GRIT AGATA VAMOS 2029-2030 Campaign

Europe/Paris
GuestHouse (GANIL)

GuestHouse

GANIL

Description

The AGATA European Tracking array will be hosted at the GANIL Facility in 2029 and 2030 with a possible extension in 2031. The primary objective is an experimental campaign using a 2\pi AGATA coupled to GRIT, a 4\pi silicon array for light charged particle spectroscopy, and the high acceptance VAMOS magnetic spectrometer. 

The present meeting aims at defining more precisely the physics objectives with the goal of editing a white book to prepare the campaign. The worshop will also include technical aspects with discussion on the detection systems geometries, constrains, front end electronic and softwares. The management of the campaign will be also introduced. 

The campaign will benefit of the existing SPIRAL1 beams but developpment of new beams will be encouraged. 

The meeting is in presence but remote connection is available

https://cnrs.zoom.us/j/92308700103?pwd=KNXiOgn4FxLJWsI1velyH5EnU3lvob.1

Inscription
Registration
    • 14:00 16:10
      Presentation of the detectors
      • 14:00
        Introduction by GANIL Management 15m
        Orateur: Fanny Farget (GANIL)
      • 14:15
        AGATA Status 25m
        Orateur: Dr Emmanuel CLEMENT (GANIL)
      • 14:40
        GRIT Status 25m
        Orateur: Didier Beaumel (IPN Orsay)
      • 15:05
        VAMOS Status 25m
        Orateur: Dr Diego RAMOS DOVAL (GANIL)
      • 15:30
        SPIRAL1 Status for the campaign 25m
        Orateur: Pascal Jardin Jardin (CNRS/GANIL)
    • 16:10 16:30
      Coffee 20m
    • 16:30 18:30
      Physics 1
      • 16:30
        Microscopic origins of shape coexistence at N, Z ∼ 40 explored through direct transfer 30m
        Orateur: Charlie James PAXMAN (GANIL)
      • 17:00
        DSAM Measurement in 24Ne – Ab-Initio test 30m
        Orateur: Dr Emmanuel CLEMENT (GANIL)
      • 17:30
        Spectroscopy of proton-rich nuclei using charge-exchange reactions and proton adding with a 3He target 30m
        Orateur: BEATRIZ FERNANDEZ DOMINGUEZ (USC)
    • 09:30 11:00
      Physics 2
      • 09:30
        Probing mixed-spin np pairing in the super-collective Z~60 and A~130 region 30m
        Orateur: Jeremie Dudouet (IP2I)
      • 10:00
        Study of n-­‐p pairing in fp-­‐shell through two-­‐nucleon transfer reactions 30m
        Orateur: Marlene Assie (IJCLab)
      • 10:30
        Nuclear Astrophysics from UK 30m
        Orateur: Gavin Lotay
    • 11:00 11:20
      Coffee 20m
    • 11:20 12:50
      Data Flow and Data Analysis
      • 11:20
        GRIT Data Pipe 20m
        Orateurs: Dr Adrien Matta (LPC Caen, CNRS-IN2P3), Valérian Girard-Alcindor (IJCLAB)
      • 11:40
        AGATA Data pipe 20m
        Orateurs: Jeremie Dudouet (IP2I), Olivier Stezowski (IP2I)
      • 12:00
        VAMOS data pipe 20m
        Orateur: Dr Diego RAMOS DOVAL (GANIL)
      • 12:20
        Common DMP (Discussion) 20m

        Open discussion on how to organize the data management Post experiment.

    • 13:00 14:00
      Lunch 1h
    • 14:00 15:30
      Physics 3.
      • 14:00
        Clustering in medium-mass proton-rich nuclei studied through Li-induced stripping reactions 30m
        Orateurs: Didier Beaumel (IPN Orsay), Valérian Girard-Alcindor (IJCLAB)
      • 14:30
        Order of magnitude lifetime measurements in 66Ni 30m
        Orateur: Joa Ljungvall (IPHC/IN2P3/CNRS)
      • 15:00
        SRC and Shell evolution with the 3He,d reaction 30m
        Orateur: Andrea Gottardo (LNL INFN)
    • 15:30 16:00
      Coffee 30m
    • 16:00 17:00
      Physics 4
      • 16:00
        Italian Mid Mass Contribution 20m
        Orateur: Daniele Mengoni (University and INFN - Padova)
      • 16:20
        Italian Light Nuclei Contribution 20m
        Orateur: Dr Simone Bottoni (University of Milano and INFN)
      • 16:40
        (3He,n) reaction by Italy 20m
        Orateur: Franco Galtarossa (INFN Sezione di Padova)
    • 17:00 18:00
      Scientific Discussion

      How to organize a "white Book" ?
      How to organize the future Pre-PAC ?
      How we see the future PAC ?
      How we see the involvment of the PI's team on top of the GRIT, VAMOS, AGATA collaboration ?

    • 09:00 10:00
      Mechanics and infra
      • 09:00
        AGATA integration 30m
        Orateur: Patrice Gangnant
      • 09:30
        GRIT Integration 30m
        Orateur: Marlene Assie (IJCLab)
    • 10:00 10:30
      Coffee 30m
    • 10:30 11:30
      Front - End and clock distribution
      • 10:30
        GRIT BEE 20m
        Orateur: David Etasse (LPC Caen)
      • 10:50
        AGATA BEE 20m
        Orateurs: Andres Gadea (IFIC CSIC-University of Valencia), Dr Emmanuel CLEMENT (GANIL)
      • 11:10
        SMART + GANIL coupling 20m
        Orateur: Matthieu BEZARD (GANIL (Caen))
    • 11:30 12:00
      Conclusion 30m