Litcius/Paper detail

Systematic study of near-yrast band structures in odd-mass <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Pr</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>125</mml:mn><mml:mo>−</mml:mo><mml:mn>137</mml:mn></mml:mrow></mml:mmultiscripts></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Pm</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>127</mml:mn><mml:mo>−</mml:mo><mml:mn>139</mml:mn></mml:mrow></mml:mmultiscripts></mml:math> isotopes

S. Jehangir, G. H. Bhat, N. Rather, J. A. Sheikh, R. Palit

2021Physical review. C17 citationsDOIOpen Access PDF

Abstract

In the present work, the basis space in the triaxial projected shell-model approach is expanded to include three and five quasiparticle configurations for odd-proton systems. This extension allows us to investigate the high-spin band structures observed in odd-proton systems up to and including the second band-crossing region and, as a first major application of this development, the high-spin properties are investigated for odd-mass $^{125\ensuremath{-}137}\mathrm{Pr}$ and $^{127\ensuremath{-}139}\mathrm{Pm}$ isotopes. It is shown that band crossings in the studied isotopes have mixed structures with the first crossing dominated by one-proton coupled to two-neutron configuration for the lighter isotopes which then changes to three-proton configuration with increasing neutron number. Furthermore, $\ensuremath{\gamma}$ bands based on quasiparticle states are also delineated in the present work, and it is predicted that these band structures built on three-quasiparticle configurations become favored in energy for heavier systems in the high-spin region.

Topics & Concepts

YrastQuasiparticlePhysicsNeutronProtonIsotopeNeutron numberSpin (aerodynamics)Atomic physicsNuclear physicsCondensed matter physicsNeutron temperatureThermodynamicsNeutron cross sectionSuperconductivityNuclear physics research studiesAstronomical and nuclear sciencesAstro and Planetary Science