SNvD 2023@LNGS: International Conference on Supernova Neutrino Detection

May 29, 2023, 1:30 PM → Jun 1, 2023, 6:00 PM Europe/Rome

Auditorium "E: Fermi" (LNGS)

Topics:
- theory of SN emission
- lessons from 1987A
- SN observations with photons 
- past detectors for SN neutrinos
- detectors in the world ready to take SN neutrinos
- situation at LNGS 
- SNEWS alert system
- new ideas
- diffused SN

The conference will discuss the legacy and strategy for the next Supernova Neutrino detection with detectors located at both LNGS and other laboratories around the world.

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The conference will take place at Gran Sasso National Laboratory of INFN - Assergi, L'Aquila (Italy).

All information on fee and payment method are available on Conference Fee section of top-left menu.

The list of affiliated hotels and the instructions about reservation are available on the Accommodation section of top-left menu.

Shuttle bus service from affiliated hotels to the conference venue will be available during the conference days. Timetable and other details will be posted on Travel section of top-left menu.

The timetable is still preliminary.
 

INFN_Information_on_the_Processing_of_personal_data.pdf

Monday, May 29

1:30 PM → 9:25 PM talk session

1:30 PM lunch

2:30 PM Conference introduction

Speakers: Carlo Bucci (Istituto Nazionale di Fisica Nucleare), Walter M. Bonivento (INFN Cagliari)

2:50 PM Welcome from the INFN managment

Speaker: Prof. Marco Pallavicini (GE)

3:05 PM Welcome from the LNGS director

Speaker: Ezio Previtali (MIB)

3:25 PM New physics and SN neutrinos

Speaker: Manibrata Sen (Max-Planck-Institut für Kernphysik)

4:05 PM SuperKamiokande sensitivity

Speaker: Takeda Atsushi (ICRR, Univ. of Tokyo)

4:35 PM RESNOVA

Speaker: Luca Pattavina (INFN-LNGS / TUM)

5:05 PM Coffee break

5:45 PM DarkSide-20k/ARGO sensitivity

Speaker: Davide Franco (APC)

6:15 PM Supernova neutrinos and oscillations

Speaker: James Kneller (NC State University)

7:00 PM Xenon-nT and Darwin/XLZD sensitivity

Speaker: Melih Kara (KIT-Karlsruhe)

Tuesday, May 30

9:00 AM → 10:30 PM talk session

9:00 AM SN @ JUNO

Speaker: Achim Stahl (University of Aachen)

9:30 AM The Theory of Three-Dimensional Core-Collapse Supernova Explosions

Using our code Fornax we have simulated the collapse and explosion of the cores of many massive-star models in three spatial dimensions. This is the most comprehensive set of realistic 3D core-collapse supernova (CCSN) simulations yet performed and has provided very important insights into the mechanism and character of this 60-year-old astrophysical puzzle. Most 3D models explode naturally and without artifice by the neutrino mechanism, aided by turbulent convection. I will present detailed results from this suite of runs and the novel conclusions derived from our new capacity to simulate many 3D, as opposed to 2D and 1D, full physics models every year. Emerging are insights into the criteria for explosion, the systematics of explosion energy and residual neutron-star mass with progenitor, the characteristics of proto-neutron star convection, neutrino and gravitational-wave emissions and signatures, the morphology of CCSN explosions, and supernova nucleosynthesis. This new capability, enabled by this new algorithm and modern HPC assets, is poised to transform our understanding of this central astrophysical phenomenon.

Speaker: Adam Burrows (Princeton University)

10:30 AM SN at SNO+

Speaker: Tseng Jeffrey (Oxford University)

11:00 AM Coffee break

11:25 AM Studies of the SN1987A region

Speaker: Marco Miceli (INAF-Osservatorio Astronomici di Palermo G. S. Vaiana)

12:00 PM Neutron stars

Speaker: Prof. Jocelyn Bell-Burnell (University of Dundee)

1:30 PM Lunch

2:30 PM SN modelling and neutrinos

Speaker: Hans-Thomas Janka (Max Planck Institute for Astrophysics)

3:30 PM SN@DUNE

4:00 PM pre-collapse phase and multi-messenger signatures of core-collapse supernovae.

Speaker: Kei Kotake (Fukuoka University)

4:50 PM Coffee break

5:20 PM Quantum decoherence in Supernova neutrino detection

Speaker: Marcos Vinicius dos Santos (Unicamp)

5:40 PM LZ sensitivity

Speaker: Matthew Szydagis (University of Albany)

6:10 PM SN neutrino fluxes in different experiments and anti-neutrino fluxes

Speaker: Andrea Gallo Rosso (GSSI)

6:40 PM LVD Legacy

Speaker: Carlo Francesco Vigorito (Istituto Nazionale di Fisica Nucleare)

8:30 PM Conference Dinner

Wednesday, May 31

9:00 AM → 2:30 PM talk session

9:00 AM SNEWS alert system

9:25 AM SNEWS software stacks

Speaker: Jost Migenda (King’s College London)

9:45 AM Follow up with GRANMA

Speaker: Alexis Coleiro (APC / University Paris Diderot)

10:15 AM SN@HYPERK

Speaker: Gianfranca De Rosa (Istituto Nazionale di Fisica Nucleare)

10:45 AM Coffee

11:15 AM Multi-messenger: GWs and neutrinos

Speaker: Giulia Pagliaroli (Istituto Nazionale di Fisica Nucleare)

11:45 AM DSNB

Speaker: Shunsaku Horiuchi (Virginia TEch)

12:25 PM HALO

Speaker: Clarence Virtue (Laurentian University / SNOLAB)

1:00 PM Supernova-produced dark matter and directional detectors like CYGNO

Speaker: Elisabetta Baracchini (Istituto Nazionale di Fisica Nucleare)

1:30 PM Lunch

2:30 PM → 5:00 PM talk session

3:00 PM KM3net

Speaker: Vladimir Kulikovskiy (Istituto Nazionale di Fisica Nucleare)

3:30 PM Measurement of cross-section with COHERENT

Speaker: Yuri Efremenko (University of Tennessee, Knoxville)

4:00 PM Directionality/Pointing/Triangulation

Speaker: Kate Scholberg (Duke University)

4:30 PM Coffee

5:00 PM → 7:20 PM Visit: Underground laboratory visit

Thursday, June 1

9:00 AM → 11:25 AM session

9:00 AM Legacy from Borexino

Speaker: Riccardo Biondi (Istituto Nazionale di Fisica Nucleare)

9:30 AM SN @ ICECUBE

Speaker: Segev BenZvi (University of Wisconsin)

10:00 AM Triangulation methods

Speaker: Jeffrey Tseng (University of Oxford)

10:30 AM SN@CUORE AND CUPID

Speaker: Matteo Biassoni (Istituto Nazionale di Fisica Nucleare)

11:00 AM Neutrino mass ordering from Supernova neutrinos

Speaker: Cesar Jesus-Valls (Kavli IPMU)

11:30 AM → 12:00 PM Coffee

12:00 PM → 2:40 PM wrap-up

12:00 PM The SNOWMASS process for SN neutrinos

Speaker: Erin O'Sullivan (Uppsala University)

12:25 PM Round table: next steps

Speakers: Aldo Ianni (Istituto Nazionale di Fisica Nucleare), Francesco Vissani (Istituto Nazionale di Fisica Nucleare)