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Wilczek, Andrzej; Szadziński, Albert; Bodek, Kazimierz; Ciepał, Izabela; Eslami-Kalantari, Mohammad; Kalantar Nayestanaki, Nasser; 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; ramazani sharifabadi, reza; Rozpȩdzik, Dagmara; Skwira-Chalot, Izabela; Stephan, Elżbieta; Włoch, Bogusław; [...]

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

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  • Media type: E-Article
  • Title: Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector
  • Contributor: Wilczek, Andrzej; Szadziński, Albert; Bodek, Kazimierz; Ciepał, Izabela; Eslami-Kalantari, Mohammad; Kalantar Nayestanaki, Nasser; 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; ramazani sharifabadi, reza; Rozpȩdzik, Dagmara; Skwira-Chalot, Izabela; Stephan, Elżbieta; Włoch, Bogusław; [...]
  • Published: Stichting SciPost, 2020
  • Published in: SciPost Physics Proceedings (2020) 3
  • Language: Not determined
  • DOI: 10.21468/scipostphysproc.3.005
  • ISSN: 2666-4003
  • Keywords: General Medicine ; General Chemistry
  • Origination:
  • Footnote:
  • Description: 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.
  • Access State: Open Access