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Predicting the formation of stars, black holes, and gravitational-wave signals with young galaxy clusters

Research Project

Project/Area Number 21K13911
Research Category

Grant-in-Aid for Early-Career Scientists

Allocation TypeMulti-year Fund
Review Section Basic Section 15010:Theoretical studies related to particle-, nuclear-, cosmic ray and astro-physics
Research InstitutionThe University of Tokyo

Principal Investigator

ATA METIN  東京大学, カブリ数物連携宇宙研究機構, 特任研究員 (60836229)

Project Period (FY) 2021-04-01 – 2023-03-31
Project Status Granted (Fiscal Year 2021)
Budget Amount *help
¥2,990,000 (Direct Cost: ¥2,300,000、Indirect Cost: ¥690,000)
Fiscal Year 2022: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2021: ¥2,080,000 (Direct Cost: ¥1,600,000、Indirect Cost: ¥480,000)
KeywordsGravitational waves / Binary black holes / Constrained simulations / Young galaxy clusters
Outline of Research at the Start

As a first step I will run constrained simulations of young galaxy clusters of which I reconstructed the initial conditions in a previous work. The idea is to first use dark matter simulations to show that we can predict the further evolution of these clusters. Once this first project is successfully finished, we will go ahead and run hydrodynamical simulations. These simulations will incorporate star formation models that we will use to predict the formation of binary black holes and gravitational wave. With this work we can improve the physics of star formation by comparing to observations.

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Published: 2021-04-28   Modified: 2021-08-30  

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