CORDIS Project
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This project focuses on advancing black hole spectroscopy by studying quasinormal modes of black holes. It combines mathematical and numerical relativity to understand how perturbations affect these modes, aiming to enhance the scientific understanding of gravitational waves in astrophysics.
Gravitational Wave (GW) astronomy has emerged as a fundamental field, allowing us to probe gravity in its strongest regime.
Black hole (BH) spectroscopy is a highly effective method for extracting spacetime information from observed GW signals.
The late-time radiation of newly formed black holes is characterized by an exponentially damped, oscillating signal.
Measuring the decaying scales and oscillating frequencies — the so-called quasinormal modes (QNMs) — offers insightful information about t…
KOBENHAVNS UNIVERSITET
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THE UNIVERSITY OF TEXAS SYSTEM
United States, Austin
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
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