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Unveiling the origins of white-dwarf explosions

Project description

Research delves deeper into white dwarf explosions

The explosive deaths of white dwarfs are essential for heavy element nucleosynthesis, galaxy feedback and binary system evolution. Type Ia supernovae (SNe Ia) help measure cosmological distances and were instrumental in the discovery of the accelerating universe. Recent surveys suggest SNe Ia may not be the only way white dwarfs explode, indicating potential populations of faint, fast-evolving explosions caused by interactions with intermediate-mass black holes, neutron star mergers or triple-system collisions. Funded by the European Research Council, the CosmicLeap project aims to understand these explosions better. By gathering a large sample of white dwarf events, applying machine learning techniques and determining explosion rates in various galaxies, CosmicLeap will elucidate the diversity of these events and their implications for nucleosynthesis, cosmology and future gravitational wave detections.

Objective

The explosive deaths of white dwarfs are essential in heavy element nucleosynthesis, galaxy feedback, and for understanding the evolution of binary systems. Type Ia supernovae (SNe Ia) are famous for their key role as cosmological-distance indicators and in the discovery of the accelerating Universe. Recent high-cadence surveys, and theoretical advances, have hinted that SNe Ia may not be the dominant way in which white dwarfs explode, with the potential existence of large populations of faint and rapidly evolving white-dwarf explosions. These unexplored classes of exotic transients may come from white dwarfs being torn apart by intermediate-mass black holes, mergers with neutron stars, or collisions in triple systems, but the mapping between explosions and observed transients is undetermined.
This project aims at providing the first complete census of the multiple ways that white dwarfs explode by mapping their observations to their explosion physics and constraining their diversity. This sample will be crucial for defining optimal samples of SNe Ia for cosmology, as well as determining the rates and contributions of white-dwarf explosions to the origin of the elements. We will achieve this by i) obtaining the largest ever, rapidly discovered and spectroscopically confirmed sample, of white-dwarf transients with detailed follow-up observations, ii) the application of machine-learning techniques (e.g. neural-network emulators) for rapid comparison to sophisticated explosion models, and iii) the determination of the rates and diversity of their explosions in different galaxy environments. The confirmation and exploration of the multiple explosion channels for producing normal SNe Ia and exotic white-dwarf transients will have major implications for their nucleosynthetic yields, their use in cosmology, as well as predicting rates of double white dwarfs that will be detected in huge numbers in the Milky Way by the gravitational-wave detector, LISA.

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Call for proposal

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(opens in new window) ERC-2023-COG

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Host institution

THE PROVOST, FELLOWS, FOUNDATION SCHOLARS & THE OTHER MEMBERS OF BOARD, OF THE COLLEGE OF THE HOLY & UNDIVIDED TRINITY OF QUEEN ELIZABETH NEAR DUBLIN
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.

€ 1 993 995,00
Address
COLLEGE GREEN TRINITY COLLEGE
D02 CX56 Dublin
Ireland

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Region
Ireland Eastern and Midland Dublin
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.

€ 1 993 995,00

Beneficiaries (1)

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