Cargando…
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: | , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Lenguaje: | eng |
Publicado: |
2020
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.21468/SciPostPhysProc.3.005 http://cds.cern.ch/record/2713478 |