CORRELATION STUDIES OF THE 5H SPECTRUM M.S. Golovkov1, L.V. Grigorenko1, A.S. Fomichev1, S.A. Krupko1, Yu.Ts. Oganessian1, A.M. Rodin1, S.I. Sidorchuk1, R.S. Slepnev1, S.V. Stepantsov1, G.M. Ter-Akopian1, R. Wolski1,2, A.A. Korsheninnikov3, E.Yu. Nikolskii3, P. Roussel-Chomaz 4, W. Mittig4, R. Palit5, C. Angulo6, V. Bouchat7, V. Kinnard7, T. Materna7, F. Hanappe7, O. Dorvaux8, L. Stuttge 8, A.A. Yukhimchuk9, V.V. Perevozchikov9, S.K. Grishechkin9, Yu.I. Vinogradov9, S.V. Zlatoustovskiy9. 1 Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Russia The Henryk Niewodniczanski Institute of Nuclear Physics, Krakow, Poland 3 RIKEN, Hirosawa, Japan; On leave from the Kurchatov Institute, Moscow, Russia 4 GANIL, Caen Cedex5, France 5 GSI, Darmstadt, Germany 6 Centre de Recherche du Cyclotron, UCL, Louvain-La-Neuve, Belgium 7 Universite Libre de Bruxelles, PNTPM, Bruxelles, Belgium 8 Institut de Recherches Subatomiques, IN2P3/Universite Louis Pasteur, Strasbourg, France 9 RNFC – All-Russian Research Institute of Experimenntal Physics, Sarov, Nizhni Novgorod region, 67190 Russia 2 Very asymmetric nuclear matter is a phenomenon in subatomic physics remaining far from a good understanding. The study of the superheavy hydrogen isotope 5H could shed light on this subject. Controversy in results obtained to date on the 5H system [1-5] gave rise to an intense discussion that has appeared even in the popular literature. Essentially, the question was whether the 5H ground state (g.s.) is located at 1.7-1.8MeV above the t+2n decay threshold [2,3], or at about 3 MeV [4] or even higher [1,5]. Theory calculations are sensitive to model assumptions and also give diverse predictions on 5 H. New experiments could resolve this important question. In the present work we studied the same reaction 3H(t,p)5H as in Ref.[4] but in a different kinematical region. The experimental setup is shown in Fig.1. A 58 MeV triton beam was produced at the Dubna U-400M cyclotron. The ACCULINNA separator was used to reduce the angular spread and energy dispersion of the primary triton beam to 7 mrad and 0.3 MeV (FWHM), respectively. Finally, the triton beam with intensity of 3*107 particles/s was focused in a 5 mm spot on a cryogenic tritium target [6]. The 4 mm thick target cell was filled with tritium to a pressure of 860 mbar and cooled down to 25°K. Slow protons emitted to the back from the target hit a 300 µ thick Si detector with double-sided strips. This annular detector, having an active area with inner and outer diameters of 32 and 85 mm, respectively, was installed 100 mm upstream of the target. Charged particles moving in the forward direction were detected by a telescope consisting of four annular Si detectors of the same radial dimensions as the one used to detect protons. Neutrons were detected by 48 scintillation modules of the time-of-flight spectrometer DEMON. Being installed at a distance of 2.5 m from the target the modules covered an angular range of θlab = 5° – 40°. The forward array detected the 5H→t+2n decay products emitted almost at any angle. Fig. 1. Experimental set up. Analysis was made for the detected triple ptn coincidence events. Such events uniquely identify the p+5H outgoing channel and make complete kinematical reconstruction possible. Results are shown in the CM system of the decay products of 5H (t+2n). The direction of the momentum transfer, kbeam - kp, occurring in the reaction 3H(t,p)5H was chosen as Z axis (see Fig. 1). The most striking result was the observation of a sharp oscillating picture in the triton angular distribution shown in Fig.2 by points. The analysis showed that the bulk of the data observed in the present experiment can be explained on the assumption that the direct twoneutron transfer dominates in the 3H(t,p)5H reaction leading to the population of the broad, overlapping 3/2+ and 5/2+ states in 5H. This is supported by the following arguments: One could consider the 5H system as a “proton hole” in 6He. So, definite similarity between these systems can be expected. Theoretical predictions give Jπ=1/2+ for the ground state of 5H. Its low-lying excited states are supposed to be a 3/2+ and 5/2+ doublet. One should expect a weak population of the 5H g.s. in the 3H(t,p)5H reaction. This is due to the statistical factor and also is a consequence of the “angular momentum mismatch” arising from the fact that the light proton can not carry away as much angular momentum as the heavier triton projectile brings in. DWBA calculations confirm this expectation. with the doublet of the excited 3/2+ and 5/2+ states of 5H and excited doublet. Fig. 3. The missing mass spectrum of 5H. Bottom panel: data are shown by points, histogram is the result of model calculations. Top panel: shown are the efficiency corrected results of the fit. The dashed and dotted curves show the contributions of the 1/2 + g.s. and 3/2+, 5/2+ doublet, respectively. Fig. 2 Distribution over the triton angle observed in the CM system of 5H for different ranges of the E5H energy. Points show the experimental data, histograms present the results of model calculations. We employed the following procedure for data analysis. Correlations occurring at the 5H decay are described as W(E)= † J'M' ρ A J'M' A J'M' JMJ'M' where AJM are the decay amplitudes depending on the 5H decay dynamics and ρ is the density matrix describing the polarization of the 5H states populated in the 3H(t,p)5H reaction. We expanded the amplitudes AJM over a limited set of hyperspherical harmonics. A similar approach was employed in Ref. [7]. Histograms in Figs. 2 and 3 show the results of calculations which take into account the detection efficiency. The missing mass spectrum of 5H (presented in Fig. 3) shows a broad structure above 2.5 MeV. The strong correlation patterns seen in Fig. 2c,d allowed us to unambiguously identify this structure as a mixture of the 3/2+ and 5/2+ states. Such a correlation is a rare phenomenon for transfer reactions involving nuclei with nonzero spin and means that the 3/2+ and 5/2+ states are either almost degenerate or the reaction mechanism causes a specific interference of these states. It should be noted that at E5H<2.5 MeV (see Fig. 2a,b) excellent agreement with experimental points could be achieved only at a condition that the calculations assumed the population of the 1/2+ 5H g.s. and its interference The data analysis lead the authors to a conclusion that the g.s. resonance of 5H is located close to 1.8 MeV and has a width of about 1.3 MeV. The observed g.s. resonance position is in a good agreement with the experimental observations of Refs. [2,3]. Furthermore, the present data show that the doublet of the wide excited 3/2+–5/2+ states populated in the 3H(t,p)5H reaction achieves its maximum at E5H5 MeV. The correlation picture observed in the present work at E5H<2.5 MeV shows the interference of the 3/2+–5/2+ doublet with the 1/2+ g.s. This is consistent with the alternative explanation presented in Ref. [3] for the small width of the 1.8 MeV g.s. peak of 5H reported in this paper. References 1. D.V. Aleksandrov et al., Proc. Int. Conf. on Exotic Nuclei and Atomic Masses, Arles, France, (1995) p. 329. 2 A.A. Korsheninnikov et al., Phys. Rev. Lett., 87 (2001) 092501. 3. M.S. Golovkov et al., Phys. Lett. B, 566 (2003) 70. 4. M. Meister et al. Nucl. Phys. A, 723 (2003) 13; Phys.Rev. Lett., 91 (2003) 162504. 5. M.G. Gornov et al., Pis'ma ZhETF, 77 (2003) 412. 6. A.A. Yukhimchuk et al., Nucl. Instrum. Meth. A, 513 (2003) 439. 7. O.V. Bochkarev et al., Sov. J. Nucl. Phys. 55, (1992) 995
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