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Particle composition in relativistic jets

Project description

Determining particle composition of relativistic jets

Relativistic jets from supermassive black holes are highly energetic phenomena that play a crucial role in galaxy evolution. Their composition (electron-positron pairs, electron-proton plasma, or a mixture) affects their power and emissions, with hadronic jets potentially serving as sources of the highest-energy cosmic rays. Circular polarisation is the only reliable method for determining their composition. The ERC-funded PARTICLES project will conduct high-cadence, multifrequency radio observations of relativistic jets, measuring total intensity, linear polarisation, and circular polarisation to clarify their particle makeup. It will also employ very long baseline interferometry to link light curves with the jets’ spatial structures. The project aims to determine the precise particle composition of these jets.

Objective

Relativistic jets launched by supermassive black holes are the most extreme and energetic persistent phenomena in the Universe. They are capable of accelerating particles to energies inaccessible by particle accelerators on Earth, and deposit enormous amount of energy in their surroundings during their lifetime. They are believed to have a significant impact on galaxy evolution via feedback mechanisms. Yet, despite decades of studies, one of the most fundamental properties, the composition of these jets is still unknown. The jets can consist of either electron-positron pairs, electron-proton plasma where also protons are present and accelerated, or an admixture of the two. The composition affects the power of the jet and the presence or lack of hadrons is a crucial ingredient in modelling the multi-wavelength and multi-messenger emission of these jets. If the jets are hadronic, they are likely the origin of the highest energy cosmic rays.

Circular polarization is the only direct way to determine the particle composition of jets, and we have designed a project that will overcome limitations of previous programs to finally resolve the particle composition of relativistic jets. Previously, this has only been attempted on individual objects at low radio frequencies, or using single-frequency data lacking the required discriminating power. PARTICLES will deliver the first multifrequency-radio high-cadence observations of relativistic jets in total intensity, linear, and circular polarization for a sample of objects. In parallel, we will conduct very long baseline interferometry observations to connect our light curves with the spatially resolved structures in the jets. This unprecedented dataset will be combined with radiative transfer simulations, crucial for modelling the origin of circular polarization. These advances will enable us to answer one of the most central questions related to relativistic jets, what is their particle composition?

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Topic(s)

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HORIZON-ERC - HORIZON ERC Grants

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Call for proposal

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(opens in new window) ERC-2024-COG

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Host institution

AALTO KORKEAKOULUSAATIO SR
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.

€ 2 357 623,00
Address
OTAKAARI 1
02150 Espoo
Finland

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Region
Manner-Suomi Helsinki-Uusimaa Helsinki-Uusimaa
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.

€ 2 357 623,00

Beneficiaries (1)

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