- #1
RobertGC
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- TL;DR Summary
- An interplanetary test.
The neutrino has been puzzling since its proposal and its experimental confirmation.
There have been experimental anomalies with it for every experiment designed to test it.
One fact that might be quite key is that measurements of the mass-square of the neutrino has consistently shown it to have a negative mass-square:
Why is the square of the neutrino mass negative?
In arXiv:hep-ph/0009291 this is explained by giving the example of:
m2 = -2.5 +- 3.3eV2.
"The negative value of the neutrino mass-square simply means:"
E2/c2 -p2 = m2c2 < 0,
https://physics.stackexchange.com/questions/578556/why-is-the-square-of-the-neutrino-mass-negative
This has led to speculation the neutrino may be a tachyon. Another unusual fact about it is that its cross section gets larger at higher energies and smaller at lower energies. And with a tachyon, in contrast to a bradyon, higher energy means it is going slower, and lower energies means it going faster. This would explain why it would be harder to interact with at the lower energies.
However, with the unfortunate mistake at the OPERA experiment where is was offered a superluminal neutrino to explain an experimental anomaly, any such claim needs to have overwhelming support to confirm it.
I was thinking of having the neutrino travel through the Earth and be detected on the other side. However, even at the speed of light the travel time would be quite short and given the difficulty of detecting the neutrino it would be difficult to get the timing accurate enough to make sure the detection was above background.
Then I wanted a longer travel time. Could we have an accelerator generated neutrino pulse be aimed at the Moon or Mars or Venus, and look for the neutrinos scattered back to be captured here on Earth? Because of the low cross-section it would have to be an extremely dense beam to have enough particles to bounce back to be detectable.
Robert Clark
There have been experimental anomalies with it for every experiment designed to test it.
One fact that might be quite key is that measurements of the mass-square of the neutrino has consistently shown it to have a negative mass-square:
Why is the square of the neutrino mass negative?
In arXiv:hep-ph/0009291 this is explained by giving the example of:
m2 = -2.5 +- 3.3eV2.
"The negative value of the neutrino mass-square simply means:"
E2/c2 -p2 = m2c2 < 0,
https://physics.stackexchange.com/questions/578556/why-is-the-square-of-the-neutrino-mass-negative
This has led to speculation the neutrino may be a tachyon. Another unusual fact about it is that its cross section gets larger at higher energies and smaller at lower energies. And with a tachyon, in contrast to a bradyon, higher energy means it is going slower, and lower energies means it going faster. This would explain why it would be harder to interact with at the lower energies.
However, with the unfortunate mistake at the OPERA experiment where is was offered a superluminal neutrino to explain an experimental anomaly, any such claim needs to have overwhelming support to confirm it.
I was thinking of having the neutrino travel through the Earth and be detected on the other side. However, even at the speed of light the travel time would be quite short and given the difficulty of detecting the neutrino it would be difficult to get the timing accurate enough to make sure the detection was above background.
Then I wanted a longer travel time. Could we have an accelerator generated neutrino pulse be aimed at the Moon or Mars or Venus, and look for the neutrinos scattered back to be captured here on Earth? Because of the low cross-section it would have to be an extremely dense beam to have enough particles to bounce back to be detectable.
Robert Clark