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.
Breakthrough 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 about 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.
Novel 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. 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.
Significance
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 |
---|---|---|---|---|
MANUNKIND: Determinants and Dynamics of Collaborative ExploitationThis project aims to develop a game theoretic framework to analyze the psychological and strategic dynamics of collaborative exploitation, informing policies to combat modern slavery. | ERC STG | € 1.497.749 | 2022 | Details |
Elucidating the phenotypic convergence of proliferation reduction under growth-induced pressureThe UnderPressure project aims to investigate how mechanical constraints from 3D crowding affect cell proliferation and signaling in various organisms, with potential applications in reducing cancer chemoresistance. | ERC STG | € 1.498.280 | 2022 | Details |
Uncovering the mechanisms of action of an antiviral bacteriumThis project aims to uncover the mechanisms behind Wolbachia's antiviral protection in insects and develop tools for studying symbiont gene function. | ERC STG | € 1.500.000 | 2023 | Details |
The Ethics of Loneliness and SociabilityThis project aims to develop a normative theory of loneliness by analyzing ethical responsibilities of individuals and societies to prevent and alleviate loneliness, establishing a new philosophical sub-field. | ERC STG | € 1.025.860 | 2023 | Details |
MANUNKIND: Determinants and Dynamics of Collaborative Exploitation
This project aims to develop a game theoretic framework to analyze the psychological and strategic dynamics of collaborative exploitation, informing policies to combat modern slavery.
Elucidating the phenotypic convergence of proliferation reduction under growth-induced pressure
The UnderPressure project aims to investigate how mechanical constraints from 3D crowding affect cell proliferation and signaling in various organisms, with potential applications in reducing cancer chemoresistance.
Uncovering the mechanisms of action of an antiviral bacterium
This project aims to uncover the mechanisms behind Wolbachia's antiviral protection in insects and develop tools for studying symbiont gene function.
The Ethics of Loneliness and Sociability
This project aims to develop a normative theory of loneliness by analyzing ethical responsibilities of individuals and societies to prevent and alleviate loneliness, establishing a new philosophical sub-field.
Vergelijkbare projecten uit andere regelingen
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
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 COG | € 1.997.509 | 2023 | 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 SyG | € 11.260.286 | 2023 | Details |
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 STG | € 1.499.762 | 2023 | Details |
Illuminating neutron stars with radiative plasma physicsThis project aims to develop first-principles 3D models and a simulation toolkit for neutron star radiative plasmas to enhance understanding of their emission mechanisms and improve astrophysical theories. | ERC STG | € 2.211.196 | 2024 | Details |
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.
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.
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.
Illuminating neutron stars with radiative plasma physics
This project aims to develop first-principles 3D models and a simulation toolkit for neutron star radiative plasmas to enhance understanding of their emission mechanisms and improve astrophysical theories.