Szczegóły publikacji
Opis bibliograficzny
Measurement of anti-$^{3}He$ nuclei absorption in matter and impact on their propagation in the Galaxy / S. Acharya, [et al.], B. BALIŚ, [et al.], M. GORGOŃ, [et al.], A. HORZYK, [et al.], M. JABŁOŃSKI, [et al.], J. KITOWSKI, [et al.], P. J. Konopka, [et al.], S. D. KORYCIAK, [et al.], P. G. RUSSEK, [et al.] // Nature Physics ; ISSN 1745-2473. — 2023 — vol. 19 no. 1, s. 61–71. — Bibliogr. s. 66–68, Abstr. — Publikacja dostępna online od: 2022-12-12. — P. J. Konopka - afiliacja: European Organization for Nuclear Research (CERN), Geneva, Switzerland
Autorzy (1032)
Dane bibliometryczne
| ID BaDAP | 145060 |
|---|---|
| Data dodania do BaDAP | 2023-02-22 |
| Tekst źródłowy | URL |
| DOI | 10.1038/s41567-022-01804-8 |
| Rok publikacji | 2023 |
| Typ publikacji | artykuł w czasopiśmie |
| Otwarty dostęp |  |
| Creative Commons | |
| Czasopismo/seria | Nature Physics |
Abstract
In our Galaxy, light antinuclei composed of antiprotons and antineutrons can be produced through high-energy cosmic-ray collisions with the interstellar medium or could also originate from the annihilation of dark-matter particles that have not yet been discovered. On Earth, the only way to produce and study antinuclei with high precision is to create them at high-energy particle accelerators. Although the properties of elementary antiparticles have been studied in detail, the knowledge of the interaction of light antinuclei with matter is limited. We determine the disappearance probability of 3He ¯ when it encounters matter particles and annihilates or disintegrates within the ALICE detector at the Large Hadron Collider. We extract the inelastic interaction cross section, which is then used as an input to the calculations of the transparency of our Galaxy to the propagation of 3He ¯ stemming from dark-matter annihilation and cosmic-ray interactions within the interstellar medium. For a specific dark-matter profile, we estimate a transparency of about 50%, whereas it varies with increasing 3He ¯ momentum from 25% to 90% for cosmic-ray sources. The results indicate that 3He ¯ nuclei can travel long distances in the Galaxy, and can be used to study cosmic-ray interactions and dark-matter annihilation.