Dark Matter · Early Universe
Supermassive Dark Stars (SMDSs)
Supermassive dark stars (SMDSs) are luminous stellar objects formed in the early Universe at redshift z~10–20, made primarily of hydrogen and helium, yet powered by dark matter annihilation. Differentiating SMDSs from early galaxies containing zero metallicity stars at similar redshifts requires spectral, photometric, and morphological comparisons.
With only the Roman Space Telescope (RST), differentiation of SMDSs — particularly those formed via adiabatic contraction with M > 105 M☉ and lensed by >100× — is possible due to their distinct photometric signatures from the first galaxies. Those formed via dark matter capture can be differentiated only by image morphology: point object (SMDSs) vs. extended object (sufficiently magnified galaxies).
By additionally employing James Webb Space Telescope (JWST) spectroscopy, we can identify the HeII 1640 absorption line, a “smoking gun” for SMDS detection. Although RST doesn't cover the required wavelength band (for z>10 objects), JWST does, hence the two can be used in tandem to identify SMDSs.
The detection of SMDSs would confirm a new type of star powered by dark matter and may shed light on the origins of the supermassive black holes powering bright quasars observed at z>6.
Research Highlights

Related Papers
Zhang, S., Ilie, C., & Freese, K. (2024). ApJ, 965(2), 121. arXiv:2306.11606★ First Author