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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

As Contributors: Andrzej Wilczek
Preprint link: scipost_201910_00038v1
Date accepted: 2019-12-20
Date submitted: 2019-10-26 02:00
Submitted by: Wilczek, Andrzej
Submitted to: SciPost Physics Proceedings
Proceedings issue: 24th European Few Body Conference (University of Surrey, U.K.)
Academic field: Physics
Specialties:
  • Nuclear Physics - Experiment

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.

Published as SciPost Phys. Proc. 3, 005 (2020)



Submission & Refereeing History

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Submission scipost_201910_00038v1 on 26 October 2019

Reports on this Submission

Report 1 by Paul Stevenson 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

Report

The report gives a status update of the study of the Space Star Anomaly in pd breakup based on analysis of data from BINA at 50-100MeV/A The introduction gives a readable background to the problem, followed by sections on the experimental work. Some representative results are given, with a forward look to future plans. The work should be published in the proceedings of the conference, as a well-written representation of the presented work at the EFB24 conference

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