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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...
| Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , |
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| Lenguaje: | eng |
| Publicado: |
2020
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.21468/SciPostPhysProc.3.005 http://cds.cern.ch/record/2713478 |
| _version_ | 1780965400590155776 |
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| author | 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 |
| author_facet | 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 |
| author_sort | Wilczek, Andrzej |
| collection | CERN |
| 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. |
| id | oai-inspirehep.net-1784960 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2020 |
| record_format | invenio |
| spelling | oai-inspirehep.net-17849602020-03-21T20:57:55Zdoi:10.21468/SciPostPhysProc.3.005http://cds.cern.ch/record/2713478engWilczek, AndrzejSzadziński, AlbertBodek, KazimierzCiepał, IzabelaEslami-Kalantari, MohammadNayestanaki, Nasser KalantarKhatri, GhanshyambhaiKistryn, StanisławKłos, BarbaraKozela, AdamKuboś, JoannaKulessa, PawełŁobejko, AngelinaMagiera, AndrzejMardanpour, HosseinMesschendorp, JohanMazumdar, IndranilParol, WiktorRamazani-Moghaddam-Aran, AhmadRozpȩdzik, DagmaraSkwira-Chalot, IzabelaStephan, ElżbietaWłoch, BogusławWrońska, AleksandraZejma, JacekCurrent stage of studies of the star configurations at intermediate energies with the use of the BINA detectorNuclear Physics - ExperimentThe 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.oai:inspirehep.net:17849602020 |
| spellingShingle | Nuclear Physics - Experiment 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 Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector |
| title | Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector |
| title_full | Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector |
| title_fullStr | Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector |
| title_full_unstemmed | Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector |
| title_short | Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector |
| title_sort | current stage of studies of the star configurations at intermediate energies with the use of the bina detector |
| topic | Nuclear Physics - Experiment |
| url | https://dx.doi.org/10.21468/SciPostPhysProc.3.005 http://cds.cern.ch/record/2713478 |
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