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Searching for High Energy Neutrino counterpart signals; The case of the Fermi Bubbles signal and of Dark Matter annihilation in the inner Galaxy
High Energy Astrophysical Phenomena · Submitted 7 Jun 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We find that some of these models will be probed by the IceCube DeepCore detector.
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The abstract, sentence by sentence
The recent uncovering of the \textit{Fermi} Bubbles/haze in the \textit{Fermi} gamma-ray data has generated theoretical work to explain such a signal of hard $\gamma$-rays in combination with the \textit{WMAP} haze signal. Many of these theoretical models can have distinctively different implications with regards to the production of high energy neutrinos. We discuss the neutrino signals from different models proposed for the explanation of the \textit{Fermi} Bubbles/haze, more explicitly, from Dark Matter annihilation in the galactic halo with conditions of preferential CR diffusion, from recent AGN jet activity, from periodic diffusive shock acceleration, from stochastic 2nd order Fermi acceleration and from long time-scale star formation in the galactic center in combination with strong galactic winds. We find that some of these models will be probed by the IceCube DeepCore detector. Moreover, with a km$^3$ telescope located at the north hemisphere, we will be able to discriminate between the hadronic, leptonic and the DM models. Additionally using the reconstructed neutrino spectra we will probe annihilation of TeV scale dark matter towards the galactic center.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The recent uncovering of the \textit{Fermi} Bubbles/haze in the \textit{Fermi} gamma-ray data has generated theoretical work to explain such a signal of hard $\gamma$-rays in combination with the \textit{WMAP} haze signal. | background 1.00 | 0.04 | 0.02 | asserted 1.00 |
| s1 | Many of these theoretical models can have distinctively different implications with regards to the production of high energy neutrinos. | background 0.88 | 0.06 | 0.03 | asserted 0.53 |
| s2 | We discuss the neutrino signals from different models proposed for the explanation of the \textit{Fermi} Bubbles/haze, more explicitly, from Dark Matter annihilation in the galactic halo with conditions of preferential CR diffusion, from recent AGN jet activity, from periodic diffusive shock acceleration, from stochastic 2nd order Fermi acceleration and from long time-scale star formation in the galactic center in combination with strong galactic winds. | contribution 0.94 | 0.31 | 0.05 | asserted 0.93 |
| s3 | We find that some of these models will be probed by the IceCube DeepCore detector. | result 0.85 | 0.88 | 0.23 | asserted 0.63 |
| s4 | Moreover, with a km$^3$ telescope located at the north hemisphere, we will be able to discriminate between the hadronic, leptonic and the DM models. | result 0.37 | 0.16 | 0.20 | hedged possibility 0.67 |
| s5 | Additionally using the reconstructed neutrino spectra we will probe annihilation of TeV scale dark matter towards the galactic center. | result 0.34 | 0.21 | 0.18 | asserted 0.53 |
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Original abstract
The recent uncovering of the \textit{Fermi} Bubbles/haze in the \textit{Fermi} gamma-ray data has generated theoretical work to explain such a signal of hard $\gamma$-rays in combination with the \textit{WMAP} haze signal. Many of these theoretical models can have distinctively different implications with regards to the production of high energy neutrinos. We discuss the neutrino signals from different models proposed for the explanation of the \textit{Fermi} Bubbles/haze, more explicitly, from Dark Matter annihilation in the galactic halo with conditions of preferential CR diffusion, from recent AGN jet activity, from periodic diffusive shock acceleration, from stochastic 2nd order Fermi acceleration and from long time-scale star formation in the galactic center in combination with strong galactic winds. We find that some of these models will be probed by the IceCube DeepCore detector. Moreover, with a km$^3$ telescope located at the north hemisphere, we will be able to discriminate between the hadronic, leptonic and the DM models. Additionally using the reconstructed neutrino spectra we will probe annihilation of TeV scale dark matter towards the galactic center.
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References
How the literature uses it
5 arXiv papers cite this in 5 sentences
Papers citing it · 4 sentences without a confident label
Cites it as background 1 paper
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This has led to a flurry of activity in both the particle physics [ref] and astrophysics [ref] communities, and competing interpretations of the source of the excess abound.
Wavelet-Based Techniques for the Gamma-Ray Sky · The Inner Galaxy · 0.89
What it cites · 1 sentence without a confident label
Uses data or values from 1 paper
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The HI ISM gas has also a scale hight that towards the GC is $≃0.15$ kpc and increasing up to 0.3 kpc at the solar ring [ref] ; while the H2 gas a scale hight of 0.1 kpc [ref] .
Three-Dimensional Distribution of the ISM in the Milky Way Galaxy: II. The Molecular Gas Disk · eXciting Dark Matter annihilation, connecting to the Fermi haze and the WMAP haze · 0.93
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