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Alleviating H₀ and S₈ Tensions Simultaneously in K-essence Cosmology
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Alleviating H₀ and S₈ Tensions Simultaneously in K-essence Cosmology
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The present work begins by examining the early-Universe inflationary epoch of a special K-essence model, which incorporates a linear coupling term between the scalar field potential and the canonical Lagrangian. For the power law potential, we both numerically and analytically prove that the inflationary parameters such as the spectral index and tensor-to-scalar ratio are compatible with the recent BICEP/Keck observations. Continuing this work, our analysis based on comparing early-Universe observations with late-Universe measurements indicates that the tension on the Hubble parameter $H_0$ and the growth of structure parameter $S_8$ can be alleviated simultaneously. More precisely, compared to the standard $\Lambda$CDM model, our model can reduce $H_0$ tension to roughly $2.2 \sigma$ and the $S_8$ discrepancy diminishes to $0.82\sigma$.
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Cited by 1 Pith paper
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Hubble tension in k-essence: Evidence for robust tension alleviation
Dilaton and tachyon k-essence models robustly reduce Planck–late-Universe H0 tension to 0.14σ and 0.69σ without dataset-dependent fine-tuning of model parameters.
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