SISSA
This nodeTrieste, Italy
Black hole astrophysics, environmental effects, tests of gravity, GW statistics and machine learning
ERC Synergy Grant · 101167314
Making sense of the unexpected in the gravitational-wave sky, SISSA node
GWSky is an ERC Synergy Grant that unites four nodes — SISSA, the Max Planck Institute for Gravitational Physics (AEI) in Potsdam, UCLA, and the Niels Bohr Institute — to build the theoretical framework and analysis tools needed for the coming flood of gravitational-wave observations. This site is the SISSA node.
14
Current researchers
33
Papers from the node
2025–2031
Six-year Synergy Grant
Four nodes
SISSA is one of four nodes. The consortium site is gwsky.org.
Albert Einstein Institute
Potsdam, Germany
PI Alessandra Buonanno
Gravitational-wave modelling and strong-field dynamics
UCLA
Los Angeles, USA
PI Zvi Bern
Quantum field theory methods for gravity
Niels Bohr Institute
Copenhagen, Denmark
PI Maarten van de Meent
Nonlinear strong-field dynamics and self-force
Meetings organised
Seminars and meetings27–31 July 2026
Precision Gravitational Wave Astronomy: From Theory to Discovery
Haus Sexten · Sexten / Sesto, Italy
Meeting website8–12 June 2026
Perspectives on Gravity: From Theory to Observation
IFPU · Trieste, Italy
Meeting website2–4 February 2026
LISA Fundamental Physics and Waveforms Working Groups Meeting
SISSA · Trieste, Italy
Meeting website12–16 January 2026
The Dynamics of Black Hole Mergers and Gravitational Wave Generation
IFPU · Trieste, Italy
Meeting website9–12 December 2025
GWSky Kick-off Meeting
Max Planck Institute for Gravitational Physics (AEI) · Potsdam, Germany
Meeting website17–21 November 2025
EPTA Meeting 2025
SISSA · Trieste, Italy
Meeting website29 September – 3 October 2025
Ultralight dark matter and observable phenomena
IFPU · Trieste, Italy
Meeting website26–30 May 2025
Gravitational Wave Probes of Black Hole Environments
IFPU · Trieste, Italy
Meeting websiteRecent papers
All papers2026-10 · arXiv:2610.12082
Gravitational radiation from a photon on the light ring: multipole fluxes and the logarithmic divergenceE. Barausse
2026-09 · arXiv:2609.05407
Nonlinear evolution in Galileon EFTs: Regularization and screeningF. Thaalba, A. Held, R. Cayuso, T. P. Sotiriou
2026-09 · arXiv:2609.03329
Introducing SINFONIA: Symplectic, slimplectic and Magnusian (Neural) Flows for Orbital Numerical Integration and AccelerationL. J. Gomes Da Silva
2026-07 · arXiv:2607.00845
Environmental effects vs. modified gravity in the LISA massive black hole binary populationL. Copparoni, E. Barausse
Seminars at SISSA
All seminars19 Nov 2026
Gabriele Astorino
Title to be announced
3 Dec 2026
Thomas Apostolidis
Toward the CompactHedron: Bounds on Neutron Stars from Microscopic Principles
8 Oct 2026
Rocco D'Agostino
Nonlocal gravity: from cosmology to astrophysics