PhD International School on Technologies in Gravitational Waves Detection 2026

Europe/Rome
Ettore Majorana Centre for Scientific Culture, Erice, Sicily

Ettore Majorana Centre for Scientific Culture, Erice, Sicily

Via Gian Filippo Guarnotti, 26, 91016 Erice (TP), Italy
Description

 

We are pleased to announce the first edition of the PhD International School on Technologies in Gravitational Waves Detection (STGWD). The event will be held at Ettore Majorana Centre for Scientific Culture in Erice, Sicily (Italy), on May 20th-27th, 2026.

 

The scientific program includes a theoretical introduction to the fundamental principles of gravitational wave detection, along with lectures and practical sessions dedicated to the main features of ground-based and space-based interferometric detectors, paying particular attention to the following fields:

 

  • GW theoretical aspects and principia
  • Future GW Observatories
  • Technologies aspects (interferometry, optics, controls, noise mitigation)
  • Data Analysis

 

The school STGWD is designed primarily for PhD students, recent MSc graduates, final‑year MSc candidates, and early‑career researchers, while remaining open to anyone eager to deepen their expertise.

 

STGWD aims to foster scientific exchange through dedicated time for discussions, hands‑on activities, and poster sessions. The event offers an excellent opportunity to strengthen connections within the GW community and to expand networks with fellow young researchers as well as established experts.

 

Registration will be open from 19/01/2026 to 30/04/2026

Payment information are available in the indico page after the pre-registration phase.

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Scientific Organizing Committee: M. Punturo, P. Campana, H. Luek, G. Gemme, D. D'Urso, G. Cella, R. Dolesi, F. Travasso, L. Naticchioni.

Directors: F. Travasso, L. Naticchioni

Registration
International School on Technologies in Gravitational Waves Detection 2026
    • 14:00 15:50
      GW theoretical aspects and principia
      • 14:00
        Theoretical aspects of GW 1h 50m
        Speaker: Dr Giancarlo Cella (INFN Pisa)
    • 15:50 16:05
      Coffee Break 15m
    • 16:05 17:55
      GW theoretical aspects and principia
      • 16:05
        GW detectors principia 1h 50m
        Speaker: Gianluca Gemme (INFN)
    • 09:00 10:50
      GW theoretical aspects and principia
      • 09:00
        Theoretical aspects of GW 1h 50m
        Speaker: Dr Giancarlo Cella (INFN Pisa)
    • 10:50 11:05
      Coffee Break 15m
    • 11:05 12:55
      GW theoretical aspects and principia
      • 11:05
        GW detectors principia 1h 50m
        Speaker: Gianluca Gemme (INFN)
    • 12:55 14:30
      Lunch 1h 35m
    • 14:30 16:20
      3G GW Observatories
      • 14:30
        3G observatories and ET 1h 50m
    • 16:20 16:35
      Coffee Break 15m
    • 16:35 18:25
      3G GW Observatories
      • 16:35
        Space-based detectors: sensitivity 1h 50m
        Speaker: Bill Weber
    • 09:00 10:50
      Optics & interferometry
      • 09:00
        Optical configuration 1h 50m
        Speaker: Antonio Perreca
    • 10:50 11:05
      Coffee Break 15m
    • 11:05 12:55
      Interferometer test masses
      • 11:05
        Seismic filtering 1h 50m
        Speaker: Piero Chessa (University of Perugia)
    • 12:55 14:30
      Lunch 1h 35m
    • 14:30 16:20
      Interferometer test masses
      • 14:30
        Coatings & Materials 1h 50m
        Speaker: Michele Magnozzi
    • 16:20 16:35
      Coffee Break 15m
    • 16:35 18:25
      Optics & interferometry
      • 16:35
        Space interferometry 1h 50m
        Speaker: Gudrun Wanner
    • 20:00 22:00
      Socia Dinner 2h
    • 09:00 10:50
      Optics & interferometry
      • 09:00
        Optical configuration 1h 50m
        Speaker: Antonio Perreca
    • 10:50 11:05
      Coffee Break 15m
    • 11:05 12:55
      Optics & interferometry
      • 11:05
        Interferometer Controls 1h 50m
        Speaker: Manuel Pinto
    • 12:55 14:30
      Lunch 1h 35m
    • 09:00 10:50
      Optics & interferometry
      • 09:00
        Laser Technologies 1h 50m
        Speaker: Marco Galimberti
    • 10:50 11:05
      Coffee Break 15m
    • 11:05 12:55
      Optics & interferometry
      • 11:05
        Stray light 1h 50m
        Speaker: Dr Livia Conti (INFN)
    • 12:55 14:30
      Lunch 1h 35m
    • 14:30 16:20
      Interferometer test masses
      • 14:30
        Thermal compensation 1h 50m
        Speaker: Ilaria Nardecchia
    • 16:20 16:35
      Coffee Break 15m
    • 16:35 18:25
      Noise control
      • 16:35
        Noise control in a space-based observatory 1h 50m
        Speaker: Lorenzo Sala
    • 09:00 10:50
      Optics & interferometry
      • 09:00
        Squeezing 1h 50m
        Speaker: Fiodor Sorrentino
    • 10:50 11:05
      Coffee Break 15m
    • 11:05 12:55
      Optics & interferometry
      • 11:05
        Stray light 1h 50m
        Speaker: Dr Livia Conti (INFN)
    • 12:55 14:30
      Lunch 1h 35m
    • 14:30 16:20
      Data Analysis
      • 14:30
        Data analysis methodologies 1h 50m
        Speaker: Francesco Pannarale (Sapienza – University of Rome & INFN Roma)
    • 16:20 16:35
      Coffee Break 15m
    • 16:35 18:25
      Data Analysis
      • 16:35
        Data Analysis for space-based detectors 1h 50m
        Speaker: Riccardo Buscicchio
    • 09:00 10:50
      Data Analysis
      • 09:00
        Data analysis methodologies 1h 50m
        Speaker: Francesco Pannarale (Sapienza – University of Rome & INFN Roma)
    • 10:50 11:05
      Coffee Break 15m
    • 11:05 12:55
      Interferometer test masses
      • 11:05
        Elements of cryogenics in GW detectors 1h 50m
        Speaker: Ettore Majorana
    • 12:55 14:30
      Lunch 1h 35m
    • 14:30 16:20
      Noise control
      • 14:30
        Environmental noise and impact on the detector 1h 50m
        Speaker: Rosario De Rosa
    • 16:20 16:35
      Coffee Break 15m
    • 16:35 18:25
      2G detectors achievements
      • 16:35
        Scientific achievements of the current detectors 1h 50m
        Speaker: Barbara Patricelli (University of Pisa and INFN - Pisa)