Modeling binary neutron star from inspirals to remnants and their multimessenger emissions
InspiReM aims to enhance theoretical modeling of binary neutron star mergers using advanced simulations to connect gravitational and electromagnetic signals for groundbreaking discoveries in multimessenger astronomy.
Projectdetails
Introduction
Binary neutron star mergers (BNSMs) are unique astrophysical laboratories to explore all four fundamental interactions in their extreme regimes. The landmark detection of the gravitational wave GW170817 and its counterparts in the entire electromagnetic spectrum demonstrated the enormous impact of BNSM observations on fundamental physics and astrophysics, including the nature of matter at supranuclear densities, the origin of high-energy cosmic photons, and the formation of heavy elements.
Project Goals
The goal of InspiReM is to break new ground in the theoretical modeling of BNSMs and to deliver first-principles models linking the source dynamics to the observed radiations. The programme timely addresses central open problems in the modeling of the different coalescence phases with a novel, comprehensive, general-relativistic, (3+1)D and multiscale approach.
Methodology
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Simulations and Analytical Methods: Simulations and analytical relativity methods are combined to deliver full-spectrum gravitational-wave templates for unbiased, high-precision measurements in gravitational-wave astronomy.
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Postmerger Investigations: Merger remnants and outflows are investigated on uncharted postmerger timescales, including, for the first time, all the relevant processes from the four interactions.
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Secular Evolution Exploration: The self-consistent secular evolution of the outflows up to days and years is further explored to directly connect the strong-gravity engine to the electromagnetic emission.
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Bayesian Approaches: Bayesian approaches with simulation-driven models are developed for the joint analyses of gravitational and electromagnetic signals.
Team Expertise
InspiReM leverages recent breakthroughs and the unique interdisciplinary expertise of my team on all aspects of the research. The project also develops novel techniques for exascale parallel computations in relativistic astrophysics.
Expected Impact
If successful, InspiReM will shape the rising field of multimessenger astronomy and drive new groundbreaking discoveries in the related fields.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 1.997.509 |
Totale projectbegroting | € 1.997.509 |
Tijdlijn
Startdatum | 1-4-2023 |
Einddatum | 31-3-2028 |
Subsidiejaar | 2023 |
Partners & Locaties
Projectpartners
- FRIEDRICH-SCHILLER-UNIVERSITÄT JENApenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
From Subatomic to Cosmic Scales: Simulating, Modelling, Analysing Binary Neutron Star MergersThe project aims to develop theoretical models for binary neutron star mergers to enhance the accuracy of multi-messenger observations, enabling insights into matter at supranuclear densities and the expansion rate of the Universe. | ERC Starting... | € 1.499.762 | 2023 | Details |
From inspiral to kilonovaThis project aims to develop a novel simulation framework to connect neutron star merger dynamics with multi-messenger signals, enhancing our understanding of cosmic events and their aftermath. | ERC Advanced... | € 2.499.675 | 2022 | Details |
Dynamical Formation of Black Hole MergersThis ERC research program aims to advance gravitational wave astrophysics by developing tools and methods to investigate binary black hole mergers and their formation in dense stellar environments. | ERC Starting... | € 1.919.186 | 2022 | 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 |
Holography in the Gravitational Wave EraThis project aims to enhance understanding of quantum matter and gravity through holography, focusing on cosmological phase transitions, neutron star mergers, and spacetime singularities. | ERC Advanced... | € 2.499.451 | 2025 | Details |
From Subatomic to Cosmic Scales: Simulating, Modelling, Analysing Binary Neutron Star Mergers
The project aims to develop theoretical models for binary neutron star mergers to enhance the accuracy of multi-messenger observations, enabling insights into matter at supranuclear densities and the expansion rate of the Universe.
From inspiral to kilonova
This project aims to develop a novel simulation framework to connect neutron star merger dynamics with multi-messenger signals, enhancing our understanding of cosmic events and their aftermath.
Dynamical Formation of Black Hole Mergers
This ERC research program aims to advance gravitational wave astrophysics by developing tools and methods to investigate binary black hole mergers and their formation in dense stellar environments.
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.
Holography in the Gravitational Wave Era
This project aims to enhance understanding of quantum matter and gravity through holography, focusing on cosmological phase transitions, neutron star mergers, and spacetime singularities.