Fragmentation cross-sections for cosmic ray nuclei in the interstellar medium
<p>Table of the cumulative (included ghost nuclei) and direct fragmentation cross sections <strong>on H target</strong> generated with the <a href="https://github.com/carmeloevoli/XS4GCR">XS4GCR</a> code.</p> <p>More than 3800 channels are included from Ni64 to H1.</p> <ul> <li>Tables are saved as txt files with ' ' as delimiter.</li> <li>For each row the first 4 integers represent: fragment Z, fragment A, projectile Z and projectile A</li> <li>The following 160 values are the cross sections (in mbarn) as a function of the projectile kinetic energy per nucleon</li> <li>The first row is identified with 0 0 0 0 as the first 4 values and contains the values of the kinetic energy per nucleon (log spaced between 10 MeV/n and 1 TeV/n) at which the cross sections are computed.</li> </ul>
ShareScore
36/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 8
- Harmonization
- 8
- Access
- 16
- Reuse readiness
- 0
- Engagement
- 4