first test on the 22ne(p,γ)23na reaction at luna

Clicks: 70
ID: 219037
2014
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This article has not been analysed, so there is no overall score — reader engagement is measured and shown alongside.
AI Quality Assessment
Not analyzed
Readership in this journal
Steady

Ranked #484 of 625 articles by views in utilitas mathematica

Most read Least read

Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 625 in total.

Mint this article as an NFT
Not yet minted

Create a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.

5 SUSD one-off · no wallet required
Abstract
The 22Ne(p,γ)23Na reaction is involved in the hydrogen burning neon-sodium cycle. In second-generation stars, where the central temperature is higher than 0.05 109 K, hydrogen burning can proceed also via the NeNa cycle. The 22Ne(p,γ)23Na cross section, dominated by a large number of resonances never measured directly, is still affected by large uncertainties. At the Laboratory for Underground Nuclear Astrophysics (LUNA), in the Gran Sasso National Laboratory in Italy, several cross sections have been measured in the past down to the energies of astrophysical interest. An experimental study of the 22Ne(p,γ)23Na reaction is under preparation at LUNA, using a windowless gas target system and two HPGe detectors.
Reference Key
francesca2014epjfirst Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Cavanna Francesca
Journal utilitas mathematica
Year 2014
DOI
10.1051/epjconf/20146607004
URL
Keywords

Citations

No citations found. To add a citation, contact the admin at info@scimatic.org

No comments yet. Be the first to comment on this article.