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| Funder | Science and Technology Facilities Council |
|---|---|
| Recipient Organization | King's College London |
| Country | United Kingdom |
| Start Date | Sep 30, 2024 |
| End Date | Mar 30, 2028 |
| Duration | 1,277 days |
| Number of Grantees | 2 |
| Roles | Student; Supervisor |
| Data Source | UKRI Gateway to Research |
| Grant ID | 2929476 |
We will study the transient radio signature produced when dark matter clumps known as axion miniclusters encounter neutron stars.
We will statistically model the population of both miniclsuters and neutron stars, based on the latest simulations and observations.
We will study in depth the observational strategies to observe this signal in the proposed "ASTRA" axion radio telescope. We will investigate uncertainties due to early Universe simulations of the axion, and theoretical models. We will investigate other observables related to miniclusters such as in haloscope lineshapes, and in microlensing.
King's College London
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