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...
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Format: | Article |
Language: | English |
Published: |
SciPost
2020-02-01
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Series: | SciPost Physics Proceedings |
Online Access: | https://scipost.org/SciPostPhysProc.3.005 |