Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946
Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the t...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Megna, R. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2013 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media Dordrecht 2013 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 350(2013), 1 vom: 27. Nov., Seite 245-250 |
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| Übergeordnetes Werk: |
volume:350 ; year:2013 ; number:1 ; day:27 ; month:11 ; pages:245-250 |
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| DOI / URN: |
10.1007/s10509-013-1709-6 |
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| 520 | |a Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. | ||
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10.1007/s10509-013-1709-6 doi (DE-627)OLC2066272655 (DE-He213)s10509-013-1709-6-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Megna, R. verfasserin aut Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. Neutrino astrophysics Supernova remnants SNR RX J1713.7-3946 Gamma rays Enthalten in Astrophysics and space science Springer Netherlands, 1968 350(2013), 1 vom: 27. Nov., Seite 245-250 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:350 year:2013 number:1 day:27 month:11 pages:245-250 https://doi.org/10.1007/s10509-013-1709-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 350 2013 1 27 11 245-250 |
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10.1007/s10509-013-1709-6 doi (DE-627)OLC2066272655 (DE-He213)s10509-013-1709-6-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Megna, R. verfasserin aut Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. Neutrino astrophysics Supernova remnants SNR RX J1713.7-3946 Gamma rays Enthalten in Astrophysics and space science Springer Netherlands, 1968 350(2013), 1 vom: 27. Nov., Seite 245-250 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:350 year:2013 number:1 day:27 month:11 pages:245-250 https://doi.org/10.1007/s10509-013-1709-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 350 2013 1 27 11 245-250 |
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10.1007/s10509-013-1709-6 doi (DE-627)OLC2066272655 (DE-He213)s10509-013-1709-6-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Megna, R. verfasserin aut Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. Neutrino astrophysics Supernova remnants SNR RX J1713.7-3946 Gamma rays Enthalten in Astrophysics and space science Springer Netherlands, 1968 350(2013), 1 vom: 27. Nov., Seite 245-250 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:350 year:2013 number:1 day:27 month:11 pages:245-250 https://doi.org/10.1007/s10509-013-1709-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 350 2013 1 27 11 245-250 |
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10.1007/s10509-013-1709-6 doi (DE-627)OLC2066272655 (DE-He213)s10509-013-1709-6-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Megna, R. verfasserin aut Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. Neutrino astrophysics Supernova remnants SNR RX J1713.7-3946 Gamma rays Enthalten in Astrophysics and space science Springer Netherlands, 1968 350(2013), 1 vom: 27. Nov., Seite 245-250 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:350 year:2013 number:1 day:27 month:11 pages:245-250 https://doi.org/10.1007/s10509-013-1709-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 350 2013 1 27 11 245-250 |
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10.1007/s10509-013-1709-6 doi (DE-627)OLC2066272655 (DE-He213)s10509-013-1709-6-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Megna, R. verfasserin aut Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media Dordrecht 2013 Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. Neutrino astrophysics Supernova remnants SNR RX J1713.7-3946 Gamma rays Enthalten in Astrophysics and space science Springer Netherlands, 1968 350(2013), 1 vom: 27. Nov., Seite 245-250 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:350 year:2013 number:1 day:27 month:11 pages:245-250 https://doi.org/10.1007/s10509-013-1709-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 350 2013 1 27 11 245-250 |
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Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946 |
| abstract |
Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. © Springer Science+Business Media Dordrecht 2013 |
| abstractGer |
Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. © Springer Science+Business Media Dordrecht 2013 |
| abstract_unstemmed |
Abstract In this paper we show how to calculate the neutrino flux from a resolved source of high energy gamma-rays, of which have been measured fluxes and spectral indexes of each of the parts in which has been divided for the observations. For the calculation of the neutrino flux need to know the theoretical photon/neutrino ratios and have to consider the oscillation probability of neutrinos. As a numerical example the case of the Supernova Remnant RX J1713.7-3946 observed by H.E.S.S. experiment is presented here. Gamma-rays up to tens of TeV have been observed from RX J1713.7-3946, making this source a possible site of hadronic interactions and thus a source of neutrinos. The H.E.S.S. experiment observed 14 different regions in RX J1713.7-3946, measuring in each one the gamma-ray flux and spectral index. The technique presented in this paper can be applied to other high energy astrophysical sources, point-like or resolved. © Springer Science+Business Media Dordrecht 2013 |
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| container_issue |
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| title_short |
Method to calculate the neutrino flux from a resolved source of high energy gamma-rays: the case of SNR RX J1713.7-3946 |
| url |
https://doi.org/10.1007/s10509-013-1709-6 |
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| doi_str |
10.1007/s10509-013-1709-6 |
| up_date |
2024-07-04T04:07:31.514Z |
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