Observations reveal unique spectral signatures in early galaxies, suggesting dark star formation pathways.
AbstractJWST has unveiled a range of compact, red, line-broadened sources (“little red dots”) along-side a population of unexpectedly luminous galaxies at z ≳ 10. These observations revivequestions about the formation of early massive black-hole seeds and the rapid assembly of met-als and dust. We explore whether supermassive dark stars (SMDSs)—baryonic objects poweredtemporarily by dark-matter annihilation—offer a unified pathway to form ∼ 105 – 107M⊙ black-hole seeds very early on. This scenario predicts distinctive spectral signatures that can be testedwith current and forthcoming JWST data.
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SIKX HILTON (2026) studied this question.
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