Szczegóły publikacji
Opis bibliograficzny
First measurements of deuteron production spectra in p+p collisions at beam momentum of 158 GeV/c at the NA61/SHINE spectrometer at the CERN SPS / Anirvan Shukla, [et al.], W. KUCEWICZ, [et al.], Ł. MIK, [et al.], K. WITEK, [et al.] // PoS Proceedings of Science [Dokument elektroniczny]. — Czasopismo elektroniczne ; ISSN 1824-8039 . — 2025 — vol. 501 art. no. 397, s. 1–14. — Wymagania systemowe: Adobe Reader. — Bibliogr. s. 11–12, Abstr. — Publikacja dostępna online od: 2025-12-30. — ICRC 2025 : 39th International Cosmic Ray Conference : 15–24 July 2025, Geneva, Switzerland
Autorzy (144)
- AGHKucewicz Wojciech
- AGHMik Łukasz
- AGHWitek Kamil
- Shukla Anirvan
Dane bibliometryczne
| ID BaDAP | 167008 |
|---|---|
| Data dodania do BaDAP | 2026-04-24 |
| Tekst źródłowy | URL |
| DOI | 10.22323/1.501.0397 |
| Rok publikacji | 2025 |
| Typ publikacji | referat w czasopiśmie |
| Otwarty dostęp | |
| Creative Commons | |
| Czasopismo/seria | PoS Proceedings of Science |
Abstract
The NA61/SHINE spectrometer at the CERN Super Proton Synchrotron (SPS) scans particle production in collisions of nuclei with various sizes at a set of energies covering the SPS energy range towards various physics goals. This paper presents the first differential production measurements of deuterons at energies relevant for cosmic-ray studies, produced in inelastic p+p interactions at incident projectile momentum of 158 GeV/c (√s = 17.3 GeV). The double-differential spectra are presented as functions of rapidity and transverse momentum and are compared to predictions of the thermal and coalescence models. These measurements are essential for improving our understanding of cosmic (anti)nuclei production, as detecting cosmic antinuclei can be a breakthrough approach to identifying dark matter. The primary source of cosmic antinuclei background is interactions between cosmic-ray protons and interstellar hydrogen gas. Gaining a deeper insight into the deuteron production mechanism in p+p interactions is an essential first step in modeling cosmic antinuclei production.