CM2talk#357

Reconstructing Dark Energy

Current status of the H_0 and growth tensions: theoretical models and model-independent constraints

作者

Arman ShafielooKorea Astronomy and Space Science Institute

Reconstructing the expansion history of the universe and properties of dark energy have been among the main goals of physical cosmology. I will discuss about reconstructing dark energy in light of most recent cosmological observations including DESI-2024 BAO observations, Union3 supernova compilation and Planck CMB data.

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