Level of unseen elastic scatterings

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In summary, the conversation discusses the frequency of visible matter particles undergoing elastic scattering with unseen particles, such as neutrinos, antineutrinos, and dark matter particles. The background of elastic scattering events is also mentioned, with the possibility of distant galaxies being blurred if the background is large. The conversation also touches on the impact of elastic scattering on vision, and the potential observability of low energy but penetrating radiation from cosmic ray neutrinos or dark matter particles.
  • #1
snorkack
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How often are visible matter particles seen to undergo elastic scattering with particles that remain otherwise unseen?
Known particles that may cause such scattering include neutrinos and antineutrinos (three flavours each) which are also seen in inelastic destruction and formation processes. Also, since dark matter is thought to not fit neutrino properties, that also means unknown number of different dark matter particles are eligible to cause elastic scattering of visible particles.

So, how well is background of elastic scattering events measured?
 
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  • #2
If it were large distant galaxies would be blurred.
 
  • #3
Vanadium 50 said:
If it were large distant galaxies would be blurred.
Why? No more so than darkness of a closed room.
 
  • #4
Scattered light changes direction. If you have a large angle scvatter you can no longer associate it with the source (e.g. the blue sky) and if it's a small angle scatter it's no longer coming from the exact same direction so it blurs.
 
  • #5
A muon undergoing elastic scattering off an electron in retina would cause vision the same as a photon being destroyed by interaction with an electron in retina does.
Likewise, a neutrino undergoing elastic scattering off an electron in retina would cause vision. And so would a dark matter particle undergoing elastic scattering of an electron in retina.
 
  • #6
And if the universe were a retina, this would matter.

This is silly. I'm out of here.
 
  • #7
It matters in terms of observability.
Asking the question this way: do particle observers/astronomers observe any background of low energy but penetrating radiation, in places otherwise sheltered from more visible radiations like visible light or muons? Such as cosmic ray neutrinos, or dark matter particles?
 

Related to Level of unseen elastic scatterings

1. What is the level of unseen elastic scatterings?

The level of unseen elastic scatterings refers to the amount of energy that is scattered by particles during a collision, but is not detected or measured by the experimental apparatus.

2. Why is the level of unseen elastic scatterings important?

Understanding the level of unseen elastic scatterings is important in particle physics experiments because it can affect the accuracy and precision of measurements. It is also important for determining the properties of particles and their interactions.

3. How is the level of unseen elastic scatterings calculated?

The level of unseen elastic scatterings is typically calculated by comparing the total energy of the particles before and after a collision. The difference in energy is attributed to unseen elastic scatterings.

4. Can the level of unseen elastic scatterings be reduced?

Yes, there are several techniques that can be used to reduce the level of unseen elastic scatterings, such as improving the experimental apparatus, increasing the energy of the particles, or using different detection methods.

5. How does the level of unseen elastic scatterings impact the interpretation of experimental data?

The level of unseen elastic scatterings can introduce uncertainties in experimental data, which can affect the interpretation of results. It is important for scientists to consider and account for these unseen scatterings when analyzing data and drawing conclusions.

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