Bulletin of the American Physical Society
5th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Volume 63, Number 12
Tuesday–Saturday, October 23–27, 2018; Waikoloa, Hawaii
Session MF: Nuclear Matter and Nuclear Astrophysics
2:00 PM–5:00 PM,
Saturday, October 27, 2018
Hilton
Room: King's 2
Chair: Jeremy Holt, Texas A&M University
Abstract ID: BAPS.2018.HAW.MF.3
Abstract: MF.00003 : Study of light cluster production in intermediate energetic heavy-RI collision at RIBF*
2:30 PM–2:45 PM
Presenter:
Masanori Kaneko
(Department of Physics, Kyoto university)
Author:
Masanori Kaneko
(Department of Physics, Kyoto university)
The physics motivation of the SpiRIT (SAMURAI Pion-reconstruction and Ion Tracker) collaboration is to place a constraint on the symmetry energy term in the nuclear equation of state at around twice saturation densities. Charged pion ratio in intermediate energetic heavy-ion collisions(HIC) is predicted as a good probe to extract symmetry energy, however, there is still large model dependence. Not only nucleon dynamics but also cluster-cluster correlation in HIC are reported to influence pion production. In order to discuss pion with less uncertainty, it is necessary to understand properties on nucleon and cluster well.
We performed the experiment at the RIKEN-RIBF with four kinds of Sn-Sn isotopic collisions at 270 MeV/nucleon in spring 2016. Charged particles were measured and identified by the SpiRIT-TPC in combination with the SAMURAI magnet. Light charged particles(LCP) in HIC could be a possible benchmark to understand cluster property. In this talk, yields of LCP and their dynamics will be discussed.
*This work is supported by the Japanese MEXT KAKENHI grant No. 24105004, and the U.S. DOE underĀ Grant Nos. DE-SC0004835, DE-SC0014530, DE-NA0002923, the US NSF Grant No. PHY-1565546, and the Polish NSC Grant Nos. UMO-2013/09/B/ST2/04064 and UMO-2013/10/M/ST2/00624.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.MF.3
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