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Black hole dynamics and the origin of supermassive black holes

Every massive galaxy in the Universe contains a supermassive black hole in the center, which has grown from a smaller black hole, a so called seed black hole. Galaxies must have acquired their seed black holes in the early Univers... see more

31/05/2026

NUIM

216K€

Project Budget: 216K€

Project leader

NATIONAL UNIVERSITY OF IRELAND MAYNOOTH No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

PARTICIPATION DEPralty Sin fecha límite de participación.

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Financing granted El organismo HORIZON EUROPE notifico la concesión del proyecto The day 2023-03-14

HORIZON-MSCA-2022-PF-01-01: MSCA Postdoctoral Fellowships 2022 Expected Outcome:

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Este proyecto no cuenta con búsquedas de partenariado abiertas en este momento.

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No hay información privada compartida para este proyecto. Habla con el coordinador.

2 Participantes

NUIM

215.53K€ | Leader

INAF

N.D. | participant

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Project duration: 38 months Date Start: 2023-03-14
End date: 2026-05-31

Project leader

NATIONAL UNIVERSITY OF IRELAND MAYNOOTH No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Project Budget 216K€

participation deadline Sin fecha límite de participación.

Project description Every massive galaxy in the Universe contains a supermassive black hole in the center, which has grown from a smaller black hole, a so called seed black hole. Galaxies must have acquired their seed black holes in the early Universe, to allow for the observed long coevolution between black holes and galaxies, but recent research has shown that the dynamics of seed black holes in early galaxies are complex, and that seed black holes struggle to find their way to the center of future host galaxies. For this project, I propose the first large-scale study of seed black hole dynamics in the early Universe. I will use my extensive expertise in numerical simulations to design a high-resolution simulation able to fully resolves seed black hole trajectories. From this simulation, I will create the first large-scale catalogue of high-redshift black hole seed dynamics for different black hole formation models. I will use this unique dataset to understand galaxy seeding, determine the relative importance of different seed formation mechanisms and make observational predictions for the James-Webb Space Telescope (JWST) and Laser Interferometer Space Antenna (LISA). These upcoming major observational campaigns will soon provide an unprecedented wealth of observational data on black holes and their host galaxies in the early Universe, making the proposed project extremely timely. With this work, I will challenge the standard paradigm of rapid seed black hole delivery, and lead the way towards a paradigm shift in our understanding of the origin of supermassive black holes.

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