Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector

The Space Star Anomaly in proton-deuteron breakup cross-section occurs at energies of about 10 MeV. Data for higher energies are sparse. Therefore, a systematic scan over star configurations in the range of intermediate energies between 50 and 100 MeV/nucleon is carried out on the basis of data coll...

Descripción completa

Detalles Bibliográficos
Autores principales: Wilczek, Andrzej, Szadziński, Albert, Bodek, Kazimierz, Ciepał, Izabela, Eslami-Kalantari, Mohammad, Nayestanaki, Nasser Kalantar, Khatri, Ghanshyambhai, Kistryn, Stanisław, Kłos, Barbara, Kozela, Adam, Kuboś, Joanna, Kulessa, Paweł, Łobejko, Angelina, Magiera, Andrzej, Mardanpour, Hossein, Messchendorp, Johan, Mazumdar, Indranil, Parol, Wiktor, Ramazani-Moghaddam-Aran, Ahmad, Rozpȩdzik, Dagmara, Skwira-Chalot, Izabela, Stephan, Elżbieta, Włoch, Bogusław, Wrońska, Aleksandra, Zejma, Jacek
Lenguaje:eng
Publicado: 2020
Materias:
Nuclear Physics - Experiment
Acceso en línea:https://dx.doi.org/10.21468/SciPostPhysProc.3.005
http://cds.cern.ch/record/2713478
Descripción
Sumario:The Space Star Anomaly in proton-deuteron breakup cross-section occurs at energies of about 10 MeV. Data for higher energies are sparse. Therefore, a systematic scan over star configurations in the range of intermediate energies between 50 and 100 MeV/nucleon is carried out on the basis of data collected with the large acceptance BINA detector. The preliminary cross section results for forward star configurations at 80 MeV/nucleon slightly surpass the theoretical calculations, but the systematic uncertainties are still under study. Also, a new variable describing rotation of star configurations is proposed.

Ejemplares similares