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Fragmentation cross-sections for cosmic ray nuclei in the interstellar medium

<p>Table of the cumulative&nbsp;(included ghost nuclei) and direct fragmentation cross sections <strong>on H target</strong>&nbsp;generated with the <a href="https://github.com/carmeloevoli/XS4GCR">XS4GCR</a>&nbsp;code.</p> <p>More than 3800 channels are included from Ni64 to H1.</p> <ul> <li>Tables are&nbsp;saved as txt files with &#39; &#39; as delimiter.</li> <li>For each row the first 4 integers represent:&nbsp;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&nbsp;kinetic energy per nucleon</li> <li>The first row is identified with&nbsp;0 0 0 0 as the first 4 values&nbsp;and contains the values of the kinetic energy per nucleon (log spaced between 10&nbsp;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

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