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Mar 6, 2020 at 11:50 vote accept Ritesh Singh
Feb 28, 2020 at 16:42 history edited user59991 CC BY-SA 4.0
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Feb 27, 2020 at 14:40 comment added Richter65 Thank you @Asteroids! @TLW, to follow up on what PLL said (which was correct), there are various ways of experimentally measuring the fraction of neutrinos that get detected when they pass through a detector. The modern and most direct way is to create a neutrino beam of known intensity using a particle accelerator, and measuring the fraction of the beam that gets detected. A summary of these measurements can be found in the "bible of particle physics", the PDG: pdg.lbl.gov/2019/reviews/rpp2018-rev-nu-cross-sections.pdf
Feb 27, 2020 at 1:07 comment added Asteroids With Wings This is a great answer that abides by scientific principles rather than being sprinkled through with phrases like "we know that...".
Feb 26, 2020 at 8:51 comment added PLL @TLW: Just from the detected neutrino flux alone, you can’t tell. But if theoretical calculation A, about the sun’s output, says we should expect 1 billion neutrinos/sec, theoretical calculation B, about the detector, says we should expect to detect 10 per million of these, and we do indeed detect 10,000/s, then it’s less likely that both the theoretical calculations are wrong in ways that cancel out perfectly — especially when there are also other theoretical calculations C, D, and E that also agree with this, and experiments X, Y, Z that test other predictions of the theory.
Feb 26, 2020 at 3:04 comment added TLW To play devil's advocate for a moment: how can you experimentally tell the difference between, say, 1 billion neutrinos / second of which 10/million are detected, and 10 billion neutrinos / second of which 1/million are detected?
Feb 25, 2020 at 14:55 history edited Richter65 CC BY-SA 4.0
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Feb 25, 2020 at 3:00 history edited Richter65 CC BY-SA 4.0
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Feb 24, 2020 at 21:51 history answered Richter65 CC BY-SA 4.0