Elastic scattering measurements for the C10+Pb208 system at Elab=66 MeV

R. Linares, Mandira Sinha, E. N. Cardozo, V. Guimarães, G. V. Rogachev, J. Hooker, E. Koshchiy, T. Ahn, C. Hunt, H. Jayatissa, S. Upadhyayula, B. Roeder, A. Saastomoinen, J. Lubian, M. Rodríguez-Gallardo, J. Casal, K. C. C. Pires, M. Assunção, Y. Penionzhkevich, and S. Lukyanov
Phys. Rev. C 103, 044613 – Published 23 April 2021

Abstract

Background: The influence of halo structure of He6, B8, Be11, and Li11 nuclei in several mechanisms such as direct reactions and fusion is already established, although not completely understood. The influence of the C10 Brunnian structure is less known.

Purpose: To investigate the influence of the cluster configuration of C10 on the elastic scattering at an energy close to the Coulomb barrier.

Methods: We present experimental data for the elastic scattering of the C10+Pb208 system at Elab=66 MeV. The data are compared to the three- and the four-body continuum-discretized coupled-channels calculations assuming B9+p, Be6+α, and Be8+p+p configurations.

Results: The experimental angular distribution of the cross sections shows the suppression of the Fresnel peak that is reasonably well reproduced by the continuum-discretized coupled-channels calculations. However, the calculations underestimate the cross sections at backward angles. Couplings to continuum states represent a small effect.

Conclusions: The cluster configurations of C10 assumed in the present work are able to describe some of the features of the data. To explain the data at backward angles, experimental data for the breakup and an extension of theoretical formalism towards a four-body cluster seem to be in need to reproduce the measured angular distribution.

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  • Received 12 October 2020
  • Revised 30 December 2020
  • Accepted 5 April 2021

DOI:https://doi.org/10.1103/PhysRevC.103.044613

©2021 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

R. Linares1,*, Mandira Sinha2, E. N. Cardozo1,3, V. Guimarães3, G. V. Rogachev4,5,6, J. Hooker4,5, E. Koshchiy5, T. Ahn5, C. Hunt4,5, H. Jayatissa4,5,†, S. Upadhyayula4,5, B. Roeder5, A. Saastomoinen5, J. Lubian1, M. Rodríguez-Gallardo7,8, J. Casal7,9, K. C. C. Pires3, M. Assunção10, Y. Penionzhkevich11, and S. Lukyanov11

  • 1Instituto de Física, Universidade Federal Fluminense, 24210-340, Niterói, Rio de Janeiro, Brazil
  • 2Department of Physics, Bose Institute, 93/1 Acharya Prafulla Chandra Road, Kolkata-700009, West Bengal, India
  • 3Instituto de Física, Universidade de São Paulo, 05508-090 São Paulo, Brazil
  • 4Department of Physics and Astronomy, Texas A & M University, 77843 Texas, USA
  • 5Cyclotron Institute, Texas A & M University, 77843 Texas, USA
  • 6Nuclear Solutions Institute, Texas A & M University, 77843 Texas, USA
  • 7Departamento de Física Atómica, Molecular y Nuclear, Facultad de Física, Universidad de Sevilla, Apartado 1065, E-41080 Sevilla, Spain
  • 8Instituto Carlos I de Física Teórica y Computacional, Universidad de Sevilla, Spain
  • 9Dipartimento di Fisica e Astronomia “G. Galilei”, Università degli studi di Padova, and INFN - Sezione di Padova, Via Marzolo 8, I-35131 Padova, Italy
  • 10Departamento Física, Universidade Federal de São Paulo, Campus Diadema, 09913-030, Diadema, São Paulo, Brazil
  • 11Joint Institute for Nuclear Research, Dubna, Moscow region, 141980, Russia

  • *Corresponding author: rlinares@id.uff.br
  • Present address: Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA.

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Issue

Vol. 103, Iss. 4 — April 2021

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