Winter, Walter, 1975-....
![Sudoc [ABES], France](https://viaf.org/viaf/images/flags/SUDOC.png "Sudoc [ABES], France")
Walter Winter
VIAF ID: 18279269 (Personal)
Permalink: http://viaf.org/viaf/18279269
Preferred Forms
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100 0 _
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Walter Winter
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100 1 _
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Winter, Walter
‡d
1975-
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100 1 _
‡a
Winter, Walter
‡d
1975-
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100 1 _
‡a
Winter, Walter,
‡d
1975-....
4xx's: Alternate Name Forms(3)
Works
| Title | Sources |
|---|---|
| Blazar origin of the UHECRs and perspectives for the detection of astrophysical source neutrinos at EeV energies |
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| concordance scenario for the observation of a neutrino from the Tidal Disruption Event AT2019dsg |
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| Cosmic ray and neutrino emission from Gamma-Ray Bursts with a nuclear cascade |
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| Describing the observed cosmic neutrinos by interactions of nuclei with matter |
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| Expected neutrino fluence from short gamma-ray burst 170817A and off-axis angle constraints |
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| Improved photomeson model for interactions of cosmic ray nuclei |
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| Leptohadronic blazar models applied to the 2014-15 flare of TXS 0506+056 |
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| multi-component model for the observed astrophysical neutrinos |
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| Multi-messenger light curves from gamma-ray bursts in the internal shock model |
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| Multi-wavelength radiation models for low-luminosity GRBs, and the implications for UHECRs |
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| Neutrino oscillations et tomographie terrestre avec KM3NeT-ORCA. |
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| Neutrinos and ultra-high-energy cosmic-ray nuclei from blazars |
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| new view on auger data cosmogenic neutrinos in light of different nuclear disintegration and air-shower models |
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| Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays |
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| Perspectives for tests of neutrino mass generation at the GeV scale: experimental reach versus theoretical predictions |
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| Phänomenologische Konsequenzen nichtverschwindender Neutrinomassen an Beispielen zukünftiger Long-Baseline-Experimente |
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| Systematic parameter space study for the UHECR origin from GRBs in models with multiple internal shocks |
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| Tidally disrupted stars as possible origin of both cosmic rays and neutrinos at the highest energies |
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