Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment
| dc.creator | Ahn, H. S. | |
| dc.creator | Allison, P. S. | |
| dc.creator | Bagliesi, M. G. | |
| dc.creator | Beatty, J. J. | |
| dc.creator | Bigongiari, G. | |
| dc.creator | Boyle, P. J. | |
| dc.creator | Brandt, T. J. | |
| dc.creator | Childers, J. T. | |
| dc.creator | Conklin, N. B. | |
| dc.creator | Coutu, S. | |
| dc.creator | Duvernois, M. A. | |
| dc.creator | Ganel, O. | |
| dc.creator | Han, J. H. | |
| dc.creator | Hyun, H. J. | |
| dc.creator | Jeon, J. A. | |
| dc.creator | Kim, K. C. | |
| dc.creator | Lee, J. K. | |
| dc.creator | Lee, M. H. | |
| dc.creator | Lutz, L. | |
| dc.creator | Maestro, P. | |
| dc.creator | Malinin, A. | |
| dc.creator | Marrocchesi, P. S. | |
| dc.creator | Minnick, S. A. | |
| dc.creator | Mognet, S. I. | |
| dc.creator | Nam, S. | |
| dc.creator | Nutter, S. L. | |
| dc.creator | Park, I. H. | |
| dc.creator | Park, N. H. | |
| dc.creator | Seo, E. S. | |
| dc.creator | Sina, R. | |
| dc.creator | Swordy, S. P. | |
| dc.creator | Wakely, S. P. | |
| dc.creator | Wu, J. | |
| dc.creator | Yang, J. | |
| dc.creator | Yoon, Y. S. | |
| dc.creator | Zei, R. | |
| dc.creator | Zinn, S. Y. | |
| dc.date | 2008-08-12 | |
| dc.date.accessioned | 2026-07-07T10:12:18Z | |
| dc.date.available | 2026-07-07T10:12:18Z | |
| dc.description | We present new measurements of heavy cosmic-ray nuclei at high energies per- formed during the first flight of the balloon-borne cosmic-ray experiment CREAM (Cosmic-Ray Energetics And Mass). This instrument uses multiple charge detectors and a transition radiation detector to provide the first high accuracy measurements of the relative abundances of elements from boron to oxygen up to energies around 1 TeV/n. The data agree with previous measurements at lower energies and show a relatively steep decline (~E$^-0.6$ to E$^-0.5$) at high energies. They further show the source abundance of nitrogen relative to oxygen is ~10% in the TeV/n region. | |
| dc.description | Accepted for publication in Astroparticle Physics | |
| dc.identifier | https://arxiv.org/abs/0808.1718 | |
| dc.identifier | http://arxiv.org/abs/0808.1718 | |
| dc.identifier | Astropart. Phys. 30 (2008) 133-141 | |
| dc.identifier | doi:10.1016/j.astropartphys.2008.07.010 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/172139 | |
| dc.subject | Astrophysics | |
| dc.title | Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment | |
| dc.type | text |