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04/07/2018 09:30
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Alexis Coleiro (APC / Université Paris Diderot)04/07/2018 10:00
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Alec Habig (University of Minnesota Duluth)04/07/2018 10:20
The Supernova Early Warning System (SNEWS) is a cooperative effort between the world's neutrino detection experiments to spread the news that a star in our galaxy has just experienced a core-collapse event and is about to become a Type II Supernova. This project exploits the ~hours time difference between neutrinos promptly escaping the nascent supernova and photons which originate when the...
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Yusuke Koshio04/07/2018 11:00
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Segev BenZvi04/07/2018 11:40
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Zara Bagdasarian04/07/2018 14:00
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Sebastian Böser (Universität Bonn)04/07/2018 14:40
While the detection of a neutrino burst from a galactic supernova would provide a plethora of information on the stellar collapse as well as the neutrino properties, the low rate of 1-2 CCSNe per century make this a tedious endeavor. Instead, a detector with an effective mass of 10 Mton at 10MeV would detect extra-galactic supernovae at a rate of 1-2 per year - albeit with a much lower number...
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Inés Gil-Botella04/07/2018 15:20
The Deep Underground Neutrino Experiment (DUNE), a 40-kt liquid argon time projection chamber detector located deep underground at the 4850L of the Sanford Underground Research Facility (SURF) in South Dakota, will record the burst of neutrinos from the core collapse of a massive star in the Milky Way neighborhood.DUNE's liquid argon has unique sensitivity to the electron neutrino component of...
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04/07/2018 16:00
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Marta Colomer-Molla04/07/2018 16:30
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05/07/2018 09:30
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Massimiliano Lincetto (Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France)05/07/2018 10:00
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Vedran Brdar05/07/2018 10:30
Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova.
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In this talk we will present the update of the triangulation method for locating a core-collapse supernova by employing the neutrino arrival time differences at various detectors. We will discuss detailed numerical fits which are necessary in order to determine the uncertainties of... -
Cristina VOLPE (APC)05/07/2018 11:10
We discuss the recent progress in our understanding of flavor evolution in dense astrophysical environments, in particular core-collapse supernovae and binary neutron star mergers. We highlight what we might learn from a galactic supernova, the connection to r-process nucleosynthesis and to the recent kilonova observation.
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Antonio Marrone (Dipartimento di Fisica, Univ. di Bari & INFN Bari)05/07/2018 14:00
In this talk the status of both known and unknown neutrino oscillation parameters will be reviewed, with particular focus on the mass ordering and the its discrimination with present experiments and future projects. In this context our current understanding of supernova neutrino flavor conversions is discussed, from ordinary flavor oscillations during the shock-wave propagation to collective...
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Sajad Abbar05/07/2018 14:40
Neutrino evolution in dense neutrino media is a very nonlinear and rich phenomenon. Such a dense neutrino medium could be found in very extreme astrophysical sites such as core collapse supernovae and neutron star mergers. Studying collective neutrino oscillations in the aforementioned settings is very important since neutrinos could play a key role in their dynamics and nucleosynthesis. In...
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05/07/2018 15:20
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05/07/2018 16:00
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05/07/2018 16:30
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