Binder, R.

Bruchertseifer, H.

Buklanov, G.

Domanov, V. P.

Dressler, R.

Fischer, S.

Guseva, L. I.

Gäggeler, H. W.

Kubica, B.

Lien, Dinh Thi

Schumann, D.

Szeglowski, Z.

Taut, St

Tikhomirova, G. S.

Yakushev, A. B.

RERO DOC Digital Library

Radiochimica Acta 77, 241-244 (1997) © R. Oldenbourg Verlag, München 1997 Rapid Communication First Observation of y-Ray Emission Assigned to the Decay of 164W By R. Dressler1, D. Schumann2, St. Taut3, S. Fischer4, R. Binder5, A. B. Yakushev6, G. Buklanov6, Dinh Thi Lien6, V. P. Domanov6, Z. Szeglowski7, B. Kubica7, L. I. Guseva8, G. S. Tikhomirova8, H. W. Gäggeler '·9 and H. Bruchertseifer1 1 Paul-Scherrer-Institute, CH-5232 Villigen, Switzerland 2 University of Technology Dresden, D-01314 Dresden, Germany 3 Research Centre Rossendorf, D-01314 Dresden, Germany 4 Charité of Humboldt-University Berlin, D-10117 Berlin, Germany 5 University Leipzig, D-04109 Leipzig, Germany 6 Joint Institute of Nuclear Research, 141980 Dubna, Russia 7 H. Niewodniczanski Institute of Nuclear Physics, PL-31-342 Krakow, Poland 8 Vernadsky Institute of Geochemistry and Analytical Chemistry, 117975 Moscow, Russia 9 University Bern, CH-3012 Bern, Switzerland (Received June 26, 1997; accepted in revised form August 13, 1997) Tungsten isotopes / Excitation functions / Nuclear reaction / γ-Rays from ,MW Summary The excitation functions of the short-lived tungsten isotopes 164W and l65W produced in the nuclear reaction 24Mg + ,44Sm were measured for = 109 MeV—141 MeV. Two y-lines at (187.0 ± 0.1) keV and (268.7 ± 0.2) keV were discovered in the y-spectra of the tungsten fraction after chemi-cal separation at a beam energy of 128 MeV which we assign to ,64W. The half-life of the 187.0 keV y-]¡ne is (7.0 ± 0.2) s. 1. Introduction Short-lived tungsten isotopes are interesting as homo-logues of the transactinide element 106. If these tung-sten isotopes have y-transitions, then a very convenient on-line monitoring of the chemical separation is pos-sible if mixed rare earth and actinide targets are used for the simultaneous production of W and element 106. The half-lives of the model nuclides should be of the same order of magnitude as those of the heavy element. Presently three isotopes of element 106 with half-lives in the range of seconds are known: 263106 (Tm = 0.9 s) [1], 265106 (Ttn = 2 s—30 s) and 266106 (Tu2 = 1 0 s - 3 0 s ) [2], the latter two being more suitable for chemical experiments. From this it follows that the tungsten isotopes 164W (Ti/2 = 6.4 s ± 0.8 s) and 165W (Tu2 = 5.1 s ±0.5 s) [4, 5] are best suited as model nuclei. Unfortunately, only few data on these two exotic nuclei are available from the literature. Eastham et al. [3] measured the excitation functions for production of 162/165/,64W in the reactions 144/,47Sm (24Mg, xn) via α-detection. 165/166W were first produced by Toth et al. [4] in the reaction ,56Dy (160, xn). Additional data on 1 6 ° - , 6 6 w reported in [5, 6] were confirmed by these authors. For 164W α-branches of 2.6% [5] or 5% [6] and for ,65W < 1.5% [5] are report-ed; the other decay mode is electron capture or ß+-decay. Therefore, y-lines of these nuclides can be expected but are so far unknown. 2. Experimental The reactions 24Mg + ,44/,47,,49Sm (85% ,44Sm, 15% ,47/,49Sm) were used to produce short-lived tungsten isotopes. The experiments were performed at the U-400 cyclotron of the Flerov-Laboratory of Nuclear Reactions at JINR in Dubna, Russia. A target of 1.0mg/cm2 thickness on a 20 μπι Be-backing was bombarded by typically 1012 particles per second of 24Mg12+ ions with a beam energy of 187 MeV. First the beam passed a vacuum window consisting of a 16 μπι Al-foil. The cross-sections of 164/165W were determined at the energies 109 MeV, 115 MeV, 126 MeV, 129 MeV and 141 MeV. The beam energy was adjusted by using thin Al-degrader foils of follow-ing thicknesses: 15.0 pm, 12.2 pm, 7.5 pm, 4.7 pm, and without, respectively. The uncertainty in energy was estimated to be ± 1 MeV. The reaction products recoiling out of the target were transported from a thermalisation chamber to the chemical set-up using the NaCl/Ar gas-jet system described in [7]. First, the gas-jet passed a degasser system which was slightly modified with respect to the device described in [8] : in order to decrease the transport time from the target chamber to the detector position two instead of four filters inside the degasser were used. This decreased the chemical yield to 25%, but lowered the transport time from the production site to the detector to 20 s. For a determination of the excitation functions the produced isotopes of W, Ta, and Hf first passed a DOWEX 50X8 column which retained most of the other reaction products and were then collected on a 242 R. Dressler et al. DOWEX 1 Χ 8 column using a 0.2 M HF solution [9], For 20 min on-line "/-detection of the anion exchange column was performed with a HPGeX detector (ORTEC) ; The activities of the decay products of the short-lived W isotopes, i.e. the grand-daughters 164Hf (j-line at 153.3 keV), and ,65Hf (/-line at 179.9 keV), were used for a determination of the relative cross-sections. For later half-life measurements chemical separa-tions of tungsten were performed by adsorbing lantha-nides, Ta and Hf on a DOWEX 50X8 (200-400 mesh) column saturated with La(OH)3 and using a 0.1 M NaOH solution as eluent. Under these con-ditions the tungsten fraction passed the cation ex-change column and could be adsorbed on a following DOWEX 1 X 8 (200-400 mesh) column. Details of the chemical set-up and the column preparation are given in [8]. With this setup it was possible to detect isotopes with half-lives down to about 5 s. The tungsten fraction was collected on the DOWEX 1 column for each chemical separation during 45 s. Then the system was switched off and the '/-spectra were measured with a HPGeX detector positioned at the anion exchange column in 16 cycles of 1.8 s each. Between the consecutive measurements the computer system needed 0.6 s for saving the spectrum and starting the following measurement. The experiments were repeated 49 times and the corre-sponding spectra were summed. The anion exchange column was replaced after every experiment, whereas the cation exchange column was used for three con-secutive separations and then replaced. 3. Results and discussion 3.1 E x c i t a t i o n f u n c t i o n s The cross-sections of 164W and 165W were determined via their decay products 164Hf and 165Hf, respectively, at beam energies between 109 MeV and 141 MeV. In this region of excitation energies (E* = 40—70 MeV), based on HIVAP calculations, direct production of l64Hf via the aOn-reaction and of 165Hf via the 2pln-reaction are negligible. In addition, for the aOn-chan-nel the maximum of the excitation function is expected at about 20 MeV lower energy than the maximum of the 4n-channel which leads to 164W. The production of "l4Ta via the p3n-reaction and of 165Ta via the p2n-reactions cannot be ruled out a priori. However, these reactions would only affect the absolute values of the cross-sections and not alter the position of the maximum of the excitation functions or their shapes. Eastham et al. pointed out [3] that the pxn-channels peak at nearly the same energies as the (x + l)n-channels. For the calculations of the cross-sections growth and decay corrections were applied for the activity of the permanently collected reaction products on the anion exchange column. Only relative values for the cross section are given since the absolute intensity of « c =5 2? D 10-1 -10-2 80 100 110 120 130 140 150 160 E [MeV] lab Fig. 1. Excitation functions of , MW (Δ) and ,65W (V) from the reaction 24Mg + ,44Sm; the solid line is a fit through experimental data for 164W from [3]; the dashed lines are to guide the eye. energy [keV] Fig. 2. /-spectrum of a capillary-helix measurement at a beam energy of 128 MeV. the 153.3 keV /-line of ,64Hf and of the 179.9 keV /-line of 165Hf are unknown as well as several yields (gas-jet transportation, chemical separation) can only be approximated. Fig. 1, shows the results in relative cross-sections together with a fit through the experimental data from Eastham et al. [3] from the same nuclear reaction. Both experimental data sets for 164W are in a reason-able agreement. 3 .2 Search f o r new / - l i n e s To detect possible new /-lines of short-lived W isotopes a capillary-helix of 20 m length and 2 mm i.d. was positioned over the HPGeX detector to measure on-line and in flight the /-spectrum of the reaction products transported with the NaCl aerosol particles. First Observation of y-Ray Emission Assigned to the Decay of 164W 243 160 180 200 220 e n e r g y [ k e V ] Fig. 3. Accumulated y-spectrum of the separated tungsten frac-tion at a beam energy of 128 MeV. 1 ι » ι 1 ι ' ι ' r ' l ' I 1 ' 1 ' 1 ' 1 ' 1 — * I • 1 2 5 . 8 k e V Τ = ( 2 1 . 5 ± 0 . 6 ) s 1/2 _ " 1 - . . . . . . . 1 8 7 . 0 k e V Τ = ( 7 . 0 ± 0 . 2 ) s : 1/2 ι I ι I ι 1 . 1 1 1 2 6 8 . 7 k e V ι 1 . 1 . 1 . 1 . 1 . 1 . I , I 0 2 4 6 8 10 12 14 16 18 20 22 24 26 28 30 32 t i m e [ s ] Fig. 4. Time analysis of the 125.8 keV y-radiation from 166W, and the y-radiation at 187.0 keV and 268.7 keV assigned to ,64W. Fig. 2 shows an accumulated y-spectrum during 15 min at a beam energy of 128 MeV, which corre-sponds to the optimum energy for production of 164Hf (Fig. 1). Two unknown y-lines with energies of (187.0 ± 0 . 1 ) keV and (268.7 ± 0 . 2 ) keV were ob-served. The ratio of the activities of these two y-lines is 5.7 ± 1.9. Since these y-radiations might belong to short-lived tungsten isotopes we decided to perform a chemical separation prior to a decay study. 3 . 3 D e t e r m i n a t i o n o f t h e h a l f - l i f e With the chemical separation procedure described above decay measurements of the reaction products were carried out at 128 MeV. Fig. 3 shows the accumulated y-spectrum from all chemical separations summed up for the first 8 cycles (0 s—19.2 s) which again shows the two y-lines at 187.0 keV and 268.7 keV. Since I64W has a reported half-life of 6.4 s, an optimum binning for the time distribution of counts [13] was made by adding two consecutive spectra to generate a counting time interval of 4.8 s. First we analysed the activity of the 125.8 keV y-line from , 6 6W to check the counting system as well as the calculation algorithm. This yielded a half-life of (21.5 ± 0.6) s (see Fig. 4), which is in excellent agree-ment with (22 ± 1) s from previous work [12]. Also shown in Fig. 4 is the decay of the activity producing the two new y-lines. The time analysis of the 187 .0keV y-radiation yields a half-life of (7.0 ± 0.2) s. This value is in good agreement with the reported half-life of , 6 4W of (6.4 ± 0.8) s [5]. The intensity-ratio from this measurement for the 187.0 keV to the 268.7 keV y-line is 4.2 ± 1 . 5 , in agreement with the value from the on-line measure-ment. In a previous study using the same projectile-target combination but a lower beam energy of 112 MeV these two y-lines were not observed [8], On the basis of the measured half-life and the knowledge of the shape of the excitation functions for , M W and 1 6 ,W (Fig. 1), we conclude that the y-lines at 187.0 keV and 268.7 keV are associated with the decay of 164W and not with the decay of ,65W. References 1. Ghiorso, Α., Nitschke, J. M., Alonso, J. R., Alonso, C. T., Nurmia, M., Seaborg, G. T., Hulet, E. K„ Lougheed, R. W.: Phys. Rev. Lett. 33, 1490 (1974). 2. Lazarev, Yu. Α., Lobanov, Yu. V., Oganessian, Yu. Ts., Utyonkov, V. K., Abdullin, F. Sh., Buklanov, G. V., Gikal, Β. N., Iliev, S., Mezentsev, A. N., Polyakov, A. N., Sedykh, I. M., Shirokovsky, I. V., Subbotin, V. G., Sukhov, A. M „ Tsyganov, Yu. S., Zhuchko, V. E., Lougheed, R. W., Moody, K. J., Wild, J. F., Hulet, E. K„ McQuaid, J. H.: Phys. Rev. Lett. 73, 624 (1994). 3. Eastham, D. Α., Grant, I. S.: Nucl. Phys. A208, 119 (1973). 4. Toth, K. S., Schmidt-Ott, W.-D., Bingham, C. R., Ijaz, M. Α.: Phys. Rev. C: 12, 533 (1975). 5. Hofmann, S., Faust, W., Münzenberg, G., Reisdorf, W., Armbruster, P., Güttner, K., Ewald, Η.: Ζ. Phys. Α291 53 (1979). 6. Page, R. D., Woods, P. J., Cunningham, R. Α., Davinson, T., Davis, N. J., James, A. N., Livingston, K., Sellin, P. J., Shotter, A. C. : Phys. Rev. C53, 660 (1996). 7. Schumann, D., Dressler, R., Fischer, S., Taut, St., Binder, R., Szeglowski, Z., Kubica, B., Guseva, L. I., Tikhomirova, G. S., Constantinescu, O., Domanov, V. P., Constantinescu, M., Dinh Thi Lien, Oganessian, Yu. Ts., Brudanin, V. B., Bruchertseifen H.: Radiochim. Acta 35, 69 (1995). 8. Schumann, D., Dressler, R., Taut, St., Nitsche, H., Szeglowski, Z., Kubica, B., Guseva, L. I., Tikhomirova, G. S., Yakushev, Α., Constantinescu, O., Domanov, V. P., Constantinescu, M., Dinh Thi Lien, Oganessian, Yu. Ts., Brudanin, V. B., Zvara, I., Bruchertseifen H.: J. Radioanal. Nucl. Chem., Letters 214, 1 (1996). 9. Szeglowski, Z., Bruchertseifen H., Brudanin, V. B., Buklanov, G. V., Constantinescu, O., Dinh Thi Lien, Domanov, V. P., Guseva, L. I., Hussonnois, M., Tikhomiro-va, G. S., Zvara, I., Oganessian, Yu. Ts.: J. Radioanal. Nucl. Chem., Letters 186, 353 (1994). 10. Hild, T., Schmidt-Ott, W.-D., Freystein, V., Meissner, F., Runte, E., Salewski, H., Michaelsen, R.: Nucl. Phys. A492, 237 (1989). 244 R. Dressler et al. 11. Reisdorf, W„ Schädel, M.: Z. Phys. A343, 4 (1992). 12. Dressler, R.: Diploma thesis, Univ. Leipzig, 1992 (in german), unpublished; and Heller, W., Binder, R., Bruchertseifen H., Becker, U., Haberberger, F., Herrmann, G., Kratz, J. V., Mendel, M., Nähler, Α., Pense-Maskow, M., Trautmann, N., Wiehl, N., Brüchle, W., Jäger, E., Schädel, M., Schausten, B., Alstad, J., Skarnemark, G., Dressler, R., Fischer, S., Roß, Α., Eichler, B., Hiibener, S.: Institut für Kernchemie, Universität Mainz, Jahresbericht 1991, p. 28 (1992), unpublished. 13. Zlokasov, V. B.: Nucl. Instr. Meth. Phys. Res. A275, 392 (1989). 14. Bruchertseifer, H., Langrock, E., Muzychka, Yu. Α., Oganesian, Tu. Ts., Pavlat, T., Penionzhevich, Yu. E., Pustyl'nik, Β. I., Schilling, K. D.: JINR Ρ 7-80-666, unpub-lished. 

Rapid Communication: First Observation of y-Ray Emission Assigned to the Decay of 164W

Rapid Communication: First Observation of y-Ray Emission Assigned to the Decay of 164W

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