Institute of Physics Nuclear Spin Measurements in Some Nuclides of the Alkali Elements Rubidium and Francium
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SCf UPPSALA UNIVERSITY INSTITUTE OF PHYSICS NUCLEAR SPIN MEASUREMENTS IN SOME NUCLIDES OF THE ALKALI ELEMENTS RUBIDIUM AND FRANCIUM C. Ekström, S. Ingelman, G. Wannberg and M. Skarestad UUIP-954 March 1977 ISSN 0042-0263 NUCLEAR SPIN MEASUREMENTS IN SOME NUCLIDES OF THE ALKALI ELEMENTS RUBIDIUM AND FRANCIUM C. Ekström ) Department of Physics, Chalmers University of Technology and University of Gothenburg, Gothenburg, Sweden. S. Ingelman and G. Wannberg Institute of Physics, University of Uppsala, Uppsala, Sweden. M. Skarestad +) E. P. Division, CERN, Geneva, Switzerland. and The ISOLDE Collaboration, CERN, Geneva, Switzerland. ABSTRACT The nuclear spins of several nuclides of the alkali elements rubidium and francium have been measured using atomic-beam magnetic resonance techniques. The following results have been 77 7 7>m 7 5 obtained: Rb I » V2» 'tt> I •= 0, Rb 1 = 4, »Rb I = /2' 208 209 210 211 "•mRb 1=6, Fr 1=7, Fr I = «/2, Fr 1=6, Fr 220 221 5 I = 9/2, 2i2Fr 1 = 5, 2i3Fr I = »/a» Fr 1 = 1, Fr I = /2, 222Fr 1=2. The spin valuss are discussed briefly in terms of current nuclear models. *) Present address s E. P. Division, CERN, CH-1211 Geneva 23, Switzerland. +) Present address ; Department of Chemistry, University of Oslo, N-1000 Oslo 3, Norway. - 1 - 1. INTRODUCTION Nuclides of the alkali elements rubidium, cesium and francium are obtained in high yields at the ISOLDE facility as spallaticn products from 600 NeV proton reactions in different targets, followed by on-line suface ionization and isotope separation [1]. In a previous paper [2J, we reported on an on-line oven foil system which efficiently converts an ion-beam of alkalis frorr. the separator to an atomic-beam, and on the measurements of nuclear spins and moments of several cesium isotopes using ABMR techniques. The same methods have been used in the present work to measure nuclear spins in some rubidium and francium nuclides. The element francium is here for the first time subject to ABMR measurements. 2. EXPERIMENTAL PROCEDURE AND RESULTS Referring to our work on cesium [2], we limit our presentation of the experimental techniques to details specific to the present work on rubidium and francium. For the production of rubidium, targets of yttrium or niobium were used. The production yields of different rubidium isotopes at the collector chamber of the isotope separator are shown in Fig. 1. In the same figure are given the corresponding data on francium yields from a target of graphite cloth impregnated with uranium. The main part of the experiments were performed on-line, i.e. guiding the ion-beam from the isotope separator directly to a heated tantalum foil covered with a layer of yttrium. From that surface the activity evaporated continuously in the form of free atoms. Off-line techniques were used in part of the experiments on the more long-lived isotopes. Appropriate types of detectors were used to measure the activity passing through the atomic-beam apparatus; thin plastic scin- tillators for the detection of &*, surface barrier detectors - 2 - for a and Ge(Li) detectors for certain Y-lines. The simple electronic structure of the alkali elements makes them particularly suited for atomic-beam measurements [2] . The electronic splitting factor for the ground state of rubidium has been measured by Bok len et al. [3] to be gy» 2.0023319(14) . The g -factor for francium has not been determined. Spin mea- u surements performed in weak external magnetic fields are, however» not sensitive to small variations in the g -value. j According to the formula relating the nuclear spin to the resonance frequency [2j : v 9 " J T 21 + 1 we obtain at the strongest field used in the francium measure- ments, vBB/h * 6.185 MHz, a difference of 6 kHz in resonance frequency assuming g = 2.0023 or 2.0033. This difference is smaller than the line width of the resonance signals which is about 30 kHz. In the experiments on francium we have assumed an electronic splitting factor g = 2.0028. Spin searches in the rubidium and francium nuclides were made according to the equation above. The final results, shown in Table 1, were established by the observation of resonance signals in at least two different external magnetic fields, for rubidium u_B/h = 1.079, 1.370, 2.964 and 4.029 MHz and for francium 4.482 and 6.185 MHz, and by the absence of resonance signals at the frequencies corresponding to other spin values. 1 Spin values in the range /2 - 'V: were checked in the odd-A isotopes and 0 - 7 in the doubly-odd ones. In Figs. 2 - 4, we exhibit decay curves of some resonance signals obtained in rubidium and francium. Of particular interest are those shown in Fig. 3. In an off-line experiment, a sample of 7*Rb was evaporated from the atomic-beam oven. By applying the frequencies corresponding to the spin values I « 0 and I * 4 in exposing two collectors alternatively, it was possible to make an isomer - 3 - separation. The two decay curves correspond to the 17 min ground state and the 6 min isomeric state, respectively. particular attention was paid to the ground state of 7*Rb, in which resonance signals were observed at the 1=0 frequencies. Such signals may also be obtained in the case of a non-zero spin and an extremely small hyperfine structure separation Av. A nucleus with 1=1 would give three resonance signals separated by 2/j«Av. in order to check the possibility of a non-zero spin we made a careful frequency scan in a field of u^B/h = 1.370 MHz, from 700 kHz below to 200 kHz above the spin 1=0 frequency. Only one resonance signal was observed, having a line width of 40 kHz. Assuming this line to be composed of three unresolved lines h?ving widths of 30 kHz t the width of the potassium calibration line at this field, we get a hyperfine structure separation of 8 kHz. This is an upper limit in the case of a non-zero spin, since spin values larger than 1=1 would imply a larger number of resonances and thus a smaller hyperfine structure separation. The corresponding upper limit of the nuclear magnetic moment may be calculated to be 3*10~6n.m. We have not taken into account any broadening of the observed resonance line due to field inhomo- geneities, which would be three times larger in the case 1=0 than for 1=1, thus making the assumption of a non-zero spin in 7eRb even more improbable. 3. DISCUSSION 3.1 The rubidium isotopes The neutron-deficient rubidium isotopes belong to a region where both the protons and the neutrons range between the magic numbers 28 and 50. Nolte et al. [4] have made a systematic study of the first excited 2+ states in doubly-even nuclei belonging to this region. The shell closures at the magic numbers are clearly identified through the high excitation energies. In addition to these shell closures, closed subshells are observed at neutron number N = 38 in nuclei close to Z • 28, and at proton number - 4 - Z » 40 in nuclei close to N = 50. The effect of the subshell closures is» however» completely lost far front Z = 28 and N = 50 respectively» and maximum deformation is obtained at the centre of the region enclosed by 28 = ( N,Z ) =50. The lightest rubidium 7 isotopes investigated in this work, "''••'•m» »m)# are located close to the centre of this region. Here, rotational bands based 1 on the orbitals [301 /i], [301 V2] and [303 V2]» and perturbed rotational bands associated with the low-spin Nilsson orbitals originating from the g9 . shell model state have been identified in several nuclides, both odd-proton and odd-neutron ones. The different orbitals may be found in the energy level diagram for odd protons shown in Fig. 5. These levels have been calculated within the Nilsson model employing the shell parameters tc = 0.071 and |i - 0.300. The levels occupied by the 37th proton of rubidium at a deformation of about e = 0.2 are drawn in heavy lines. It is 5 79 seen that the measured nuclear spin I = /2 in Rb may be inter- 5 3 77 s preted as [303 V2] or /2[440 V2] and I = /2in Rb as [301 /2] A preliminary result from a magnetic moment measurement in 7sRb V= 3.37(6) n.m.indicates that the ground state should be classi- 5 5 fied by the orbital /2[440 V2] rather than [303 /2] • The theoretical moments of these states are 3 n.m. and 1 n.m., respectively. The nuclear spins of the ground and isomeric states of 78Rb, 1=0 and 1=4, may be obtained by coupling the neutron 5 77 5 orbital /2[.44O Vz] of Kr to the proton orbitals /2[440 V2] and [301 V2] . Further experimental data, particularly on the level structure in 77Rb and 79Rb would be of great interest. A rotational structure would support the assignments proposed here. The isotope 81>Rb is located relatively close to the N * 50 shell closure. The measured isomeric state spin 1-6 may accordingly be given the shell model assignment 6~( wg, , vd, , ) . It '2 3.2 The francium isotopes The light francium isotopes studied in this work, 20lFr - 2l3Fr, appear in the corner Z > 82, N < 126, close to the shell closures. The shell model proton state h» , here accounts for several ground states in the Z * 83 bismuth and Z * 85 astatine isotopes.