Following theoretical predictions of competing prolate and oblate potential-energy minima, we present experimental evidence for the coexistence of prolate and oblate nuclear shapes which are associated in a given nucleus with the same single-quasiproton orbital. Prolate A/ 5 *2 and oblate A/^l bands observed in the ll9 I nucleus are proposed as built on an h n/2 proton with low K and high K, respectively.PACS numbers: 21.10. Re, 23.20.Js, 27.60,+j In a number of odd-proton nuclei for Z > 50, the h u / 2 proton orbital is observed as a low-A^ (K = y ) decoupled AI =*2 rotational band with a prolate quadrupole deformation 1 " 4 of p~-0.2, where K is the angular momentum projection on the axis of deformation. Theoretical calculations for the nh\\/2 orbital, using the Nilsson-Strutinsky procedure, 5 reveal, however, specific (Z,7V) regions where the high-AT (K = -y) oblate energy minimum is competitive with that of the usually observed K = y prolate bandhead. The Nilsson diagram already suggests this general tendency provided the potential-energy surfaces allow significant deformations. Despite these theoretical expectations, high-AT oblate A11/2 proton orbitals have not been observed. The purpose of this study is to search experimentally for the coexistence of this theoretically predicted low-lying h\\/2 oblate proton orbital.
Aluminum nitride (AlN) has a polar crystal structure that is susceptible to electric dipolar interactions. The inversion domains in AlN, similar to those in GaN and other wurtzite-structure materials, decrease the energy associated with the electric dipolar interactions at the expense of inversion-domain boundaries, whose interface energy has not been quantified. We study the atomic structures of six different inversion-domain boundaries in AlN, and compare their interface energies from density functional theory calculations. The low-energy interfaces have atomic structures with similar bonding geometry as those in the bulk phase, while the high-energy interfaces contain N-N wrong bonds. We calculate the formation energy of an inversion domain using the interface energy and dipoles' electric-field energy, and find that the distribution of the inversion domains is an important parameter for the microstructures of AlN films. Using this thermodynamic model, it is possible to control the polarity and microstructure of AlN films by tuning the distribution of an inversion-domain nucleus and by selecting the low-energy synthesis methods.
No abstract
In a recent Letter Nikam and Ring 1 describe the existence of a series of "diabolical points" associated with minimum interaction between configurations of rapidly rotating superfluid nuclei differing by two quasiparticles. They discuss the connection of the diabolical points with the chemical potential X and the angular velocity of rotation co and propose Coulomb-excitation plus pair-transfer experiments circumscribing such points to study the Berry phase factor associated with such a singularity.Experimental contours of constant neutron number in the (X n ,co) plane are shown for erbium and ytterbium isotopes in Fig. 1. The experimental determination of X n and co is discussed in Ref. 2. To obtain data for each neutron number an analysis is made for both the evenspin, positive-parity yrast sequence in even-even isotopes, labeled (;r,a) =( + ,0), and the lowest negative-parity decay sequence in the odd-mass isotopes ( -, j ). Band crossings associated with the excitation of pairs of /13/2 quasineutrons should be identical in these decay sequences. Such a plot is the experimental analog of Fig. 1 of Ref. 1.A predicted 1 feature of the diabolical points, an increased density of single-particle levels associated with vanishing interaction between states differing by two quasiparticles, is observed experimentally (see Fig. 1). Specifically, a "bunching" of experimental levels is observed at hco^0.27MeV for both TV =90-92 and 96-97. Likewise, the observed bunching of experimental levels for TV =90-92 at hco^ 0.42 MeV could be associated with a second band crossing based on the excitation of either two additional /13/2 quasineutrons or another pair of quasineutrons (e.g., negative-parity mixed h9/2 and /7/2X The band crossing observed at hco^O.42 MeV has been associated with the excitation of a pair of A11/2 quasiprotons 3 with a strong interaction between the associated zero-and two-quasiprotons levels. No increased density of quasineutron states should be associated with such a quasiproton band crossing. Therefore, the physical basis for this increased density of states at high frequency is not yet known.In conclusion, the increased density of single-quasiparticle states, i.e., a diabolical point, predicted 1 at weakly interacting band crossings associated with the excitation of pairs of quasiparticles, is observed. Such data identify candidates for Coulomb-excitation plus twoparticle-transfer studies sensitive to the Berry phase factor associated with circumscribing such a diabolical point. 40361. Discussions with P. Ring are acknowledged. I 91 93 | 95 97J 99 | -9.0 -8.5 -8.0 -7.5 Xn(MeV) FIG. 1. Empirical contours of constant neutron number, TV, as a function of X n and co. For reference, the observed rotational frequencies of the lowest /13/2 quasineutron band crossings in the even-even yrast sequences are indicated by the horizontal dashed lines labeled hco c . The experimental data sources are summarized in Refs. 2 and 4.
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.
customersupport@researchsolutions.com
10624 S. Eastern Ave., Ste. A-614
Henderson, NV 89052, USA
This site is protected by reCAPTCHA and the Google Privacy Policy and Terms of Service apply.
Copyright © 2024 scite LLC. All rights reserved.
Made with 💙 for researchers
Part of the Research Solutions Family.