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.
Projectdetails
Introduction
The birth of multimessenger Astronomy is unfolding in front of our eyes, largely thanks to incredible observational developments. The new observations challenge theory on numerous frontiers and my goal is to address some of those and to open others.
Relativistic Jets
Relativistic jets are the classical multimessenger sources, typically dominating the observed signature of the objects that launch them. Relativistic jets even have their own gravitational waves signature, Jet-GW, that arises from the jet acceleration.
Jet-GW Significance
This signal, largely ignored so far, is a memory type wave that enables us to “see” directly the jet launching process, and is probably the only way to do so. Detection of Jet-GWs is extremely challenging and they may be easily missed if they are not looked for.
Research Goals
In this program, I aim to achieve the understanding of these signals essential for their detection. In addition, I propose to explore observational implications of relativistic jets as they are manifested in:
- Binary neutron star mergers (BNS)
- Gamma-ray bursts (GRBs)
- A subpopulation of supernovae (SNe) that harbor hidden jets
- Tidal disruption events (TDEs)
Methodology
I will study the basic physics involved, carry out large scale simulations, and probe new observational results. I will focus on new physics, for example, photodissociation of heavy nuclei during jet propagation within BNS ejecta, that hasn’t been considered so far.
Tidal Disruption Events
Powerful jets appear in some TDEs, but not in others. This makes TDEs natural laboratories to pursue the major open question: under which conditions are powerful jets launched?
Commonalities Among Events
Although BNS, GRBs, SNe, and TDEs appear to be very different, their jets have a lot in common. Understanding them requires analysis of the same basic physics and application of similar numerical tools.
Conclusion
This joint study that breaks artificial conceptual barriers will be highly beneficial and fruitful.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 2.498.750 |
Totale projectbegroting | € 2.498.750 |
Tijdlijn
Startdatum | 1-10-2022 |
Einddatum | 30-9-2027 |
Subsidiejaar | 2022 |
Partners & Locaties
Projectpartners
- THE HEBREW UNIVERSITY OF JERUSALEMpenvoerder
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
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 |
Multi-messenger Studies of Extragalactic Super-collidersThis project aims to explore proton acceleration, jet formation, and neutrino production in active galactic nuclei using multi-messenger observations to enhance our understanding of extreme cosmic energy processes. | ERC Advanced... | € 2.799.989 | 2025 | 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 |
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 |
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 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.
Multi-messenger Studies of Extragalactic Super-colliders
This project aims to explore proton acceleration, jet formation, and neutrino production in active galactic nuclei using multi-messenger observations to enhance our understanding of extreme cosmic energy processes.
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.
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.
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.