Can the Neutron-Neutron Scattering Length be Determined from n-d Breakup Experiments? W. von Witsch Institut für Strahlen- und Kernphysik, Universität Bonn, D-53115 Bonn, Germany Abstract. Two recent nd breakup experiments are discussed which were aimed at the determination of ann, the neutron-neutron scattering length. In both cases, the data were analyzed by means of state-of-the-art Monte-Carlo simulations based on rigorous three-nucleon calculations with realistic nucleon-nucleon potentials. Yet, the two results differ greatly, whereat one of them agrees with the value obtained via the 2H(π¯,nn)γ reaction, while the second one reproduces the average result of all previous nd breakup experiments. Moreover, some other recent findings regarding the nd breakup process raise the old question anew whether the nn scattering length can be extracted at all from this reaction using present-day theories. INTRODUCTION EXPERIMENTAL DETAILS The 1S0 nucleon-nucleon (NN) scattering length aNN is a powerful magnifying glass to study the NN interaction. Because the 1S0 state is almost bound, the scattering length has a large negative value, and small changes in the depth and width of a two-nucleon potential cause large changes in aNN. The neutronneutron and proton-proton scattering lengths ann and app are of special interest because, in principle, they allow a sensitive test of charge symmetry in the strong interaction. While app can be measured very accurately via pp scattering, in the case of ann the measurement is difficult because one must resort to multi-particle breakup reactions with two neutrons in the exit channel. Numerous attempts have been made to determine ann, using mostly the 2H(π¯,nn)γ and 2H(n,nn)p reactions and investigating the region of the nn final-state interaction (FSI), where the two neutrons travel together with small relative energy. While today the 2 H(π¯,nn)γ reaction seems to provide for ann a consistent average value of –18.6±0.4 fm [1,2,3], the situation regarding the nd reaction is confusing. Specifically, two very thorough investigations based on this reaction have recently been reported [4,5], with mutually exclusive results. In both cases, the data were analyzed by means of state-of-the-art Monte-Carlo simulations based on rigorous Faddeev-type calculations with realistic nucleon-nucleon potentials [6]. In this talk, I will compare the two experiments, emphasizing their respective strong and weak points, and finally address the question of whether, perhaps, with present-day theories the nn scattering length cannot be obtained from this reaction after all. The TUNL Experiment The first experiment [4] was performed at the Triangle Universities Nuclear Laboratory (TUNL) at Durham, N.C. A collimated neutron beam of 13 MeV was produced with the 2H(d,n)3He reaction by bombarding an 8-bar gas target with a 10-MeV, 2-µA deuteron beam from the tandem accelerator. The reaction target consisted of a glass cylinder, 6 cm high and 4 cm in diameter, filled with C6D12 liquid scintillator in which pulses from breakup protons as well as recoil deuterons were observed. The nn interaction was investigated in the traditional "final-state geometry", i.e. the two neutrons were detected in coincidence with two liquid-scintillator n detectors placed behind each other at the same angle on the same side of the beam. The front detector was ringshaped, and the coaxial back detector was positioned such as to fill the solid angle of the opening in the ring detector. Absolute cross sections were measured at four angles between 20.5o and 43.0o simultaneously. The integrated beam-target luminosity was obtained by recording the yield for nd elastic scattering along with the breakup data. The efficiency of the n detectors was determined by putting them in neutron fields of known intensities at TUNL and at the Physikalisch-Technische Bundesanstalt (PTB) in Braunschweig, Germany. The value of ann, deduced from the absolute cross sections, was –18.7±0.60 fm. In a parallel experiment, the well-known 1S0 np scattering length, which is –23.75±0.01 fm [7], was measured concurrently by placing several additional n detec- CP680, Application of Accelerators in Research and Industry: 17th Int'l. Conference, edited by J. L. Duggan and I. L. Morgan © 2003 American Institute of Physics 0-7354-0149-7/03/$20.00 268 timing for the determination of the neutron energies. However, it entailed strong multiple scattering effects which had to be simulated accurately. The recoil geometry chosen for the Bonn experiment avoided this, and the passive target permitted a much higher beam intensity which, together with the 100% efficiency of the proton detector and a larger cross section, nearly compensated for the smaller target thickness. Elastic deuterons could easily be distinguished from breakup protons by means of their energy and TOF. In addition, there was no problem of cross talk between closely spaced n detectors. Perhaps the biggest advantage of this geometry, however, was the simultaneous appearance in the spectrum of quasifree np scattering (QFS), where the cross section is independent of ann and thus provides a built-in normalization for the FSI peak. In this way, all problems regarding the absolute calibration of the n beam and of the n detector efficiency were essentially eliminated – assuming that the theory describes the np QFS cross section correctly. (A certain complication arose from the fact that the neutron detector was positioned on the recoil axis of the 2n system with low relative energy, so that both neutrons might hit the detector, thereby increasing its effective efficiency. However, even though this was a sizeable effect, it is governed simply by three-body kinematics and thus could be taken into account very accurately in the MC simulations.) tors on the opposite side of the beam, resulting in anp = –23.5±0.8 fm, in agreement with Ref. [7]. The Bonn Experiment The second experiment [5] was done at energies of 25.3 and 16.6 MeV at the cyclotron of the Institut für Strahlen- und Kernphysik at Bonn University. In this case, high-energy (HE) neutrons produced via the ²H(d,n)³He reaction were used together with lower-energy (LE) ones from the upper part of the breakup continuum from the ²H(d,n)pd reaction. The gas target was liquidnitrogen cooled at a pressure of 39 bar, resulting in a HE beam width of 4.0 MeV. In contrast to the TUNL measurement, a different geometry was used in Bonn, where only one of the neutrons was detected together with the recoiling proton on the other side of the beam ("recoil geometry"). In an evacuated "proton arm", a 50-mg/cm2thick CD2 target was suspended in the intensity plateau of the tightly collimated n beam. The breakup protons first had to pass through a thin scintillation foil detector (SFD), positioned near the target but outside of the n beam, before being stopped in a 5-mm-thick scintillator. The signals produced in the SFD served as start signals for all TOF measurements, including the TOF of the incoming n beam. For the absolute normalization of the neutron fluence, a double proton recoil telescope (PRT) was placed in the beam, detecting protons emitted from a CH2 target at angles of ±35o. The efficiency of the n detector was determined in situ by means of np scattering, using the same setup with the CD2 target replaced by a CH2 foil. At 25.3 MeV, a value of ann = –16.3±0.4 fm was deduced from the absolute cross section while the relative cross sections at 25.3 and 16.6 MeV, normalized in the region of quasi-free np scattering (see below), yielded –16.1±0.4 fm and –16.2±0.3 fm, respectively. Also at Bonn the np scattering length was measured as a test for the experimental procedure. In a first measurement, done at 25.3 MeV in recoil geometry, the proton arm was replaced by a second n detector, and a 4.4-cm-diameter scintillator target was used, leaving the rest of the setup unchanged. Subsequently, a measurement in FSI geometry was made in which a Si surface barrier detector was placed in front of an n detector at 32O [8]. The results of the two experiments were anp = –23.9±1.0 and –24.3±1.1 fm, respectively, which is also in agreement with the value known from free np scattering. Discussion Differing by almost four standard deviations, the ann results of the two experiments are obviously conflicting, while being internally consistent. The four angles measured at TUNL gave results which agree among themselves and also with the average value from the 2 H(π¯,nn)γ reaction. Similarly, all three results of the Bonn experiment agree with each other, whereat two of them, at 25.3 and 16.6 MeV, were deduced from the relative cross sections, and one, at 25.3 MeV, from the absolute count rate. The Bonn results are also in agreement with those of all previous kinematically complete, n-induced breakup experiments [9]. Thus, while the TUNL results seem to indicate that there is no angular dependency, those from Bonn show independence with respect to the bombarding energy. Of course, the different geometries of the two experiments should not matter because, at relative energies Enn ≈ 0, the breakup amplitude does not depend on which two of the three final-state particles are detected. Nevertheless, although both results appear to be well-founded experimentally, one of them is obviously wrong. In order to resolve this disturbing situation, it is planned to repeat the two experiments at TUNL simultaneously [10]. To this end, both experiments are to be placed in the same neutron beam, one behind the other, thereby eliminating many relative uncertainties. Comparison Comparing the two experiments, each one had its specific advantages. Only the final-state geometry employed at TUNL allowed the use of a thick, active target, resulting in a higher count rate and facilitating the 269 Since all results [4,5,8] for the neutron-proton scattering length agree with each other, and also with the value known from free np scattering, it appears that the nd breakup reaction should, in principle, also be suitable for the extraction of ann. However, here a caveat might be in order. While modern 3N calculations describe most of the nd data very well, both below and above the breakup threshold, there are some striking exceptions. Specifically, in a recent experiment at Bonn [11], np and nn QFS have been measured in the nd reaction, with very surprising results: while for np QFS the calculations reproduce the measured cross section perfectly [12], there is a difference of almost 20% for nn QFS, corresponding to more than 5 standard deviations! (The nn part of this experiment will be repeated at the China Institute for Atomic Energy in Beijing [13].) Similarly, in the so-called "space star" geometry the measured nd breakup cross sections are some 25% larger than predicted [14]. Another case is the well known "Ay puzzle", i.e. the fact that the theory is unable to correctly describe the vector analyzing power in nd and pd scattering [15]. Finally, no threenucleon-force (3NF) effects have been observed in Ref. [4] although they are predicted by the theory and should have been seen in the experiment. Taken together, these observations strongly suggest that there are still some important parts missing in the theory, most likely in the 3NF, and that there might even be an as yet unknown difference between the nn and the np interaction. The nd breakup reaction is still the best tool for the investigation of these fundamental questions. REFERENCES 1. C.R. Howell et al., Phys. Lett. B 444, 252 (1998). 2. O. Schori, B. Gabioud, C. Joseph, J.P. Perroud, D. Rüegger, M.T. Tran, P. Truöl, E. Winkelmann, and W. Dahme, Phys. Rev. C35, 2252 (1987). 3. B. Gabioud et al., Nucl. Phys. A420, 496 (1984). 4. D.E. Gonzáles Trotter, F. Salinas, Q. Chen, A.S. Crowell, W. Glöckle, R.C. Howell, C.D. Roper, D. Schmidt, I. Slaus, H. Tang, W. Tornow, R.L. Walter, H. Witała, and Z. Zhou, Phys. Rev. Letters 83, 3788 (1999). 5. V. Huhn, L. Wätzold, Ch. Weber, A. Siepe, W. von Witsch, H. Witała, and W. Glöckle, Phys. Rev. C 63, 014003 (2001). 6. H. Witała, Th. Cornelius, and W. Glöckle, Few-Body Syst. 3, 123 (1988); H. Witała, W. Glöckle, and Th. Cornelius, Phys. Rev. C 39, 384 (1989); W. Glöckle, H. Witała, D. Hüber, H. Kamada, and J. Golak, Phys. Rep. 274, 107 (1996). 7. L. Koester and W. Nistler, Z. Phys. A 272, 189 (1975). 8. J. Deng, A. Siepe, and W. von Witsch, to be published. 9. see: K. Bodek, J. Krug, W. Lübke, S. Obermanns, H. Rühl, M. Steinke, M. Stephan, and D. Kamke, Few-Body Syst. 8, 23 (1990), and references therein. 10. private communication, C.R. Howell, Duke University and TUNL, Durham, N.C, U.S.A. 11. A. Siepe, J. Deng, V. Huhn, L. Wätzold, Ch. Weber, W. von Witsch, H. Witała, and W. Glöckle, Phys. Rev. C 65, 034010 (2002). 12. see also Ref. [5]. 13. private communication, Z. Zhou, CIAE, Beijing, People's Republic of China. 14. C.R. Howell et al., Nucl. Phys. A631, 692c (1998); and references therein. 15. E.M. Neidel and W. Tornow, TUNL Progress Report – XL, Durham, N.C., U.S.A. (2001) p. 21. 270
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