Abstract
The new technique of accelerator mass spectrometry was successfully applied to measure the 26Mg(p, n)26 Alg (7.2 × 105 yr) cross section for proton energies Ep = 5.2−6.9 MeV. This cross section thar threshold is of astrophysical interest because of the recently observed 26Mg excess in meteoritic material and its bearing on the early solar system.
| Original language | English |
|---|---|
| Pages (from-to) | 303-306 |
| Number of pages | 4 |
| Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
| Volume | 94 |
| Issue number | 3 |
| DOIs | |
| State | Published - 1980 |
| Externally published | Yes |
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