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.
Projectdetails
Introduction
Recent years have seen the blossoming of multi-messenger astrophysics where gravitational waves, photons, and neutrinos provide complementary views on cosmic explosions involving some of the Universe’s most enigmatic objects, namely neutron stars and black holes.
Significant Observations
The first observation of a neutron star merger via both gravitational waves and, days later, an electromagnetic flash called "kilonova" enabled huge scientific leaps forward and was therefore celebrated as "2017 Breakthrough of the Year".
Potential of Multi-Messenger Astrophysics
Multi-messenger astrophysics has enormous potential to solve many longstanding puzzles such as:
- The origin of the heaviest elements
- The nature of the densest matter in the Universe
This potential is contingent upon our understanding of how the different messengers are physically connected.
Challenges in Current Understanding
The gravitational wave and electromagnetic emission stages, however, involve vastly different length and time scales and completely different physical processes. Therefore, currently strong assumptions need to be made regarding how both stages are actually physically connected.
Proposed Research
On the verge of this transformational era of physics, I propose to calculate for the first time the evolution from the inspiral (milliseconds before the merger) to the time after the kilonova (months later) within a common simulation framework.
Methodology
This will become possible via the novel computational methodology that I have recently developed: the world-wide first Lagrangian hydrodynamics code that also consistently solves Einstein's equations.
Advantages of New Development
Compared to conventional Numerical Relativity codes, my new development has major advantages in evolving the merger ejecta which finally cause the kilonova.
Expected Outcomes
This project will provide for the first time detailed physical structures of neutron star merger remnants and the first one-to-one mapping between the physics of the merger and the gravitational wave, neutrino, and electromagnetic signals.
Conclusion
This will present a major breakthrough for both the nuclear astrophysics and the multi-messenger communities.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 2.499.675 |
Totale projectbegroting | € 2.499.675 |
Tijdlijn
Startdatum | 1-10-2022 |
Einddatum | 30-9-2027 |
Subsidiejaar | 2022 |
Partners & Locaties
Projectpartners
- UNIVERSITY OF HAMBURGpenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
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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 |
Modeling binary neutron star from inspirals to remnants and their multimessenger emissionsInspiReM 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. | ERC Consolid... | € 1.997.509 | 2023 | 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 |
How Neutron Star Mergers make Heavy ElementsThe HEAVYMETAL project aims to analyze kilonovae from neutron star mergers to uncover nucleosynthesis pathways and the properties of heavy elements and high-density matter. | ERC Synergy ... | € 11.260.286 | 2023 | 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 |
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.
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.
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.
How Neutron Star Mergers make Heavy Elements
The HEAVYMETAL project aims to analyze kilonovae from neutron star mergers to uncover nucleosynthesis pathways and the properties of heavy elements and high-density matter.
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.