Pulse of neutrinos, E m, hits plasma->charge seperation?

In summary, when a large pulse of high-energy neutrinos hits plasma, it can lead to charge separation in the plasma. This is supported by a fluid approach and dynamical techniques in plasma physics, which show that the neutrino effective charge depends on the direction of propagation relative to the external magnetic field. This theory is applicable for magnetic fields below the Landau-Schwinger critical value and has been compared to results from quantum field theory. In an early universe model, there is evidence of neutrino fluid separation.
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Pulse of neutrinos, E>>m, hits plasma-->charge seperation?

When a large pulse of neutrinos, each with an energy much greater than the electron rest mass energy, hits some plasma does this give rise to charge separation for the plasma? Could one make a simple argument why this is true or false?

Thanks for any help.
 
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The answer seems to be "yes", but a simple argument? I found a couple of papers that use a fluid approach, but this is beyond my pay grade. http://www.springerlink.com/content/y721025uj77krm77/

http://pop.aip.org/phpaen/v11/i4/p1352_s1?isAuthorized=no
aip said:
Using dynamical techniques of the plasma physics, the neutrino (antineutrino) effective charge in a magnetized dense electron–positron plasma is determined here. It shown that its value, which is determined by the plasma collective processes, depends mainly on the propagation direction of plasma waves and neutrinos against the external magnetic field direction. The direction dependence of the effective charge occurs due to the fact that the magnetic field breaks the plasma isotropy. The present theory gives a unified picture of the problem which is valid for an external magnetic field below the Landau–Schwinger critical value. Comparison with some of the results from the quantum field theory has been made. © 2004 American Institute of Physics.

Here is the separation of the neutrino fluid in an early universe model: http://arxiv.org/PS_cache/astro-ph/pdf/0211/0211087v2.pdf
 
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1. What is the "Pulse of neutrinos" in relation to charge separation?

The "Pulse of neutrinos" refers to the emission of neutrinos from a source, such as a supernova or a high-energy particle collision. When these neutrinos interact with plasma, they can cause charge separation, which is the separation of positively and negatively charged particles.

2. How does the energy (E m) of neutrinos affect charge separation?

The energy of neutrinos, denoted as E m, is a crucial factor in determining the extent of charge separation. Higher energy neutrinos have a greater probability of interacting with plasma and causing charge separation.

3. Can neutrinos from the sun also lead to charge separation?

Yes, neutrinos from the sun can also induce charge separation in plasma. However, the effect is relatively small compared to the impact of high-energy neutrinos from other sources.

4. What is the significance of charge separation caused by neutrinos?

Charge separation caused by neutrinos has significant implications for astrophysics and particle physics. It can provide insights into the properties of neutrinos and other fundamental particles, as well as the behavior of plasma in extreme environments.

5. How do scientists detect the effects of neutrinos on charge separation?

Scientists use various experimental techniques, such as particle detectors and telescopes, to observe the effects of neutrinos on charge separation. These techniques involve measuring the characteristics of particles and radiation produced by the interaction between neutrinos and plasma.

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