Li, B., & Liu, L. (2026). Non-minimally Coupled Running Curvaton for DESI-preferred Dynamical Dark Energy and Hubble Tension.
Style de citation Chicago (17e éd.)Li, Bichu, et Lei-Hua Liu. Non-minimally Coupled Running Curvaton for DESI-preferred Dynamical Dark Energy and Hubble Tension. 2026.
Style de citation MLA (9e éd.)Li, Bichu, et Lei-Hua Liu. Non-minimally Coupled Running Curvaton for DESI-preferred Dynamical Dark Energy and Hubble Tension. 2026.
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