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astro-ph.CO2025

Torsion cosmology in the light of DESI, supernovae and CMB observational constraints

Tonghua Liu, Xiaolei Li, Tengpeng Xu +2

In this work, we investigate a torsion-based cosmological model within the Einstei-Cartan framework, constrained by the latest combined datasets including DESI DR2 BAO, PantheonPlu…

astro-ph.CO2025

Advancing Cosmological Parameter Estimation and Hubble Parameter Reconstruction with Long Short-Term Memory and Efficient-Kolmogorov-Arnold Networks

Jiaxing Cui, Marek Biesiada, Ao Liu +3

In this work, we propose a novel approach for cosmological parameter estimation and Hubble parameter reconstruction using Long Short-Term Memory (LSTM) networks and Efficient-Kolmo…

astro-ph.CO2024

Newest measurements of Hubble constant from DESI 2024 BAO observations

Wuzheng Guo, Qiumin Wang, Shuo Cao +6

In this Letter, we use the latest results from the Dark Energy Spectroscopic Instrument (DESI) survey to measure the Hubble constant. Baryon acoustic oscillation (BAO) observations…

astro-ph.CO2024

Model independent calibration for sound horizon combining observations of supernovae and transversal BAO measurements

Tonghua Liu, Xinyi Zhong, Jieci Wang +1

The sound horizon is a key theoretical prediction of the cosmological model that depends on the speed of sound and the rate of expansion in the early universe, before matter and ra…

astro-ph.CO2024

Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO

Tonghua Liu, Shuo Cao, Marek Biesiada +2

In this Letter, we propose a model-independent method to determine the Hubble constant and curvature simultaneously taking advantage of the possibilities of future space-borne grav…