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Production cross sections for intermediate mass fragments from dynamical and statistical decay of projectile-like fragments in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Sn</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>124</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">Ni</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>64</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Sn</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>112</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>+</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">Ni</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>58</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>collisions at<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>35</mml:mn><mml:mspace width="4pt"/><mml:mi>A</mml:mi></mml:mrow></mml:math>MeV

P. RussottoINFN, Sezione di Catania, ItalyE. De FilippoINFN, Sezione di Catania, ItalyA. PaganoINFN, Sezione di Catania, ItalyL. AcostaINFN, Laboratori Nazionali del Sud, Catania, ItalyL. AuditoreINFN, Gruppo Collegato di Messina and Dip. di Fisica, Univ. di Messina, ItalyV. BaranPhysics Faculty, University of Bucharest, RomaniaI. BerceanuNational Institute of Physics and Nuclear Engineering “Horia Hulubei,” Bucharest, RomaniaB. BorderieInstitut de Physique Nucléaire, CNRS/IN2P3, Université Paris-Sud 11, Orsay, FranceR. BougaultLPC Caen, ENSICAEN, University of Caen, CNRS/IN2P3, Caen FranceM. BrunoINFN, Sezione di Bologna and Dipartimento di Fisica, Univ. di Bologna, ItalyT. CapFaculty of Physics, University of Warsaw, Warsaw, PolandG. CardellaINFN, Sezione di Catania, ItalyS. CavallaroDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyM. B. ChatterjeeSaha Institute of Nuclear Physics, Kolkata, IndiaA. ChbihiGANIL (DSM-CEA/CNRS/IN2P3), Caen, FranceM. ColonnaINFN, Laboratori Nazionali del Sud, Catania, ItalyM. D’AgostinoINFN, Sezione di Bologna and Dipartimento di Fisica, Univ. di Bologna, ItalyM. Di ToroDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyL. FrancalanzaDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyJ. D. FranklandGANIL (DSM-CEA/CNRS/IN2P3), Caen, FranceE. GalichetConservatoire National des Arts et Métiers, F-75141 Paris Cedex 03, FranceW. GawlikowiczCardinal Stefan Wyszyński University, Warsaw, PolandE. GeraciDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyB. GnoffoDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyA. GrzeszczukInstitute of Physics, University of Silesia, Katowice, PolandP. GuazzoniINFN, Sezione di Milano and Dipartimento di Fisica, Univ. di Milano, ItalyS. KowalskiInstitute of Physics, University of Silesia, Katowice, PolandG. LanzaloneINFN, Laboratori Nazionali del Sud, Catania, ItalyG. LanzanòINFN, Sezione di Catania, ItalyN. Le NeindreLPC Caen, ENSICAEN, University of Caen, CNRS/IN2P3, Caen FranceI. LombardoINFN, Sezione di Napoli and Dipartimento di Fisica, Univ. di Napoli, ItalyC. MaiolinoINFN, Laboratori Nazionali del Sud, Catania, ItalyT. MinnitiINFN, Sezione di Catania, ItalyE.V. PaganoDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyM. PapaINFN, Sezione di Catania, ItalyE. PiaseckiHeavy Ion Laboratory, University of Warsaw, Warsaw, PolandS. PirroneINFN, Sezione di Catania, ItalyR. PłanetaM. Smoluchowski Institute of Physics, Jagellonian Univ., Cracow, PolandG. PolitiDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyF. PortoDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyL. QuattrocchiINFN, Gruppo Collegato di Messina and Dip. di Fisica, Univ. di Messina, ItalyM. F. RivetInstitut de Physique Nucléaire, CNRS/IN2P3, Université Paris-Sud 11, Orsay, FranceE. RosatoINFN, Sezione di Napoli and Dipartimento di Fisica, Univ. di Napoli, ItalyF. RizzoDipartimento di Fisica e Astronomia, Univ. di Catania, Catania, ItalyK. SchmidtInstitute of Physics, University of Silesia, Katowice, PolandK. Siwek-WilczyńskaFaculty of Physics, University of Warsaw, Warsaw, PolandI. Skwira-ChalotFaculty of Physics, University of Warsaw, Warsaw, PolandA. TrifiròINFN, Gruppo Collegato di Messina and Dip. di Fisica, Univ. di Messina, ItalyM. TrimarchìINFN, Gruppo Collegato di Messina and Dip. di Fisica, Univ. di Messina, ItalyG. VerdeINFN, Sezione di Catania, ItalyM. VigilanteINFN, Sezione di Napoli and Dipartimento di Fisica, Univ. di Napoli, ItalyJ. P. WieleczkoGANIL (DSM-CEA/CNRS/IN2P3), Caen, FranceJ. WilczyńskíNational Centre for Nuclear Research, Świerk/Warsaw, PolandL. ZettaINFN, Sezione di Milano and Dipartimento di Fisica, Univ. di Milano, ItalyW. ZipperInstitute of Physics, University of Silesia, Katowice, Poland
2015lv
ABI

Аннотация

Background: In heavy-ion collisions at intermediate energies the production of light charged particles and intermediate mass fragments (IMFs) is due to different reaction mechanisms and different time scales, ranging from fast dynamical processes to statistical emission from the equilibrated system.Purpose: We compare the IMF statistical and dynamical emission probabilities in collisions of a neutron-rich $^{124}\mathrm{Sn}+^{64}\mathrm{Ni}$ system and a neutron-poor $^{112}\mathrm{Sn}+^{58}\mathrm{Ni}$ system at the laboratory energy of 35 $A$ MeV.Method: The IMFs production mechanism in semiperipheral reactions has been investigated in our previous works. In this paper, the analysis is expanded for the same set of data and production cross sections have been evaluated for dynamical and statistical emission in a coherent way for light and heavy fragments.Results: The data analysis has evidenced a strong competition between dynamical and statistical emission mechanisms. Probability of the dynamical emission of IMFs is strongly influenced by the ($N/Z$) ratio of the colliding system.Conclusions: It is demonstrated that the statistical emission is equally probable for the two systems, while the dynamical emission is enhanced for the neutron-rich system, especially for heavy fragments ($Z\ensuremath{\ge}6$). The observed effect points at a high sensitivity of the prompt-dynamical emission to the ($N/Z$) ratio of a given system.

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