Neutrinos-Antineutrinos in the universe

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SUMMARY

This discussion centers on the production and detection of neutrinos and antineutrinos in the universe. It confirms that Earth produces antineutrinos primarily through the decay of radioactive nuclei, while solar neutrinos are predominantly detected from the reaction p + p → d + e+ + ν. The conversation also highlights that neutrinos from the Big Bang, known as relic neutrinos, are too low in energy for current detectors to identify. Additionally, it notes that the detection capabilities of neutrino detectors depend on the specific methods employed.

PREREQUISITES
  • Understanding of beta decay processes (beta minus and beta plus)
  • Familiarity with neutrino detection methods and technologies
  • Knowledge of solar neutrino production mechanisms
  • Concept of relic neutrinos and their significance in cosmology
NEXT STEPS
  • Research the mechanisms of beta decay and its implications for particle physics
  • Explore different neutrino detection technologies, such as liquid scintillator detectors
  • Study the role of solar neutrinos in astrophysics and their detection challenges
  • Investigate the properties and significance of relic neutrinos in the context of the Big Bang theory
USEFUL FOR

Physics students, astrophysicists, and researchers interested in particle physics and cosmology will benefit from this discussion.

omiros
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Hello everybody, I am a first year physics student and I have a question about neutrinos and antineutrinos.

In a beta minus decay we will get an antineutrino, so I assume that Earth 'produces' more antineutrinos. Does it?

However from a beta plus we get neutrinos and positrons. So does that mean that we had more protons in the beginning that started becoming neutrons? Do the neutrinos that we find now, were mostly created after the big bang?

Do neutrino detectors detect antineutrinos too?

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Does that mean that the number of the electrons in stars etc is getting smaller, cause of positrons? (random)
 
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omiros said:
Do the neutrinos that we find now, were mostly created after the big bang?
Most of the neutrinos we detect are solar neutrinos coming from p + P → d + e+ + ν. Neutrinos from the big bang are known as relic neutrinos and are too low energy to be detectable.
 
A few neutrinos from supernovae and other cosmic events can be detected, together with atmospheric neutrinos (produced by cosmic rays hitting our atmosphere) and nuclear reactor antineutrinos (beta- decays, so just antineutrinos).

Similar to the cosmic microwave background, primordial neutrinos (= from the big bang) lost energy during the expansion of space, so current detectors are not sensitive enough to see them.
 
omiros said:
In a beta minus decay we will get an antineutrino, so I assume that Earth 'produces' more antineutrinos. Does it?
The Earth does produce antineutrinos; they are from the decay of radioactive nuclei (http://www.physicstoday.org/resource/1/phtoad/v64/i9/p14_s1). I am sure the Earth produces neutrinos as well, but I am not aware of a similar measurement for them.

omiros said:
Do neutrino detectors detect antineutrinos too?
It depends on the method they are using for detection (Wikipedia- Neutrino detector).
 
Hi Bill:

Bill_K said:
Most of the neutrinos we detect are solar neutrinos coming from p + P → d + e+ + ν.

Is the "P" here a typo where "p" was intended? If not, whar does "P" mean?
 
omiros said:
Do neutrino detectors detect antineutrinos too?

It depends on what and how you want to measure in neutrino detectors and what detectors you are using.
 
Buzz Bloom said:
Is the "P" here a typo where "p" was intended? If not, whar does "P" mean?
It was a two year old typo (and as the thread is very old, I'll close it, feel free to discuss in other threads or open a new one).

Actually, it was not correct either because neutrinos from that particular reaction are very low-energetic and hard to detect, that was achieved for the first time in 2014.
 

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