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Current stage of studies of the star configurations at intermediate energies with the use of the BINA detector
by A. Wilczek, A. Szadzinski, K. Bodek, I. Ciepal, N. Kalantar-Nayestanaki, G. Khatri, St. Kistryn, B. Klos, A. Kozela, J. Kubos, P. Kulessa, A. Lobejko, A. Magiera, J. Messchendorp, I. Mazumdar, W. Parol, R. Ramazani-Sharifabadi, D. Rozpedzik, I. Skwira-Chalot, E. Stephan, B. Wloch, A. Wronska, and J. Zejma
Submission summary
| Authors (as registered SciPost users): | Andrzej Wilczek |
| Submission information | |
|---|---|
| Preprint Link: | scipost_201910_00038v1 (pdf) |
| Date accepted: | Dec. 20, 2019 |
| Date submitted: | Oct. 26, 2019, 2 a.m. |
| Submitted by: | Andrzej Wilczek |
| Submitted to: | SciPost Physics Proceedings |
| Proceedings issue: | 24th European Few Body Conference (EFB2019) |
| Ontological classification | |
|---|---|
| Academic field: | Physics |
| Specialties: |
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Abstract
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.
Current status:
Editorial decision:
For Journal SciPost Physics Proceedings: Publish
(status: Editorial decision fixed and (if required) accepted by authors)
Reports on this Submission
Report #1 by Paul Stevenson (Referee 1) on 2019-12-17 (Contributed Report)
- Cite as: Paul Stevenson, Report on arXiv:scipost_201910_00038v1, delivered 2019-12-17, doi: 10.21468/SciPost.Report.1495