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JetNS SIGNED

Relativistic Jets in Astrophysics -Compact binary mergers, Gamma-Ray Bursts, and Beyond

Total Cost €

EC-Contrib. €

Partnership

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JetNS project word cloud

Explore the words cloud of the JetNS project. It provides you a very rough idea of what is the project "JetNS" about.

seemingly forefront nature surrounding transient mediated puzzles origin compact supernovae theoretical what propagation em sheding timey era interaction listed observations drives mechanism jet astronomy energy mergers grbs neutrino sources unrelated transients gw signal broad constraint sne interact exploding beginning explosions binary first hold goals messenger core decade progress relativistic microphysics shocks media astrophysics base bursts basis lsst rapid ray implications gamma gravitational emerged types sn radiation detected time discovered jets counterparts neutrinos electromagnetic models collapse changed surveys modeling domain waves regular questions light estimates icecube probing ska

Project "JetNS" data sheet

The following table provides information about the project.

Coordinator	TEL AVIV UNIVERSITY Organization address address: RAMAT AVIV city: TEL AVIV postcode: 69978 website: http://www.tau.ac.il/ contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	Israel [IL]
Total cost	1˙981˙250 €
EC max contribution	1˙981˙250 € (100%)
Programme	1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
Code Call	ERC-2018-COG
Funding Scheme	ERC-COG
Starting year	2019
Duration (year-month-day)	from 2019-01-01 to 2023-12-31

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	TEL AVIV UNIVERSITY TEL AVIV UNIVERSITY Organization address address: RAMAT AVIV city: TEL AVIV postcode: 69978 website: http://www.tau.ac.il/ contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	IL (TEL AVIV)	coordinator	1˙981˙250.00

Map

Project objective

What is the origin of the electromagnetic (EM) counterparts of gravitational waves observed from compact binary mergers? What makes short gamma ray bursts (GRBs)? What are the sources of IceCube’s high-energy neutrinos? Are all core-collapse supernovae exploding via the same mechanism? These are some of the puzzles that have emerged with the rapid progress of time domain astronomy. Relativistic jets in compact binary mergers and GRBs, and their interaction with the surrounding media hold the key to these, and other, seemingly unrelated broad-impact questions. Here I propose a new forefront study of how relativistic jets interact with their surrounding media and of its numerous implications, focusing on compact binary mergers and GRBs. The goal of this project is to study, first, the jet-media interaction, and the microphysics of the radiation-mediated shocks that it drives. I will then use the results, together with available observations, to learn about compact binary mergers, GRBs and SNe, sheding light on the questions listed above, and probing the nature of relativistic jets in general. Important goals will include: (i) General models for the propagation of relativistic jets in various media types. (ii) Modeling of the EM signal generated by jet-media interaction following compact binary mergers. (iii) Estimates of the neutrino signal from jet-media interaction in GRBs and SNe. (iv) Constraint the role of jets in SN explosions. This project is timey as it comes at the beginning of a new multi-messenger era where the EM counterparts of GW sources are going to be detected on a regular basis and where the face of transient astrophysics is going to be changed by a range of large scale surveys such as LSST, the SKA, and more. This project will set the theoretical base for understanding numerous known and yet-to be discovered transients that will be detected in the next decade.

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The information about "JETNS" are provided by the European Opendata Portal: CORDIS opendata.