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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Solar Neutrinos and the Eclipse Effect · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/hep-ph_9908313/</link><description>Collected HN comments and submissions linking this paper.</description><language>en</language><lastBuildDate>Mon, 02 Nov 2026 11:16:22 GMT</lastBuildDate><atom:link href="https://hackerpaper.kaipfister.de/p/hep-ph_9908313/feed.xml" rel="self" type="application/rss+xml" /><item><title>Solar Neutrinos and the Eclipse Effect — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=39954715</link><guid isPermaLink="false">urn:hackerpapers:mention:hep-ph_9908313:39954715</guid><pubDate>Sat, 06 Apr 2024 19:21:39 GMT</pubDate><description>&lt;p&gt;If you prefer to read on arXiv, https://arxiv.org/abs/hep-ph/9908313v2 Abstract: &amp;quot;The solar neutrino counting rate in a real time detector like Super--Kamiokanda, SNO, or Borexino is enhanced due to neutrino oscillations in the Moon during a partial or total solar eclipse. The enhancement is calculated as a function of the neutrino parameters in the case of three flavor mixing. This enhancement, if seen, can further help to determine the neutrino parameters.&amp;quot;&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/hep-ph_9908313/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>hep-ph</category></item></channel></rss>
