Cosmophysical aspects of relativistic nuclear fragmentation

Fuente: arXiv
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Bibliographic Details
Main Authors: Zaitsev, A. A., Marimuthu, N., Artemenkov, D. A., Zarubin, P. I., Peresadko, N. G., Rusakova, V. V.
Format: Preprint
Published: 2023
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_version_ 1866913239201218560
author Zaitsev, A. A.
Marimuthu, N.
Artemenkov, D. A.
Zarubin, P. I.
Peresadko, N. G.
Rusakova, V. V.
author_facet Zaitsev, A. A.
Marimuthu, N.
Artemenkov, D. A.
Zarubin, P. I.
Peresadko, N. G.
Rusakova, V. V.
contents 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 2$α$ decays of $^{8}$Be, the Hoyle 3$α$ state, and the search for a 4$α$ 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 $\pm$ 7 MeV/$c$. The importance of such events for the interpretation of cosmophysical observations is noted.
format Preprint
id arxiv_https___arxiv_org_abs_2307_16465
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Cosmophysical aspects of relativistic nuclear fragmentation
Zaitsev, A. A.
Marimuthu, N.
Artemenkov, D. A.
Zarubin, P. I.
Peresadko, N. G.
Rusakova, V. V.
Nuclear Experiment
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 2$α$ decays of $^{8}$Be, the Hoyle 3$α$ state, and the search for a 4$α$ 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 $\pm$ 7 MeV/$c$. The importance of such events for the interpretation of cosmophysical observations is noted.
title Cosmophysical aspects of relativistic nuclear fragmentation
topic Nuclear Experiment
url https://arxiv.org/abs/2307.16465