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Prof. Pau Amaro Seoane (Universitat Politècnica de València)31/03/2026, 10:05
The Galactic Centre contains populations of stellar-mass and
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substellar-mass compact objects orbiting the central black hole,
classified as early extreme-mass ratio inspirals (E-EMRIs) and extremely
large mass ratio inspirals (XMRIs). These systems constitute asymmetric
binaries, characterized by mass ratios exceeding 10,0000 to 1. This mass
differential causes the secondary body to... -
Dr Mai Qiao (ICTP - AP / University Chinese Academy of Sciences)31/03/2026, 11:30
Numerous astrophysical observations indicate the existence of dark matter via gravitational effects, yet its nature remains elusive. Experiments exploring non-gravitational interactions between dark matter and Standard Model (SM) particles include indirect, direct, and collider detection. Meanwhile, gravitational-wave (GW) observations of compact binary coalescences since GW150914 also offer...
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