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Origin and Magnetization of astronomical Jets

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.

Fields of science (EuroSciVoc)

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Programme(s)

Multi-annual funding programmes that define the EU’s priorities for research and innovation.

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

ERC-COG - Consolidator Grant

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Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

(opens in new window) ERC-2017-COG

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Host institution

BAR ILAN UNIVERSITY
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 1 951 744,00
Address
BAR ILAN UNIVERSITY CAMPUS
52900 Ramat Gan
Israel

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Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 1 951 744,00

Beneficiaries (1)

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