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<jats:title>Abstract</jats:title> <jats:p>The Roman Space Telescope’s Galactic Bulge Time Domain Survey will constitute the most sensitive microlensing survey of the Galactic bulge to date, opening up new opportunities to search for dark matter (DM). Many extensions of the Standard Model predict the formation of <jats:italic>extended</jats:italic> DM substructures, such as DM subhalos, boson/axion stars, and halo-dressed primordial black holes. We demonstrate that for such targets, Roman will be sensitive to a broad parameter space up to 4 orders of magnitude below existing constraints. Our analysis can be readily applied to other extended DM configurations as well.</jats:p>
収録刊行物
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- The Astrophysical Journal Letters
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The Astrophysical Journal Letters 965 (1), L3-, 2024-04-01
American Astronomical Society
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詳細情報 詳細情報について
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- CRID
- 1360584339781535616
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- ISSN
- 20418213
- 20418205
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- 資料種別
- journal article
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- データソース種別
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- Crossref
- KAKEN