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SNEWS Meeting @ Neutrino2020

19–20 Jun 2020
Zoom
US/Central timezone

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Contribution List

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3. Manibrata Sen
Manibrata Sen
19/06/2020, 07:00
4. Laurie Walk
Dr Walk Laurie
19/06/2020, 07:20
5. Tommy Lam
Tommy Lam (Virginia Tech)
19/06/2020, 07:40
15. Pointing with presupernova neutrinos
Cecilia Lunardini (Arizona State University)
19/06/2020, 08:15
16. Shape analysis and combination of presupernova signals
Andrey Sheshukov (JINR)
19/06/2020, 08:35
17. Pre-supernova neutrino alert with SNO+
Janet Rumleskie (Laurentian University)
19/06/2020, 08:55
29. Overview
Segev BenZvi (University of Rochester)
19/06/2020, 09:30
22. Sensitivity of KM3Net to CCSNe: Online and Offline Performance
Massimiliano Lincetto, marta colomer (km3net)
19/06/2020, 09:36
24. Sensitivity of RES-NOVA to supernova neutrinos
Luca Maria Pattavina (INFN - National Institute for Nuclear Physics)
19/06/2020, 09:54
25. Sensitivity of LZ to supernova neutrinos
Elise McCarthy (University of Rochester)
19/06/2020, 10:12
19. Scimma and Hopskotch
Amanda Depoian (Purdue University), Skylar(Yiyang) Xu (Rice Univeristy)
19/06/2020, 10:40
20. Signifcance-based Alerts
Andrey Sheshukov (JINR)
19/06/2020, 11:00
7. Introduction to session
Jeffrey Tseng (University of Oxford (GB))
20/06/2020, 07:00
8. Pointing based on anisotropic interactions
Kate Scholberg (Duke University)
20/06/2020, 07:05
9. Pointing confidence area estimation
Dr Vladimir Kulikovskiy (INFN Genova), marta colomer (km3net)
20/06/2020, 07:15
10. Time measurements from individual experiments
Clarence Virtue (Laurentian University)
20/06/2020, 07:30
11. Pointing with shape information
Jia-Shian Wang (University of Hong Kong (HK))
20/06/2020, 07:40
12. Systematic uncertainties discussion
20/06/2020, 07:50
13. Discussion on Next Steps
Kate Scholberg (Duke University)
20/06/2020, 08:05
30. Intro to fire drill overall strategy
Erin O'Sullivan (Stockholm University)
20/06/2020, 08:30
31. Brainstorming - supernova modelling
Evan O'Connor, James Kneller (NC State University)
20/06/2020, 08:40
32. Brainstorming - Detector response
Segev BenZvi (University of Rochester)
20/06/2020, 08:45
33. Brainstorming - Pre-supernova
Andrey Sheshukov (JINR), Cecilia Lunardini (Arizona State University)
20/06/2020, 08:50
34. Brainstorming - implementation
Alec Thomas Habig (University of Minnesota (US))
20/06/2020, 08:55
35. Brainstorming - triangulation
Jeffrey Tseng (University of Oxford (GB)), Kate Scholberg (Duke University)
20/06/2020, 09:00
36. Brainstorming - Multimessenger
Dan Milisavljevic (Purdue University)
20/06/2020, 09:05
37. Brainstorming - Outreach
Justin Vasel (Indiana University)
20/06/2020, 09:10
38. Discussion
20/06/2020, 09:15
2. Analytic Model for Supernova Neutrinos
Tommy Lam (Virginia Tech)
Signal Prediction - Modeling
Poster
Signal Prediction - Modeling

We report the status of upgrading the analytic supernova model of Mueller et al. (2016) with a focus on neutrino emission. Our simple model is calibrated to existing numerical supernova simulations and will include the dependence on the mass density property of the progenitor to yield neutrino predictions within seconds.
23. Detector response of KM3Net, offline implementation
Massimiliano Lincetto, marta colomer (km3net)
21. Discussion
Alec Thomas Habig (University of Minnesota (US))

Open discussion (everyone).
28. Preparing to Observe the Next Galactic Supernova with IceCube
Spencer Griswold (University of Rochester)
Alert Formation - Fire Drills
Poster
Alert Formation - Fire Drills

The next Galactic supernova will be a historic opportunity for multi-messenger astronomy. A core collapse will produce a neutrino burst visible up to half a day before electromagnetic radiation from the explosion, providing an early warning for optical follow-up and valuable insight about the proto-neutron star. Since local supernovae are exceedingly rare, it is critical that neutrino...
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