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What are the details of how neutrons are produced as a result of cosmic ray particles hitting our planet's atmosphere?

For instance, what is the pathway that creates the highest number of neutrons from cosmic ray particles?

The article "Single event upset" states:

An SEU happens due to cosmic particles which collide with atoms in the atmosphere, creating cascades or showers of neutrons and protons. At deep sub-micrometre geometries, this affects semiconductor devices at sea level.

But it does not describe the mechanism.

The Wikipedia article on the neutron states something similar:

Cosmic radiation interacting with the Earth's atmosphere continuously generates neutrons that can be detected at the surface.

What are the processes, in detail?

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How about some more specific tags? Like particle-radiation, hadron, baryon, neutron? –  Peter Mortensen Nov 10 '10 at 16:24
    
my guess would be that the neutrons are produced in the core of sun itself and not from any terrestrial reactions.. –  Vineet Menon Aug 17 '11 at 10:48
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@Vineet Menon: Neutrons produced in the core of the sun would be scattered many times, so they would end up decaying before they could escape. –  Ben Crowell Aug 17 '11 at 20:27
    
@Ben - Again, I remember solving a problem in Renik Halliday(I guess you know about that book, John Wiley), where you hav to solve the time(with earth as refernce) in which the neutron decays. Remember: the speed is relativistic at least 0.9c. –  Vineet Menon Aug 19 '11 at 4:24
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3 Answers

OK, here is something concrete and quantitative, "Guidelines for predicting single-event upsets in neutron environments":

Neutrons in the atmosphere result from cosmic-ray spallation interactions with nitrogen and oxygen nuclei. A typical reaction is a 1 GeV proton fragmenting a nitrogen necleus into lighter charged particles and simultaneoously emitting a couple of neutrons.

Cosmic ray spallation.


From "Cosmic ray induced ionization in the atmosphere: Full modeling and practical applications":

... full numerical model, which computes the cosmic ray induced ionization in the entire atmosphere, from the ground level up to the stratosphere, all over the Globe. The model computations reproduce actual measurements of the atmospheric ionization in the full range of parameters, from equatorial to polar regions and from the solar minimum to solar maximum. A detailed numerical recipe is given in section 2.5 together with the precalculated tabulated ionization yield function (Tables 1 and 2). Using this method, one can easily compute the CRII for any desired location and conditions, instead of using, e.g., a neutron monitor count rate as a proxy.

It does not describe it, but the CORSIKA (Cosmic Ray Simulations for Kascade) simulation tool is used.


Google-fu: quantitative neutrons cosmic rays atmosphere

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And, though the rate goes down precipitously both the spallation fraction and the mean number of neutrons go up when you have a deep underground detector. And the mean energy is higher. The result is that cosmic ray events in low background detectors are quite something. –  dmckee Jan 8 '11 at 0:12
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Between what I've learned about cosmic rays and what I can find online (example: http://www.fisica.unlp.edu.ar/~veiga/experiments.html), it seems that the primary source of neutrons in cosmic ray showers is the disintegration of the atomic nuclei that are struck by the cosmic ray or its decay products.

As you may know, cosmic rays enter the atmosphere with enormous amounts of energy, so when one strikes a nucleus, it's going to disrupt the nuclear structure. The net effect could be anything from just kicking out a single particle to shattering the entire nucleus into several pieces, as in nuclear fission - it depends on the energy of the cosmic ray and the type of atom/molecule it hits. If the cosmic ray is especially high-energy, the products of the reaction will also have high energies, and they can interact with other nuclei, repeating the same process. A wide variety of particles are produced in these interactions, including neutrons, pions, kaons, and other hadrons.

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Spallation of air atoms' nuclei is the easiest way - there are neutrons kicked out of the nucleus directly or emmited by radioactive elements, which were activated by cosmic rays.

Also neutrons can be produced upon hadronization of quark-gluon-plasma or from electron capturing in air nuclei.

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