27–30 Apr 2026
Palais des papes, Avignon
Europe/Paris timezone

On the origin of dynamical dark energy in cosmographic parameters

30 Apr 2026, 15:40
10m
Chambre du Trésorier (Palais des papes, Avignon)

Chambre du Trésorier

Palais des papes, Avignon

Speaker

Maurice van putten (Sejong University)

Description

A dynamical dark energy is derived from the scaling dimension two in UVIR-consistency between a bare cosmological constant with Big Bang cosmologies. The resulting Hubble expansion predicts the Hubble constant H0 to be $\sqrt{6/5}$ times the H0 in Planck-$\Lambda$CDM analysis of the CMB. Expressed equivalently in $w(a)$CDM, this new Hubble expansion predicts a phantom crossing at redshift $z=1.9$ coincident with the peak in the cosmic star-formation rate and galaxy mergers. [Based, in part, on van Putten, 2025, JHEAP Lett, 45, 195.]

Author

Maurice van putten (Sejong University)

Presentation materials