Properties of nuetrinos in space

In summary, the conversation discusses questions about the energy and density of neutrinos, specifically those ejected from the sun and those present in deep space. It is mentioned that the gamma for a 1 GeV neutrino would be strongly dependent on its rest mass, which is currently unknown. The conversation also includes links to sources discussing the estimated density of neutrinos in the universe. Finally, it is noted that the gamma for a neutrino can only be computed if its mass is known.
  • #1
Albertgauss
Gold Member
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Just a couple of numbers I'm having trouble finding.

Does anyone know what a typical energy for a nuetrino ejected from the sun is?

Any number on a guess-timate of what the density of nuetrinos is in deep space?

Also, same two questions for electron nuetrinos and Tau nuetrinos.

A 1 Gev Nuetrino, would the gamma for this nuetrino be 4.5(10^8)?
 
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  • #2
Quick reply on the last question. The gamma would be strongly dependent on neutrino rest mass, which is unknown. The gamma would certainly be very large and of the general order you propose.
 
  • #3
Hi! For what concerns the first question, see

http://www.sns.ias.edu/~jnb/SNviewgraphs/snviewgraphs.html

figure 2.

For what concerns the secon question

http://lappweb.in2p3.fr/neutrinos/anunivers.html

"The theory estimated also the neutrino density in the universe: about 110 per cm3, for each neutrino family, that means 330 neutrinos per cm3 as a whole"

For what concerns the question on the gamma, one should know the masses of the neutrinos; it is quite accepted that they are massive, but, as far as I know, there is a lot of uncertainty about their value; so you cannot compute the gamma; notice that if you know the mass m then you can simply solve computing gamma=E/m.

Francesco

PS: Sorry PAllen; I have sent the post short after you..
 

What are neutrinos and what are their properties?

Neutrinos are subatomic particles that have no charge and a very small mass. They are one of the fundamental particles in the Standard Model of particle physics. Neutrinos have three flavors: electron, muon, and tau. They also have very weak interactions with other particles, making them difficult to detect.

How do neutrinos behave in space?

In space, neutrinos travel at nearly the speed of light and can pass through most matter without interacting. However, they can be affected by strong gravitational fields and magnetic fields. They are also affected by the structure of the universe, such as the density of matter in the universe.

What are the sources of neutrinos in space?

Neutrinos can be produced in a variety of astrophysical processes, such as nuclear reactions in stars, supernovae explosions, and black holes. They can also be produced in high-energy collisions of cosmic rays with particles in space.

How are neutrinos detected in space?

Neutrinos are detected using large, specialized instruments such as neutrino telescopes. These instruments use different detection methods, including measuring the faint flashes of light produced when neutrinos interact with matter, or detecting the charged particles produced when neutrinos collide with other particles.

What can studying neutrinos in space tell us about the universe?

Studying neutrinos in space can provide valuable information about the structure and evolution of the universe. Neutrinos can also help us understand the processes that occur in extreme environments, such as inside stars and black holes. Additionally, studying neutrinos can help us better understand the fundamental laws of physics and potentially uncover new physics beyond the Standard Model.

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