6533b851fe1ef96bd12a9769

RESEARCH PRODUCT

Nonquenched Isoscalar Spin-M1Excitations insd-Shell Nuclei

P. Von Neumann-coselHiroaki MatsubaraM. YosoiLucia PopescuAtsushi TamiiPetr NavrátilHitoshi NakadaAchim RichterWataru HoriuchiYukie MaedaKatsumasa FujitaR. NevelingJ. CarterH. OkamuraTakahiro KawabataF. D. SmitYohei ShimizuS. KuroitaYoshiko SasamotoYasuhiko YamadaHiroshi TokiedaKichiji HatanakaSatoshi SakaguchiK. SudaM. ItohYuji TameshigeJuzo ZenihiroMasanori DozonoB. RubioYasuhiro SakemiI. PoltoratskaHarutaka SakaguchiYoshitaka FujitaT. AdachiY. ShimbaraHisanori Fujita

subject

PhysicsMatrix (mathematics)IsovectorProtonIsospinIsoscalarNuclear TheoryStochastic matrixGeneral Physics and AstronomyInelastic scatteringAtomic physicsNuclear ExperimentSpin (physics)

description

Differential cross sections of isoscalar and isovector spin-M1 (0(+)→1(+)) transitions are measured using high-energy-resolution proton inelastic scattering at E(p)=295  MeV on (24)Mg, (28)Si, (32)S, and (36)Ar at 0°-14°. The squared spin-M1 nuclear transition matrix elements are deduced from the measured differential cross sections by applying empirically determined unit cross sections based on the assumption of isospin symmetry. The ratios of the squared nuclear matrix elements accumulated up to E(x)=16  MeV compared to a shell-model prediction are 1.01(9) for isoscalar and 0.61(6) for isovector spin-M1 transitions, respectively. Thus, no quenching is observed for isoscalar spin-M1 transitions, while the matrix elements for isovector spin-M1 transitions are quenched by an amount comparable with the analogous Gamow-Teller transitions on those target nuclei.

https://doi.org/10.1103/physrevlett.115.102501