SN neutrinos at the crossroads: astrophysics, oscillations, and detection

Name: SN neutrinos at the crossroads: astrophysics, oscillations, and detection
Start: 2019-05-13T08:00:00+02:00
End: 2019-05-17T19:00:00+02:00
Location: ECT* - Villa Tambosi

13 May 2019, 08:00 → 17 May 2019, 19:00 Europe/Rome

Meeting room (ECT* - Villa Tambosi)

Meeting room

ECT* - Villa Tambosi

Strada delle Tabarelle, 286 38123 - Villazzano (TN) Italy

Alessandro Mirizzi ( University of Bari ) (University of Bari), Basudeb Dasgupta ( Tata Institute for Fundamental Research ) (Tata Institute for Fundamental Research)

Description

SN neutrinos at the crossroads: astrophysics, oscillations, and detection

The next Galactic supernova (SN) would be a once in a lifetime event for particle astrophysics, offering a unique opportunity for a multi-messenger detection of gravitational waves, neutrinos of all flavors, and multi-wavelength photons. The aim of the workshop is to review and discuss the recent advances in the study of SN neutrinos and future perspectives, ranging from SN simulations, neutrino oscillations, nucleosynthesis, gravitational waves, and SN neutrino experimental searches. The workshop is structured to address these broad issues in a synergistic interdisciplinary way and to stimulate discussions and collaborations among scientists working on SN neutrinos from different perspectives.

Main Topics:

Core-collapse simulations
Microphysics of supernova core
Stellar nucleosynthesis
Neutrino flavor conversions
Exotic particle emissions
Neutrino detection strategies

Secretariat: Susan Driessen

driessen@ectstar.eu

+39 0461 314722

Monday 13 May
- 08:30 → 09:30
  
  registration
- 09:40 → 10:00
  Welcome
  - 09:40
    
    Welcome talk 20m
    
    Speaker: Prof. Jochen Wambach (Director of ECT*)
- 10:00 → 17:50
  Astrophysics Session
  - 10:00
    
    Supernovae and neutrinos 40m
    
    Speaker: Prof. John Beacom (Ohio State Univ.)
    
    ECT2019-Beacom.pdf
  - 10:40
    
    Coffee Break 40m
  - 11:20
    
    Core collapse supernova simulation at the crossroads 40m
    
    Speaker: Prof. Anthony Mezzacappa
    
    TrentoWorkshop_Mezzacappa_V6.pdf
  - 12:00
    
    Lunch 2h
  - 14:00
    
    Multi-messenger supernova neutrino detection 30m
    
    Speaker: Prof. Irene Tamborra (Niels Bohr Institute)
    
    ECT_Tamborra.pdf
  - 14:30
    
    Pushing spherically symmetric SN to explosion 30m
    
    Speaker: Prof. Carla Fröhlich (North Carolina State University)
    
    frohlich_Trento_SNnu_PUBLIC.pdf
  - 15:00
    
    SN gravitational waves at the crossroads: synergetic analysis with SN neutrinos 30m
    
    Speaker: Prof. Kei Kotake (Fukuoka University)
    
    kotake_ectstar.pdf
  - 15:30
    
    Coffee Break 40m
  - 16:10
    
    Neutrino bremsstrahlung rate in supernova matter revisited based on chiral EFT potential 30m
    
    Speaker: Dr Guo Gang (GSI)
    
    Gang_neutrino_brem.pdf
  - 16:40
    
    Probing rotation of core-collapse supernovae with neutrino gyroscopes 20m
    
    Speaker: Dr Laurie Walk (Niels Bohr Institute)
    
    LWalk_Presnetation_Trento.pdf
  - 17:00
    
    Core-collapse supernovae are thermonuclear explosions 20m
    
    Speaker: Dr Doron Kushnir (Weizmann Institute of Science)
  - 17:20
    
    Supernova neutrino detection with KM3NeT 20m
    
    Speaker: Dr Vladimir Kulikovskiy (INFN Sezione Di Genova)
    
    KM3NeT_CONF_2019_XXX_Trento_Kulikovskiy_v3.pdf
Tuesday 14 May
- 10:00 → 18:50
  Flavor conversions
  - 11:20
    
    Flavor evolution of dense neutrinos as an emergent phenomenon 40m
    
    Speaker: Dr Georg Raffelt (MPI Munich)
    
    Raffelt-Trento.pdf
  - 12:00
    
    Lunch 2h
  - 14:00
    
    Effective theory of collective neutrino oscillations 30m
    
    Speaker: Prof. Alexei Smirnov (MPI Heidelberg)
    
    Smirnov_trento19.pptx
  - 14:30
    
    Algebraic approach to collective neutrino oscillations 30m
    
    Speaker: Prof. Baha Balantekin (University of Wisconsin)
    
    ECT2019_Balantekin.pdf
  - 15:00
    
    Neutrino flavor evolution beyond the standard frameworks 30m
    
    Speaker: Prof. Cristina Volpe (APC, Paris)
    
    MCVolpe-ECT_.pdf
  - 15:30
    
    Coffee Break 40m
  - 16:10
    
    NSI effects on supernova neutrino oscillations 30m
    
    Speaker: Prof. Amol Dighe (TIFR, Mumbai)
    
    Dighe-trento19.pdf
  - 16:40
    
    Numerical toy models for fast and slow neutrino oscillations 30m
    
    Speaker: Prof. Guenter Sigl (Hamburg University)
    
    Sigl_trento.pdf
  - 17:10
    
    Coffee break 20m
  - 17:30
    
    Slow and fast collective oscillations: 3 flavor analysis 20m
    
    Speaker: Prof. Sovan Chakraborty (Indian Institute of Technology, Guwahati)
    
    Chakraborty_Trento.pdf
  - 17:50
    
    Stability of three flavor neutrino conversion in supernova 20m
    
    Speaker: Mr Christian Döring (MPI Heidelberg)
    
    Talk_ChristianDoering_14519-expanded.pdf
Wednesday 15 May
- 09:00 → 18:50
  Nucleosynthesis and new particle emission
  - 09:30
    
    Neutrinos and supernovae 40m
    
    Speaker: Prof. Thomas Janka (MPI Garching)
  - 10:10
    
    Nucleosynthesis: an overview 40m
    
    Speaker: Prof. Karlheinz Langanke (GSI Helmholtzzentrum für Schwerionenforschung GmbH)
    
    Langanke.ppt
  - 10:50
    
    Coffee break 40m
  - 11:30
    
    Neutrinos and nucleosynthesis in supernova 40m
    
    Speaker: Prof. Gabriel Martinez-Pinedo (GSI Darmstadt)
  - 12:10
    
    Lunch 1h 30m
  - 13:40
    
    Neutrino nucleosynthesis with time-dependent neutrino-emission spectra 20m
    
    Speaker: Dr Andre Sieverding (University of Minnesota)
    
    Sieverding_Trento.pdf.pdf
  - 14:00
    
    Effect of opacities on neutrino signal 30m
    
    Speaker: Prof. Tobias Fischer (Wraclow University)
    
    Fischer_trento2019.pdf
  - 14:30
    
    Coffee Break 30m
  - 15:00
    
    Colloqium: Chasing Neutrinos Around the World: A Personal History 1h
    
    ABSTRACT: Come hear a dramatic and entertaining account of the first half century of experimental neutrino science. Through rare photos, insider stories, and other primary source material, travel from Hanford and Savannah River in the US to South Africa, on to India, back to the US, over to Japan, and finally off to Sweden - twice! Hear about the soaring triumphs, crushing setbacks, and international rivalries which have helped define the last six decades in this challenging field, as well as what the
    near future has in store. This colorful lecture is based almost entirely on the speaker's first hand experiences as well as his interviews with other eyewitnesses to physics history.
    
    Speaker: Prof. Mark Vagins (IMPU Tokyo)
    
    Trento19_Vagins.pdf
  - 16:00
    
    Coffee break 20m
  - 16:20
    
    Supernovae & axions 30m
    
    Speaker: Prof. Maurizio Giannotti (Barry Univ., Miami)
    
    MGiannotti_ ECT_2019.pdf
  - 16:50
    
    Progenitors of core-collapse SNe: neutrinos and other WISPs 30m
    
    Speaker: Prof. Oscar Straniero (Italian National Instutute of Astrophysics)
    
    Straniero.pdf
  - 17:20
    
    Global comparison of spherically symmetric SN explosions 30m
    
    Speaker: Prof. Evan O'Connor (Stockholm University)
    
    OConnor_global_ectstar.pdf
  - 17:50
    
    Break 20m
  - 18:10
    
    The effect of neutrino oscillations on core-collapse supernova explosion 20m
    
    Speaker: Dr Charles Stapleford (North Carolina State University)
    
    SNCrossroads_Stapleford.pdf
  - 18:30
    
    Crossings between the angular distributions of neutrinos in the supernova core 20m
    
    Speaker: Dr Shashank Shalgar (Niels Bohr Institute)
    
    Shalgar-talk.pdf
Thursday 16 May
- 09:20 → 19:50
  Neutrino detection strategies
  - 10:00
    
    Supernova neutrino detection 40m
    
    Speaker: Prof. Kate Scholberg (Duke Univ.)
    
    trento-Scholberg.pdf
  - 10:40
    
    Coffee break 40m
  - 11:20
    
    Determining supernova unknowns with the diffuse supernova neutrino background 30m
    
    Speaker: Dr Anna Suliga (Niels Bohr Institute, University of Copenhage)
    
    Suliga_Trento2019.pdf
  - 11:50
    
    Lunch 1h 10m
  - 13:00
    
    Detecting the DSNB in water-based liquid scintillators 30m
    
    Speaker: Prof. Michael Wurm (JGU Mainz)
    
    Wurm_dsnb_wbls_trento_may19.pdf
  - 13:30
    
    Supernovae, IceCube, and new ideas 30m
    
    Speaker: Prof. Lutz Köpke (Johannes Gutenberg University Mainz)
    
    LutzKoepkeTrentoTalkshort.pptx
  - 14:00
    
    SN neutrinos at JUNO 30m
    
    Speaker: Prof. Shun Zhou (Institute of High Energy Physics, Chinese Academy of Sciences)
    
    Trento-ZHOU-190516.pdf
  - 14:30
    
    Coffee break 40m
  - 15:10
    
    Full-flavor reconstruction of supernova neutrino energy spectra 20m
    
    Speaker: Dr Huiling Li (Institute of High Energy Physics)
    
    20190516_ECT_HLi.pdf
  - 15:30
    
    The JUNO detector and its potential in detecting CCSN neutrinos 20m
    
    Speaker: Ms Cristina Martellini (University Roma 3)
    
    Martellini_Trento_2019.pdf
  - 15:50
    
    HALO-1kT: a lead-based supernova detector 20m
    
    Speaker: Dr Andrea Gallo-Rosso (Laurentian University)
    
    Gallo_Rosso_ECT.pdf
  - 16:10
    
    Coffee break 20m
  - 16:30
    
    Development of the comprehensive analysis tools for the supernova neutrino detectors 20m
    
    Speaker: Dr Vsevolod Orekhov (Johannes Gutenberg-Universität Mainz)
    
    Orekhov_sn.pdf
  - 16:50
    
    Sensitivity of SNO+ to supernova neutrinos 20m
    
    Speaker: Dr Mark Stringer (Queen Mary University Of London)
    
    Stringer_ECTSNTalk.pdf
  - 17:10
    
    Break 20m
  - 17:30
    
    Neutrino evolution in dense neutrino media and self-induced flavor equilibrium 20m
    
    Speaker: Dr Sajad Abbar (APC, Paris)
    
    Abbar_Trento_2019.pdf
  - 17:50
    
    Moments, fast conversions and SN simulations 20m
    
    Speaker: Dr Manibrata Sen (Northwestern University)
    
    ECT_Talk_Manibrata_Sen.pdf
  - 18:10
    
    Criterion for fast flavor conversion 20m
    
    Speaker: Mr Tobias Stirner (MPI Munich)
    
    CrossingProof_Stimer.pdf

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SN neutrinos at the crossroads: astrophysics, oscillations, and detection

Meeting room

ECT* - Villa Tambosi