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Synthesis of superheavy nuclei has been achieved recently through hot fusion reactions. A systematic theoretical calculation of determining the stability of the superheavy nucleus Z=114 is studied in the context of angular momentum and temperature. The level density can provide clues to the applicability of the statistical model which is only correct for a high density of excited states. The collapse of pairing correlation at moderately higher spin and at low temperature causes a shape change and stability at higher spin is also expected. The drop in separation energy is closely associated with the structural changes in the rotating nuclei; relative increase in neutron emission probability around certain values of temperature may be construed as evidence for the shape transition. Such effects are not obtained for 298 114. Hence this statistical study reveals a higher stability for 298 114 against temperature and angular momentum.
S. Santhosh Kumar. 2014. \u201cStructural Stability of Long Lived Superheavy Nucleus 298114\u201d. Global Journal of Science Frontier Research - A: Physics & Space Science GJSFR-A Volume 14 (GJSFR Volume 14 Issue A7): .
Crossref Journal DOI 10.17406/GJSFR
Print ISSN 0975-5896
e-ISSN 2249-4626
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Total Score: 102
Country: India
Subject: Global Journal of Science Frontier Research - A: Physics & Space Science
Authors: S. Santhosh Kumar, A. Victor Babu (PhD/Dr. count: 0)
View Count (all-time): 123
Total Views (Real + Logic): 4150
Total Downloads (simulated): 2309
Publish Date: 2014 12, Mon
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Synthesis of superheavy nuclei has been achieved recently through hot fusion reactions. A systematic theoretical calculation of determining the stability of the superheavy nucleus Z=114 is studied in the context of angular momentum and temperature. The level density can provide clues to the applicability of the statistical model which is only correct for a high density of excited states. The collapse of pairing correlation at moderately higher spin and at low temperature causes a shape change and stability at higher spin is also expected. The drop in separation energy is closely associated with the structural changes in the rotating nuclei; relative increase in neutron emission probability around certain values of temperature may be construed as evidence for the shape transition. Such effects are not obtained for 298 114. Hence this statistical study reveals a higher stability for 298 114 against temperature and angular momentum.
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