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Mirror Symmetry Up to the Band Termination in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>49</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi>Mn</mml:mi></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>49</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi>Cr</mml:mi></mml:math>

C. D. O’LearySchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United KingdomM. A. BentleySchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United KingdomD. E. AppelbeSchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United KingdomD. M. CullenSchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United KingdomS. ErtürkSchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United KingdomR. A. BarkSchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United KingdomA. MajSchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United KingdomTadashi SaitohSchool of Sciences, Staffordshire University, College Road, Stoke-on-Trent ST4 2DE, United Kingdom
1997lv
ABI

Abstract

High-spin states have been investigated in the mirror pair nuclei ${}^{49}\mathrm{Cr}$ ( $Z\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}24$, $N\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}25$) and ${}^{49}\mathrm{Mn}$ $(Z\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}25,N\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}24)$. Mirror symmetry up to the band termination at about 10.7 MeV has been established. A comparison of the corresponding energy levels of the pair shows, for the first time, that the Coulomb energy difference approaches zero as the band termination is approached. This is explained intuitively in terms of a pure ${f}_{\frac{7}{2}}$ shell framework. For ${}^{49}\mathrm{Cr}$, excellent agreement is found between the data and recent full $\mathrm{pf}$-shell calculations.

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