ISAPP2025: Gravitational Waves: From Theory to Detection

This astroparticle physics graduate school will cover important and timely topics that are connected to gravitational waves, taught by internationally renowned experts. A primary focus of the school will be on understanding how gravitational waves emerge from the theory of general relativity and how these can be detected using modern technologies. Gravitational wave detectors, astrophysical sources, multimessenger astronomy and quantum sensing, are examples of the core topics that will be presented to the students. Lectures will be complemented with hands-on sessions. The duration of the school is 8 days.

ISAPP is a consortium of 40 European Institutions that organize Doctorate Schools on Astroparticle Physics for more than 20 years, https://www.isapp-schools.org. The Vienna Institute of High Energy Physics of the Austrian Academy of Sciences is a member of the consortium.

Key topics of the school include: 

  • Introduction to Gravitational Waves / Basic Theory: What are gravitational waves, and how do they arise from general relativity?
  • Sources of Gravitational Waves: What are the primary astrophysical sources that generate gravitational waves, and how do they vary in strength and frequency?
  • Gravitational Wave Detectors: Current gravitational wave detectors like LIGO and Virgo employ laser interferometry—what are the future improvements that might enhance their sensitivity?
  • Data Analysis and Signal Processing: How are gravitational wave signals extracted from noisy data, and what new computational techniques are being developed for more accurate analysis?
  • Gravitational Wave Cosmology: How can gravitational wave observations provide new insights into the expansion of the universe, dark matter, and dark energy?
  • Stochastic Gravitational-Wave Background: What sources contribute to the stochastic gravitational wave background, and how can it be distinguished from individual events?
  • Tests of General Relativity: How do gravitational wave detections allow us to test the limits of General Relativity, especially in extreme environments like black hole mergers?
  • Multimessenger Astronomy: In what ways do gravitational wave observations combined with electromagnetic and neutrino signals enhance our understanding of cosmic phenomena?
  • Quantum Sensing in Gravitational Wave Detection: How are quantum technologies, such as squeezed light, improving the sensitivity of gravitational wave detectors?
  • Public Outreach and Education: What strategies are being used to increase public awareness and understanding of gravitational wave science, and why is this important for future research development?

Coming soon.

Organizers

Name Affiliation
Oliver Hahn University of Vienna
Gianluca Inguglia HEPHY Vienna
Josef Pradler University of Vienna
Jochen Schieck HEPHY and Technical University Vienna
Glenn van de Ven University of Vienna

Attendees

Name Affiliation
Wen-Yuan Ai HEPHY Vienna
Saulo Albuquerque University of Urbino
Matteo Ballelli Gran Sasso Science Institute
Rasila Banu Universität Wien
Stefano Bartolomei Università degli Studi di Firenze
Daniel Beltran Centre for Energy, Environmental and Technological Research (CIEMAT)
Janus Brink University of Vienna
Alicia Calafat Universitat de les Illes Balears
Balázs Cirok University of Szeged
Stefano Colace Università di Genova
Elena Cuoco University of Bologna
William Delplanque University of Mons
Mohamed Samy Abdelmotteleb Elzokm Gran Sasso Science Institute
Maximilian Fahrecker Universität Wien
Yavuz Can Gençel University of Zurich
Manuel Goimil-García Niels Bohr Institute
Samuel Gomez Universitat de les Illes Balears
Elisa Grilli Niels Bohr Institute
Maria-Catalina Isfan Institute of Space Science
Kata Karácsonyi University of Szeged
Gideon Koekoek University of Maastricht
Daniil Krichevskiy University of Stavanger
Garance Lankester--broche Universität Wien
Alessandro Longo Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
Michela Mapelli University of Heidelberg
Luca Massaro Maastricht University
Shaoqiang Meng Universität Wien
Chiara Anna Montecuollo University Federico II of Napoli
Anna Moreso Serra Universitat de Barcelona, ICCUB
Stefan Nellen HEPHY Vienna
Anirudh Nemmani Nicolaus Copernicus Astronomical Center Polish Academy of Sciences
Costantino Pacilio University of Milano-Bicocca
Tobias Pausch TU Wien
Florentina Pislan Institute of Space Science
Jan Ramaj Comenius University
Tania Regimbau Laboratoire d'Annecy de Physique des Particules
Federica Santucci University of Torino
Lijing Shao KAVLI - Peking University
Tamar Simhon BGU
Brecht Slootmaekers Maastricht University
Jessica Steinlechner University of Maastricht
Igor Stellet Centro Brasileiro de Pesquisas Físicas
Dawid Stepanovic Universität Wien
Leonardo Torcellini University of Salento
Kristyna Vitulova HEPHY Vienna
Tristan Weaver The Pennsylvania State University
Ann Cathrin Wesener Max-Planck-Institut für Kernphysik
Clifford M. Will University of Florida
Changhao Xu Johannes-Gutenberg Universität Mainz
Jesus Gabriel Yepez Moreno Technical University of Vienna
At a glance
Type:
Graduate School
When:
July 7, 2025 — July 18, 2025
Where:
ESI Boltzmann Lecture Hall
Organizer(s):
Oliver Hahn (U of Vienna)
Gianluca Inguglia (HEPHY Vienna)
Josef Pradler (U of Vienna)
Jochen Schieck (HEPHY and TU Vienna)
Glenn van de Ven (U of Vienna)
More:
Website