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O.M.J. SIGNED

Origin and Magnetization of astronomical Jets

Total Cost €

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EC-Contrib. €

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Partnership

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Project "O.M.J." data sheet

The following table provides information about the project.

Coordinator
BAR ILAN UNIVERSITY 

Organization address
address: BAR ILAN UNIVERSITY CAMPUS
city: RAMAT GAN
postcode: 52900
website: www.biu.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˙951˙744 €
 EC max contribution 1˙951˙744 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2017-COG
 Funding Scheme ERC-COG
 Starting year 2018
 Duration (year-month-day) from 2018-10-01   to  2023-09-30

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    BAR ILAN UNIVERSITY IL (RAMAT GAN) coordinator 1˙951˙744.00

Map

 Project objective

The mechanisms by which astronomical jets are launched, as well as their internal properties are fundamental in high-energy astrophysics. It is hypothesized that strong magnetic fields play a key role in the formation and properties of these outflows, seen in many different objects. If this hypothesis is correct, then (i) jets in different objects are likely to have similar properties; and (ii) magnetic fields are crucial in all aspects of jet formation, propagation and particle heating by energy dissipation. This project is aimed at testing these hypotheses, thereby obtaining a deeper insight into the physical processes involved in the formation and properties of jets in different objects, in view of the fact that jets may be the only gravitational wave counterparts expected to be observed in the foreseen future. Building on a decade-long expertise in building unique radiative-transfer codes, I will construct novel algorithms designed to handle radiative processes that occur simultaneously over many different time scales, and implement them in general-relativistic magneto-hydrodynamic (GR-MHD) numerical codes. This will allow, for the first time, the use of observations in constraining the unknown physics of the processes involved. In order to make maximal use of both spectral and temporal data, prime focus will be given to transient objects. I will address (i) possible roles of the mass and spin of the central black hole; (ii) the configuration and strength of the magnetic fields; (iii) the rates of magnetic energy dissipation; (iv) pair production and annihilation in shaping the high energy emission; and (v) constraining uncertain microphysics of plasma heating by non-ideal processes.

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