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Estimation of the neutrino flux and resulting constraints on hadronic emission models for Cyg X-3 using AGILE data
High Energy Astrophysical Phenomena · Submitted 6 Dec 2012
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Using the correlation of AGILE data on the flaring episodes in 2009 June and July to the hypersoft X-ray state we calculate that the upper limits on the neutrino flux given by IceCube are starting to constrain the hadronic models, which have been introduced to interpret the high-energy emission detected by AGILE.
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The abstract, sentence by sentence
In this work we give an estimate of the neutrino flux that can be expected from the microquasar Cyg X-3. We calculate the muon neutrino flux expected here on Earth as well as the corresponding number of neutrino events in the IceCube telescope based on the so-called hypersoft X-ray state of Cyg~X-3. If the average emission from Cyg~X-3 over a period of 5 yr were as high as during the used X-ray state, a total of 0.8 events should be observed by the full IceCube telescope. We also show that this conclusion holds by a factor of a few when we consider the other measured X-ray states. Using the correlation of AGILE data on the flaring episodes in 2009 June and July to the hypersoft X-ray state we calculate that the upper limits on the neutrino flux given by IceCube are starting to constrain the hadronic models, which have been introduced to interpret the high-energy emission detected by AGILE.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | In this work we give an estimate of the neutrino flux that can be expected from the microquasar Cyg X-3. | contribution 1.00 | 0.92 | 0.06 | asserted 0.91 |
| s1 | We calculate the muon neutrino flux expected here on Earth as well as the corresponding number of neutrino events in the IceCube telescope based on the so-called hypersoft X-ray state of Cyg~X-3. | contribution 0.56 | 0.93 | 0.08 | asserted 1.00 |
| s2 | If the average emission from Cyg~X-3 over a period of 5 yr were as high as during the used X-ray state, a total of 0.8 events should be observed by the full IceCube telescope. | result 1.00 | 0.84 | 0.22 | hedged possibility 0.54 |
| s3 | We also show that this conclusion holds by a factor of a few when we consider the other measured X-ray states. | result 0.95 | 0.88 | 0.10 | asserted 1.00 |
| s4 | Using the correlation of AGILE data on the flaring episodes in 2009 June and July to the hypersoft X-ray state we calculate that the upper limits on the neutrino flux given by IceCube are starting to constrain the hadronic models, which have been introduced to interpret the high-energy emission detected by AGILE. | interpretation 0.76 | 0.91 | 0.70 | asserted 0.95 |
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Original abstract
In this work we give an estimate of the neutrino flux that can be expected from the microquasar Cyg X-3. We calculate the muon neutrino flux expected here on Earth as well as the corresponding number of neutrino events in the IceCube telescope based on the so-called hypersoft X-ray state of Cyg~X-3. If the average emission from Cyg~X-3 over a period of 5 yr were as high as during the used X-ray state, a total of 0.8 events should be observed by the full IceCube telescope. We also show that this conclusion holds by a factor of a few when we consider the other measured X-ray states. Using the correlation of AGILE data on the flaring episodes in 2009 June and July to the hypersoft X-ray state we calculate that the upper limits on the neutrino flux given by IceCube are starting to constrain the hadronic models, which have been introduced to interpret the high-energy emission detected by AGILE.
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We show that in the $pγ$ processes there is a correlation between the generated EM (electrons and photons) and neutrino fluxes [ref] .
Fermi Limit on the Neutrino Flux from Gamma-ray Bursts · Conclusion and discussion · 0.96
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