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Interaction of cosmic background neutrinos with matter of periodic structure
High Energy Physics - Phenomenology · Submitted 30 Jul 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We show that in a coherent scattering process a periodic matter structure designed to match the scale of the mass square difference of neutrinos can enhance the conversion of CBNs from one mass state to another.
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The abstract, sentence by sentence
We study coherent interaction of cosmic background neutrinos(CBNs) with matter of periodic structure. The mixing and small masses of neutrinos discovered in neutrino oscillation experiments indicate that CBNs which have very low energy today should be in mass states and can transform from one mass state to another in interaction with electrons in matter. We show that in a coherent scattering process a periodic matter structure designed to match the scale of the mass square difference of neutrinos can enhance the conversion of CBNs from one mass state to another. Energy of CBNs can be released in this scattering process and momentum transfer from CBNs to electrons in target matter can be obtained.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We study coherent interaction of cosmic background neutrinos(CBNs) with matter of periodic structure. | contribution 0.99 | 0.81 | 0.06 | asserted 0.71 |
| s1 | The mixing and small masses of neutrinos discovered in neutrino oscillation experiments indicate that CBNs which have very low energy today should be in mass states and can transform from one mass state to another in interaction with electrons in matter. | background 1.00 | 0.06 | 0.05 | hedged possibility 0.91 |
| s2 | We show that in a coherent scattering process a periodic matter structure designed to match the scale of the mass square difference of neutrinos can enhance the conversion of CBNs from one mass state to another. | result 0.88 | 0.87 | 0.79 | asserted 1.00 |
| s3 | Energy of CBNs can be released in this scattering process and momentum transfer from CBNs to electrons in target matter can be obtained. | result 0.58 | 0.55 | 0.17 | asserted 0.83 |
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The paper
Original abstract
We study coherent interaction of cosmic background neutrinos(CBNs) with matter of periodic structure. The mixing and small masses of neutrinos discovered in neutrino oscillation experiments indicate that CBNs which have very low energy today should be in mass states and can transform from one mass state to another in interaction with electrons in matter. We show that in a coherent scattering process a periodic matter structure designed to match the scale of the mass square difference of neutrinos can enhance the conversion of CBNs from one mass state to another. Energy of CBNs can be released in this scattering process and momentum transfer from CBNs to electrons in target matter can be obtained.
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How the literature uses it
1 arXiv paper cite this in 2 sentences
Papers citing it · 1 sentence without a confident label
Cites it as background 1 paper
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Among the great science and technology challenges of this century is the development of the experimental capability to detect cosmic background neutrinos [ref] .
Non-Equilibrium Aspects of Relic Neutrinos: From Freeze-out to the Present Day · Key Results From our Study of Neutrino Freeze-out · 0.86
What it cites · 1 sentence without a confident label
Uses data or values from 2 papers
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Recent observation of oscillation of reactor anti-neutrinos in Daya Bay experiment [ref] , confirmed by RENO experiment [ref] , shows that $sin^2 2θ_13≈0.092$.
Observation of electron-antineutrino disappearance at Daya Bay · Introduction · 0.94
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Recent observation of oscillation of reactor anti-neutrinos in Daya Bay experiment [ref] , confirmed by RENO experiment [ref] , shows that $sin^2 2θ_13≈0.092$.
Observation of Reactor Electron Antineutrino Disappearance in the RENO Experiment · Introduction · 0.94
Cites as support 1 paper
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Numerical simulation of clustering of CBNs does not support $n_i$ in galaxy much larger than the average value either [ref] .
Gravitational clustering of relic neutrinos and implications for their detection · Introduction · 0.96
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