Parameters of neutrino interactions in targets?

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Discussion Overview

The discussion revolves around the parameters influencing neutrino interactions with various materials, focusing on the relationship between material density, atomic number, and interaction cross sections. Participants explore theoretical and practical aspects of neutrino detection and interaction rates in different contexts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant suggests that the number of neutrino interactions is proportional to the amount of material traversed, questioning whether this relationship is linear with respect to density.
  • Another participant notes that for plausible detector sizes, the neutrino beam remains strong enough that the event rate correlates with the amount of sensitive material, emphasizing the importance of the interaction cross section for different atoms.
  • A participant clarifies the distinction between "number density" of targets and "heavier" targets, introducing the concept of cross section and its role in calculating interactions.
  • It is mentioned that for thin targets, the number of interactions can be described by a specific mathematical relationship, while for thick targets, an exponential absorption law must be applied.
  • One participant reflects on historical perspectives from their graduate studies, indicating that interactions were often considered in terms of individual protons and neutrons rather than entire nuclei, and notes the differing approaches for high and low energy neutrinos.

Areas of Agreement / Disagreement

Participants express varying views on the relationship between density, atomic number, and interaction rates, indicating that multiple competing models and interpretations exist without a clear consensus.

Contextual Notes

There are unresolved aspects regarding the dependence of interaction cross sections on neutrino energy and the state of the nucleus, as well as the implications of using different models for high versus low energy neutrinos.

morenopo2012
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TL;DR
I am trying to understand which parameters are fundamental for the interaction between neutrinos in a given target.
The interaction of neutrinos should be proportional to the amount of material that it goes through. If i want to calculate the number of interactions that i could expect when a neutrino beam go through different materials, the first thing that comes to mind is the nuclei of the targets, as the target gets denser, more interactions could be expected, but, this relation is lineal?

I mean, i expect just dependence in the amount of mass, but a read some informal comments about how there is others factors as dependence of the atomic number.

Does anyone have information about that?
 
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For plausible detector sizes the neutrino beam doesn't get weaker within the range of the detector, so the event rate will be proportional to the amount of sensitive material in the detector.
To find the event rate you need the interaction cross section for each type of atom in your detector. It depends on the type of neutrino and the neutrino energy, too, and there is no simple relationship.
 
morenopo2012 said:
as the target gets denser, more interactions could be expected, but, this relation is lineal?
By "denser", do you mean more targets (nuclei) per unit volume (larger "number density" of targets), or do you mean "heavier" targets (larger atomic number and/or atomic mass)?

Are you acquainted with the concept of "cross section?" In general, for a "thin" target, such that you can neglect the decrease in intensity of the beam as it progresses through the target, the number of interactions is $$dN = -Nn \sigma \, dx$$ where ##N## is the number of incoming particles (neutrinos in your case), ##n## is the number of targets (nuclei) per unit volume, ##dx## is the thickness of the collection of targets, and ##\sigma## is the "cross section" of a single target, which encapsulates the details of the interaction of a single incoming particle with a single target.

For a "thick" collection of targets, you have to integrate to account for the decrease in intensity of the beam inside the target, which leads to an "exponential absorption law" $$N = N_0 e^{-n \sigma x}$$ Here I use "target" to mean a single nucleus. In this case the effects of "heavier" targets (nuciel) would be encoded in the cross section ##\sigma##.

However, when I was an grad student in experimental neutrino physics about 40 years ago, IIRC we thought in terms of the cross section for neutrino interactions on individual protons and neutrons. That is, we thought in terms of a collection of protons and neutrons, not a collection of nuclei. And we would have separate ##n## and ##\sigma## for protons and neutrons.
 
jtbell said:
However, when I was an grad student in experimental neutrino physics about 40 years ago, IIRC we thought in terms of the cross section for neutrino interactions on individual protons and neutrons. That is, we thought in terms of a collection of protons and neutrons, not a collection of nuclei.
That works well at high energies (with accelerators as sources, for example) but doesn't work well at low energies (e.g. neutrinos from the Sun or nuclear reactors) where you have to consider the state of the nucleus.
For neutrinos every detector is a thin detector.
 

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