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    Blue-tilted spectral running and the JWST early galaxy tension

    Mikage U. Kobayashi1,2, Gen Chiaki3, Kazutaka Kimura4, Kazuyuki Akitsu2, Kazunori Kohri5,6,2,7, Tomo Takahashi8, and Kazuyuki Omukai4

    Phys. Rev. D 114, 063537 – Published 21 September, 2026

    DOI: https://doi.org/10.1103/f18k-xmxm

    Abstract

    Recently, the James Webb Space Telescope (JWST) Collaboration has found the unexpectedly large abundance of massive galaxies with stellar masses of ∼1010M⊙ at high redshifts z≃6.5–9 compared with the prediction of the standard lambda cold dark matter (ΛCDM) model. As a possible solution to the tension, we consider a blue-tilted spectrum of density perturbations with a positive running. We find that, for αs≃0.02 and βs≃0.02, a joint analysis with CMB observations shows that the tension can be resolved at the 1σ confidence level. Such a blue-tilted spectrum is also plausible from the perspective for formations of primordial black holes on much smaller scales in the early Universe.

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