studies have been established. Conversion coefficients of most of the low-lying transitions have been determined. Angular distributions of some of the γ-rays were also measured and compared with the statistical model calculations. Definite JΠ assignments have been made to most of the low-lying levels. Life-times of the 112.1, 133.0, 286.7 and 293.2 keV levels have been measured to be 0.69±0.12, 5.3±0.6, 1.35±0.15 and 31±2 nsec respectively. The reduced transition probabilities for various low-lying transitions have been determined and compared with recent calculations. The ½ - and 9/2+ levels hitherto unknown in this nucleus has been identified. The structure of the low-lying levels is discussed in terms of the existing models.

Item Type:Article
Source:Copyright of this article belongs to Indian Academy of Sciences.
Keywords:Nuclear reactionAs(p,N)Se; γ-ray angular distribution; Nuclear structure; Deformation; Internal conversion coefficients
ID Code:3520
Deposited On:12 Oct 2010 04:21
Last Modified:16 May 2016 14:18

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