Unleashing the predictive power of tidal disruption events
This project aims to advance the understanding of tidal disruption events by developing a new computational approach to simulate emission, enabling analysis of supermassive black holes and their environments.
Projectdetails
Introduction
Tidal disruption events (TDEs) have been known for decades as unique probes of otherwise quiescent supermassive black holes and their environment, in a mass range inaccessible by any other techniques. However, fulfilling this potential has so far been hindered by a crucial lack of understanding of the physics causing the emission. My program will solve this theoretical bottleneck and unleash the predictive power of TDEs at the dawn of an observational golden era provided by the Rubin Observatory.
Understanding TDEs
A TDE occurs when a star is disrupted by a black hole, after which the stellar debris fuels the compact object, generating the detectable signal. While characterizing this emission has been prevented by the impossibility of simulating the entire gas evolution, I am pioneering a new computational approach that solves this long-standing impediment by dividing the evolution into interconnected phases.
Computational Approach
Relying on this technique, I will deliver the first paradigm for the TDE emission based on first-principles simulations.
Theoretical Lightcurves
Using this new knowledge, I will build theoretical lightcurves that directly depend on astrophysical system parameters, namely the black hole and stellar properties. Additionally, I will develop the first physically sound analysis toolkit for detected TDEs, which statistically compares these lightcurves to observed ones to infer system parameters.
Implications for Astrophysics
Applying this toolkit to the wealth of upcoming TDE detections, I will shed new light on some of the most pressing mysteries in astrophysics, including:
- The formation and growth of supermassive black holes
- The properties and interactions between the stars orbiting them
- The processes leading to relativistic jets and neutrino production
Conclusion
My ambitious research program is designed to capitalize on the observational revolution brought about by the Rubin Observatory, setting the foundations for TDE science in the decade to come with far-reaching implications across fields from galaxy evolution to high-energy astrophysics.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 1.499.853 |
Totale projectbegroting | € 1.499.853 |
Tijdlijn
Startdatum | 1-11-2024 |
Einddatum | 31-10-2029 |
Subsidiejaar | 2024 |
Partners & Locaties
Projectpartners
- THE UNIVERSITY OF BIRMINGHAMpenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
Tidal Disruption Events: A New Black Hole CensusThis project aims to utilize tidal disruption events as reliable probes to derive parameters of massive black holes through first-principles simulations and models, enhancing our understanding of their origins and growth. | ERC Consolid... | € 1.998.750 | 2024 | Details |
Black holes: gravitational engines of discoveryThe project aims to explore black holes and compact binaries through gravitational-wave and electromagnetic observations to advance understanding of strong gravity and fundamental physics. | ERC Advanced... | € 1.944.825 | 2022 | Details |
Probing cosmic large-scale structure beyond the averageThis project aims to explore fundamental physics beyond the standard model using the Euclid galaxy survey and advanced statistical methods to analyze cosmic structures and dark matter dynamics. | ERC Starting... | € 1.496.955 | 2024 | Details |
Relativistic Jets in the Multimessenger EraThis project aims to enhance the detection and understanding of gravitational wave signals from relativistic jets in multimessenger astronomy, focusing on their implications in various cosmic events. | ERC Advanced... | € 2.498.750 | 2022 | Details |
Decoding Dark Matter with Stellar Streams from Beyond the Milky WayThis project aims to analyze stellar stream data from upcoming telescopes to constrain dark matter properties and rule out inconsistent candidates through innovative statistical modeling techniques. | ERC Starting... | € 1.686.734 | 2024 | Details |
Tidal Disruption Events: A New Black Hole Census
This project aims to utilize tidal disruption events as reliable probes to derive parameters of massive black holes through first-principles simulations and models, enhancing our understanding of their origins and growth.
Black holes: gravitational engines of discovery
The project aims to explore black holes and compact binaries through gravitational-wave and electromagnetic observations to advance understanding of strong gravity and fundamental physics.
Probing cosmic large-scale structure beyond the average
This project aims to explore fundamental physics beyond the standard model using the Euclid galaxy survey and advanced statistical methods to analyze cosmic structures and dark matter dynamics.
Relativistic Jets in the Multimessenger Era
This project aims to enhance the detection and understanding of gravitational wave signals from relativistic jets in multimessenger astronomy, focusing on their implications in various cosmic events.
Decoding Dark Matter with Stellar Streams from Beyond the Milky Way
This project aims to analyze stellar stream data from upcoming telescopes to constrain dark matter properties and rule out inconsistent candidates through innovative statistical modeling techniques.