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EuroFlash: exploring the origins of fast radio bursts using a network of European radio telescopes

Project description

Understanding the relations between repeating and one-off FRBs

Fast radio bursts (FRBs) constitute a captivating astronomical phenomenon that has long captured the interest of the scientific community. The extraordinary energy density and laser-like coherent radio emissions required for their manifestation have sparked considerable intrigue regarding their origins. This fascination has spurred significant advancements. In this context, the ERC-funded EuroFlash project will establish a European radio telescope network dedicated to conducting a systematic investigation aimed at understanding the distinctions and correlations between repeating and singular FRBs. Additionally, the project aims to enhance sensitivity and observation frequency to refine localisations and discover new sources of FRBs and other astronomical phenomena.

Objective

Fast radio bursts (FRBs) present astronomers with a compelling mystery: what is creating these brilliant but ephemeral flashes that travel billions of lightyears before reaching Earth? Whatever is producing the FRBs, it requires an extreme energy density and the conditions for `laser-like’ coherent radio emission to be generated. While recent discoveries show that magnetars are a leading contender, the heterogeneous properties of the known FRB sample strongly suggest that there are multiple FRB source types. If so, then we have multiple mysterious FRB origins to uncover.

Due to the great interest in solving this puzzle, enormous progress has been made in recent years. There are now hundreds of known FRB sources, dozens of which repeat, and some of which have been localised to their exact galactic neighbourhoods. The FRB sample continues to grow at a rapid pace of several new sources per day, thanks to new wide-field radio telescopes. Studying these sources with dedicated follow-up is challenging because they emit sporadically and are only visible for milliseconds or less. At the same time, by casting an even wider net we are likely to discover new types of FRB-like signals.

With EuroFlash, I will create a coordinated network of European radio telescopes operating over a broad range of radio frequencies, providing high sensitivity and observing cadence, and achieving the best-possible localisations. I will use this network to perform a world-leading, systematic study of repeating FRBs, to understand their progenitor(s) and their relation to the apparently one-off FRB sources. I will also make a novel exploration of the parameter space of short-duration radio transients by exploiting the large field-of-view of LOFAR2.0 and commensal observations to find new sources. In doing so, I aim to discover new types of astrophysical phenomena that probe the extremes of the Universe.

Keywords

Project’s keywords as indicated by the project coordinator. Not to be confused with the EuroSciVoc taxonomy (Fields of science)

Programme(s)

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Topic(s)

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Funding Scheme

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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-2022-ADG

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Host institution

STICHTING NEDERLANDSE WETENSCHAPPELIJK ONDERZOEK INSTITUTEN
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.

€ 2 184 932,50
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.

€ 2 184 932,50

Beneficiaries (2)

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