Thermal Neutrinos: Detecting Ancient Particles in the Universe?

In summary, the conversation discusses the possibility of detecting neutrinos emitted in the distant and early universe, their thermal nature, and their interaction with matter. PTOLEMY is a planned measurement to study the cosmic neutrino background, which is believed to be thermal due to the effects of expansion. However, the non-zero masses of neutrinos gradually shift their spectrum away from a thermal spectrum.
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Cato
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Would neutrinos emitted in the distant and early universe be slowed enough to become thermal neutrinos? Could these be detected?
 
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The cosmic neutrino background should be thermal. PTOLEMY is a plan to measure it.

Neutrinos emitted by nuclear processes after the big bang are not thermal, even if they become slow in the very distant future their energy spectrum will look different.
 
  • #3
mfb said:
The cosmic neutrino background should be thermal. PTOLEMY is a plan to measure it.

Neutrinos emitted by nuclear processes after the big bang are not thermal, even if they become slow in the very distant future their energy spectrum will look different.

Do the cosmic background neutrinos remain in thermal equilibrium by interacting with matter? Or are they thermal simply because of the effects of expansion?
 
  • #4
Cato said:
Do the cosmic background neutrinos remain in thermal equilibrium by interacting with matter? Or are they thermal simply because of the effects of expansion?

The latter.

Before decoupling, neutrinos were in thermal equilibrium with the "cosmic soup". It can be shown that after decoupling, expansion of the universe redshifts a thermal spectrum for radiation into a thermal spectrum. Weinberg in his book "Cosmology" demonstrates his on pages 101-102. Weinberg

Thus the photon density has been given a black-body form even after hye photons went out of equilibrium with matter, but with a redshifted temperature.

The above applies to massless neutrinos, which is a good approximation for some of the history of the universe. Their non-zero masses, however, gradually shift their spectrum away from a thermal spectrum. From "Relativistic Cosmology" by Ellis, Maartens, and MacCallum page 304:

The most massive neutrinos become non-relativistic well after radiation matter inequality. We can estimate the non-relativistic redshift by setting the mean energy per neutrino equal to the mass.
 
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Terrific. Thanks very much.
 

1. What are thermal neutrinos?

Thermal neutrinos are a type of neutrino that are created through thermal processes, meaning they are produced at high temperatures. They are often associated with processes such as nuclear fusion or supernova explosions.

2. How are thermal neutrinos different from other types of neutrinos?

Thermal neutrinos are different from other types of neutrinos because they are created at much higher temperatures. This means they have higher energies and can travel longer distances before interacting with matter.

3. Why is it important to study thermal neutrinos?

Studying thermal neutrinos can provide valuable insights into high-energy processes, such as the formation of stars and the evolution of the universe. They can also help us understand the properties of neutrinos, which are still poorly understood particles.

4. How do scientists detect thermal neutrinos?

Scientists use large underground detectors, such as the Super-Kamiokande detector in Japan, to detect thermal neutrinos. These detectors are filled with a large amount of water or other liquid and are sensitive to the tiny flashes of light that are produced when a neutrino interacts with the detector material.

5. Do thermal neutrinos have any practical applications?

While thermal neutrinos do not have any practical applications at the moment, studying them could lead to advancements in technologies such as nuclear reactors and medical imaging. Additionally, understanding the properties of neutrinos could have implications for our understanding of the fundamental laws of physics.

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