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Talk1 h 14 min

Gravitational-wave emission from binary systems of compact objects

Luciano Rezzolla · CERN

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About

Binary systems comprising black holes and or neutron stars represent the strongest sources of gravitational waves and have recently been revealed by detectors such as LIGO and Virgo. In this series of lectures I will provide a brief introduction to the mathematical and numerical techniques that are needed for the theoretical modelling of these systems. At the same time, I will discuss how neutron-star binaries represent fantastic tools to explore fundamental aspects of gravitational and particle physics. In particular, I will provide a few examples of the ways in which neutron stars can be used to explore fundamental physics, ranging from their spectral properties, the possibility of phase transition to quark matter, the amplification of super-strong magnetic fields, and the copious emission of neutrinos.

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The talk

  1. Gravitational-wave emission from binary systems of compact objects 2025-06-02 · 1 h 14 min · CERN's player

Credits and licence

Institution
CERN
Department
Academic Training Lecture Regular Programme,2024-2025
Speaker
Luciano Rezzolla
Year
2025
Level
Graduate
Language
English
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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