Email this article 
Cosmophysical aspects of relativistic nuclear fragmentation
- Authors: Zaitsev A.A.1,2, Marimuthu N.1, Artemenkov D.A.1, Zarubin P.I.1,2, Peresadʹko N.G.1,2, Rusakova V.V.1
-
Affiliations:
- Joint Institute for Nuclear Research
- P. N. Lebedev Physical Institute of the Russian Academy of Sciences
- Issue: Vol 87, No 1 (2024)
- Pages: 40-44
- Section: ЭЛЕМЕНТАРНЫЕ ЧАСТИЦЫ И ПОЛЯ. Эксперимент
- Published: 03.10.2024
- URL: https://cardiosomatics.ru/0044-0027/article/view/674672
- DOI: https://doi.org/10.31857/S0044002724010066
- EDN: https://elibrary.ru/KEDJQJ
- ID: 674672
Cite item
Open Access
Access granted
Subscription Access
Abstract
The status of the study of multiple fragmentation of 950 MeV per nucleon Kr nuclei in a nuclear track emulsion aimed at determining the contributions of 2α decays of 8Be, the Hoyle 3α state, and the search for a 4α particle condensate state, is presented. In events with the production of few relativistic fragments of He and H, the possibility of estimating the multiplicity of neutrons in the fragmentation cone of a projectile nucleus is studied. For the planar component of neutron transverse momenta estimated from the angles of observed secondary stars, the Rayleigh distribution parameter was 35 ± 7 MeV/c. The importance of such events for the interpretation of cosmophysical observations is noted.
About the authors
A. A. Zaitsev
Joint Institute for Nuclear Research; P. N. Lebedev Physical Institute of the Russian Academy of Sciences
Author for correspondence.
Email: zaicev@jinr.ru
Russian Federation, Dubna; Moscow
N. Marimuthu
Joint Institute for Nuclear Research
Email: zaicev@jinr.ru
Russian Federation, Dubna
D. A. Artemenkov
Joint Institute for Nuclear Research
Email: zaicev@jinr.ru
Russian Federation, Dubna
P. I. Zarubin
Joint Institute for Nuclear Research; P. N. Lebedev Physical Institute of the Russian Academy of Sciences
Email: zaicev@jinr.ru
Russian Federation, Dubna; Moscow
N. G. Peresadʹko
Email: zaicev@jinr.ru
Russian Federation
V. V. Rusakova
Joint Institute for Nuclear Research
Email: zaicev@jinr.ru
Russian Federation, Dubna
References
- D. A. Artemenkov, V. Bradnova, O. N. Kashanskaya, N. V. Kondratieva, N. K. Kornegrutsa, E. Mitsova, N. G. Peresadko, V. V. Rusakova, R. Stanoeva, A. A. Zaitsev, I. G. Zarubina, and P. I. Zarubin, Phys. At. Nucl. 85, 528 (2022); doi.org/10.1134/S1063778822060035; arXiv: 2206.09690.
- A. Tohsaki, H. Horiuchi, P. Schuck, and G. Ropke, Rev. Mod. Phys. 89, 011002 (2017); doi.org/10.1103/RevModPhys.89.011002
- W. von Oertzen, Lect. Notes Phys. 818, 1 (2010); doi.org/10.1007/978-3-642-13899-7_3
- J. Abdallah et al. (DELPHI Collab.), Astophys. J. 28, 273 (2007); doi.org/10.1016/j.astropartphys.2007.06.001; arXiv: 0706.2561 [astro-ph].
- A. G. Bogdanov, R. P. Kokoulin, G. Manocchi, A. A. Petrukhin, and O. Saavedra, Astophys. J. 98, 13 (2018); doi.org/10.1016/j.astropartphys.2018.01.003
- V. S. Vorobev and A. A. Petrukhin, Phys. At. Nucl. 84, 934 (2021); doi.org/10.1134/S1063778821130408
- G. Trinchero, M. B. Amelchakov, A. G. Bogdanov, A. Chiavassa, A. N. Dmitrieva, G. Mannocchi, S. S. Khokhlov, R. P. Kokoulin, K. G. Kompaniets, A. A. Petrukhin, V. V. Shutenko, I. A. Shulzhenko, I. I. Yashin, and E. A. Yurina, Astophys. J. 945, 123 (2023); doi.org/10.3847/1538-4357/acb1fc; arXiv: 2210.09690.
- S. Typel, G. Röpke, T. Klähn, D. Blaschke, and H. H. Wolter, Phys. Rev. C 81, 015803 (2010); doi.org/10.1103/PhysRevC.81.015803; arXiv.org/ abs/0908.2344 [nucl-th].
Supplementary files
