Mass, total kinetic energy, and neutron multiplicity correlations in the binary fragmentation of Ti50+Pb208 at 294 MeV bombarding energy

S. Appannababu, M. Cinausero, T. Marchi, F. Gramegna, G. Prete, J. Bermudez, D. Fabris, G. Collazuol, A. Saxena, B. K. Nayak, S. Kailas, M. Bruno, L. Morelli, N. Gelli, S. Piantelli, G. Pasquali, S. Barlini, S. Valdré, E. Vardaci, L. Sajo-Bohus, M. Degerlier, A. Jhingan, B. R. Behera, and V. L. Kravchuk
Phys. Rev. C 94, 044618 – Published 27 October 2016

Abstract

The correlations between mass distributions of the binary fragments, total kinetic energy (TKE), and neutron multiplicity have been investigated for the reaction Ti50+Pb208 at 294 MeV bombarding energy. Although this reaction has been used to synthesize the Rf (Z=104) superheavy element, a complete study of its fragmentation dynamics is still not available in the literature. In this work, average neutron multiplicities were extracted as a function of different fragment mass splits and TKE windows. A weak increase of the prescission neutron multiplicity is observed going from asymmetric to symmetric mass splits. A fission delay time of 4.5×1020 s has been extracted for the symmetric fission. The neutron multiplicity extracted for the symmetric mass split was used to derive the average number of neutrons emitted in the spontaneous fission of Rf258. The extrapolated value of 4.7±1.4 is found to be consistent with systematics of spontaneous and neutron-induced fission in heavy nuclei and with the results of previous works for superheavy nuclei with Z=116 and Z=124.

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  • Received 8 January 2016
  • Revised 17 August 2016

DOI:https://doi.org/10.1103/PhysRevC.94.044618

©2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

S. Appannababu1,*, M. Cinausero1,†, T. Marchi1,‡, F. Gramegna1, G. Prete1, J. Bermudez1, D. Fabris2, G. Collazuol2,3, A. Saxena4, B. K. Nayak4, S. Kailas4, M. Bruno5, L. Morelli5, N. Gelli6, S. Piantelli6, G. Pasquali6,7, S. Barlini6,7, S. Valdré6,7, E. Vardaci8, L. Sajo-Bohus9, M. Degerlier10, A. Jhingan11, B. R. Behera12, and V. L. Kravchuk13

  • 1I.N.F.N. Laboratori Nazionali di Legnaro, Italy
  • 2I.N.F.N. Sezione di Padova, Italy
  • 3Dipartimento di Fisica e Astronomia dell'Università di Padova, Italy
  • 4Nuclear Physics Division, Bhabha Atomic Research Centre, Mumbai, India
  • 5Sezione I.N.F.N. and Dipartimento di Fisica e Astronomia dell'Università di Bologna, Italy
  • 6I.N.F.N. Sezione di Firenze, Italy
  • 7Dipartimento di Fisica dell'Università di Firenze, Italy
  • 8Sezione I.N.F.N. and Dipartimento di Scienze Fisiche, Università Federico II, Napoli, Italy
  • 9Universidad Simon Bolivar, Caracas, Venezuela
  • 10Nevsehir Haci Bektas University Science and Art Faculty Physics Department, Nevsehir, Turkey
  • 11Inter-University Accelerator Centre, New Delhi, India
  • 12Department of Physics, Panjab University, Chandigarh, India
  • 13National Research Centre“Kurchatov Institute,” Moscow, Russia

  • *Present Address: Departamento de Fisica Nuclear - Instituto de Fisica - Universidade de Sao Paulo, Brazil.
  • Corrsponding author: cinausero@lnl.infn.it
  • Present Address: KU Leuven Department of Physics and Astronomy Instituut voor Kern- en Stralingsfysica, Leuven, Belgium.

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Vol. 94, Iss. 4 — October 2016

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