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The 6He Optical Potential at energies around the Coulomb barrier J. P. Fernández-Garcíaa, b, M. Rodríguez-Gallardoa, c, M. A. G. Alvareza, b, A. M. Moroa a Dpto. de FAMN, Universidad de Sevilla, Apdo. 1065, 41080 Sevilla, Spain. b CNA, Universidad de Sevilla, c/ Thomas Alva Edison 7, 41092 Sevilla, Spain. c Instituto de Estructura de la Materia, CSIC, Serrano 123, 28006 Madrid, Spain. Abstract. We present an Optical Model (OM) study of 6He on 208Pb elastic scattering data, measured at laboratory energies around the Coulomb barrier (Elab=14, 16, 18, 22, and 27 MeV) [1]. For the projectile-target bare interaction, we use the microscopic São Paulo Potential (SPP). This bare interaction is supplemented with a Coulomb Dipole Polarization (CDP) potential, as well as a diffuse complex Woods-Saxon potential. Four-body Continuum-Discretized-Coupled-Channels (CDCC) calculations have been performed in order to support the optical model analysis. We have also studied the channel, which is the dominant reaction process. In the analysis of this channel, we compare the angular and energy distributions of the particles measured at 22 MeV, with Distorted Wave Born Approximation (DWBA) calculations. Keywords: Nuclear reaction 6He+208Pb, halo nucleus, Coulomb dipole polarizability, Coulomb barrier, threshold anomaly, optical model and DWBA calculations. PACS: 25.60.Dz, 25.60.Bx, 21.10.Gv, 27.20.+n OPTICAL MODEL CALCULATIONS We have performed OM calculations, in which the 6He + 208Pb potential is parametrized according to the following expression, U TOT r =V Coul r +V SPP r +U Pol r , (1) where VSPP(r) is a nuclear microscopic bare potential [2], VCoul(r) represents the Coulomb interaction, and Upol(r) contains the effects of reaction channels on the elastic scattering, given by the equation, U Pol r =U CDP r +V L r +iW L r . (2) Here UCDP(r) represents the dynamic CDP potential derived in Ref. [3], which depends only on the B(E1) distribution of the 6He projectile, and VL(r) and WL(r) are the real and imaginary parts of the phenomenological Woods-Saxon potential. The parameters of 221 CREDIT LINE (BELOW) TO BE INSERTED ON THE FIRST PAGE OF EACH PAPER CP1231, La Rábida 2009, International Scientific Meeting on Nuclear Physics, Basic Concepts in Nuclear Physics: Theory, Experiments, and Applications, edited by J. A. Caballero, C. E. Alonso, M. V. Andrés, J. E. García-Ramos, and F. Pérez-Bernal © 2010 American Institute of Physics 978-0-7354-0776-3/10/$30.00
these terms are obtained by means of a 2 fit of the elastic data. In order to obtain satisfactory fits, a large value of the diffuseness of the real and imaginary parts is required (ar ~ ai~1 fm). This is in agreement with the results found in [1]. CDCC calculations [4], based on a 3-body model of 6He ( + n + n), have also been performed. The local equivalent potential derived from these calculations have a long range, which is consistent with the large diffuseness parameters found in the OM analysis. The energy dependence of the strengths of the real and imaginary parts of the optical potential show a correlation consistent with dispersion relations [5]. (a) (b) FIGURE 1. (a) Elastic scattering angular distribution and calculations. The solid lines represent the optical model calculations using the Eq. 1. (b) Energy distribution of particles. Transfer to the continuum calculations (solid line) are compared with the experimental data. STUDY OF CHANNEL We have also analyzed the production channel. The experimental data show that this channel is the main reaction process [6]. We study this channel by means of Distorted Wave Born Approximation (DWBA) calculations, assuming that the particles are produced by transferring the two valence neutrons to bound and unbound states of the target. In this transfer mechanism, the continuum states are discretized and divided into a set of energy packages (bins). Comparing with the experimental data, we conclude that the particles are produced mainly by a two-neutron transfer mechanism to very excited states of the target. REFERENCES. 1. A. M. Sánchez-Benítez et al. Nucl. Phys. A803, 30 (2008). 2. L. C. Chamon et al. Phys. Rev. C66, 014610 (2002). 3. M. V. Andrés, J. Gómez-Camacho, M. A. Nagarajan, Nucl. Phys. A579, 273 (1994). 4. M. Rodríguez-Gallardo et al. Phys. Rev. C77, 064609 (2008). 5. G. R. Satchler, Phys. Rep. 199, 147 (1991). 6. D. Escrig et al. Nucl. Phys. A792, 2 (2007). 222