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Title: Systematics of first and second shape transition temperatures in heavy nuclei

Abstract

Thirty-one even-even isotopes ({ital Z}=72{endash}80 and {ital N}=110{endash}126) have two shape transition temperatures, where {ital T}{sub {ital c}2}{approx_gt}{ital T}{sub {ital c}1}. For temperatures above {ital T}{sub {ital c}1}, the equilibrium shape is spherical if the rotational frequency is zero. For these 31 nuclei, a slow rotation of the spherical shape creates a {ital prolate} shape rotating about its symmetry axis if the temperature is between {ital T}{sub {ital c}1} and {ital T}{sub {ital c}2}, and an oblate shape rotating about its symmetry axis if the temperature is above {ital T}{sub {ital c}2}. {copyright} {ital 1996 The American Physical Society.}

Authors:
;  [1]
  1. Physics Department, Tulane University, New Orleans, Louisiana 70118 (United States)
Publication Date:
OSTI Identifier:
383327
Resource Type:
Journal Article
Journal Name:
Physical Review, C
Additional Journal Information:
Journal Volume: 54; Journal Issue: 3; Other Information: PBD: Sep 1996
Country of Publication:
United States
Language:
English
Subject:
66 PHYSICS; TRANSITION TEMPERATURE; SHAPE; HEAVY NUCLEI; EVEN-EVEN NUCLEI; EQUILIBRIUM; ROTATION

Citation Formats

Goodman, A L, and Jin, T. Systematics of first and second shape transition temperatures in heavy nuclei. United States: N. p., 1996. Web. doi:10.1103/PhysRevC.54.1165.
Goodman, A L, & Jin, T. Systematics of first and second shape transition temperatures in heavy nuclei. United States. https://doi.org/10.1103/PhysRevC.54.1165
Goodman, A L, and Jin, T. 1996. "Systematics of first and second shape transition temperatures in heavy nuclei". United States. https://doi.org/10.1103/PhysRevC.54.1165.
@article{osti_383327,
title = {Systematics of first and second shape transition temperatures in heavy nuclei},
author = {Goodman, A L and Jin, T},
abstractNote = {Thirty-one even-even isotopes ({ital Z}=72{endash}80 and {ital N}=110{endash}126) have two shape transition temperatures, where {ital T}{sub {ital c}2}{approx_gt}{ital T}{sub {ital c}1}. For temperatures above {ital T}{sub {ital c}1}, the equilibrium shape is spherical if the rotational frequency is zero. For these 31 nuclei, a slow rotation of the spherical shape creates a {ital prolate} shape rotating about its symmetry axis if the temperature is between {ital T}{sub {ital c}1} and {ital T}{sub {ital c}2}, and an oblate shape rotating about its symmetry axis if the temperature is above {ital T}{sub {ital c}2}. {copyright} {ital 1996 The American Physical Society.}},
doi = {10.1103/PhysRevC.54.1165},
url = {https://www.osti.gov/biblio/383327}, journal = {Physical Review, C},
number = 3,
volume = 54,
place = {United States},
year = {Sun Sep 01 00:00:00 EDT 1996},
month = {Sun Sep 01 00:00:00 EDT 1996}
}