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Decoding Dark Matter with Stellar Streams from Beyond the Milky Way

Project description

Decoding dark matter through stellar streams

Understanding dark matter, which makes up 80 % of the Universe’s matter, remains one of astrophysics’ greatest challenges. Stellar streams, formed by disrupted star clusters and galaxies, hold vital clues to the distribution and behaviour of dark matter. These streams are influenced by dark matter’s mass, shape, and interaction properties, yet their full potential remains untapped. With a flood of data from cutting-edge observatories such as the Vera C. Rubin Observatory, Euclid, and the Nancy Grace Roman Space Telescope, researchers are poised to revolutionise the field. The ERC-funded BeyondSTREAMS project will harness these data to create novel statistical models and simulations, transforming stellar stream analysis. By comparing observations with predictions, it will refine our understanding of particle physics.

Objective

One of the key questions driving astrophysics research today is the nature of dark matter, which comprises 80% of the matter in the Universe. Stellar streams are sensitive to the distribution of dark matter and to the population of dark matter subhalos in galaxies, both of which depend on the mass and interactions of the dark matter particle. My proposed work will use the wealth of incoming stellar stream data materializing over the next five years from the Nancy Grace Roman Space Telescope, the Vera C. Rubin Observatory, and the Euclid Space Telescope to measure dark matter halo masses, shapes and concentrations, as well as subhalo populations of external galaxies. I will lead a fundamental shift in the approach to stellar stream studies through statistical model-to-data comparisons between theoretical predictions from various dark matter candidates (cold, warm, wave-like, self-interacting) and the actual stream data. To achieve this goal, I will develop novel numerical techniques which model and fit multiple streams at once in multiple external galaxies, run state-of-the-art N-body simulations of disrupting globular clusters in dwarf galaxies to place theoretical constraints on the expected substructure, and carry out statistical comparisons between dark matter models and properties derived from the stellar stream data. I will rule out dark matter candidates that are inconsistent with the new stellar stream data, and by the end of the 60-month grant period, I will have the world-leading constraints on dark matter from stellar streams. This work provides an innovative method for mapping the otherwise invisible dark matter, and will constrain statistical properties of dark matter related to its nature and possible extensions of the standard model of particle physics.

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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-2023-STG

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Host institution

KOBENHAVNS UNIVERSITET
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.

€ 1 686 734,00
Address
NORREGADE 10
1165 KOBENHAVN
Denmark

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Region
Danmark Hovedstaden Byen København
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.

€ 1 686 734,00

Beneficiaries (1)

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