collaborators

8 papers

astro-ph.CO2026

Cosmological constraints on the big bang quantum cosmology model

Yicheng Wang, Yupeng Yang, Xinyi Dai +3

The big bang quantum cosmology model introduces the trace of the Schouten tensor as a form of dynamic dark energy. Together with cold dark matter, these components form the so-…

astro-ph.CO2026

Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model

Xinyi Dai, Yupeng Yang, Yicheng Wang +3

We develop a modified interacting dark energy (IDE) model to study the redshift evolution of the Hubble constant (), in light of the Hubble tension. In this framework, the ene…

astro-ph.HE2025

Evidence of young magnetars in massive binary embedded in a supernova remnant as sources of active fast radio bursts

F. Y. Wang, H. T. Lan, Z. Y. Zhao +5

Fast radio bursts (FRBs) are intense pulses with unknown origins. A subclass of repeating FRBs show some common features, such as associated compact persistent radio sources (PRSs)…

astro-ph.CO2025

The Hubble Tension resolved by the DESI Baryon Acoustic Oscillations Measurements

X. D. Jia, J. P. Hu, D. H. Gao +2

The cold dark matter (CDM) cosmological model provides a good description of a wide range of astrophysical and cosmological observations. However, severe challenges to the…

astro-ph.GA2025

Calibrating relation using host galaxies of FRBs

Rui-Nan Li, Ke Xu, Dao-Hong Gao +3

Fast radio bursts (FRBs) are extragalactic radio transients that offer valuable insight of intergalactic medium (IGM). However, the dispersion measure (DM) contributed by IGM ($\rm…

astro-ph.CO2025

Measuring Hubble constant using localized and unlocalized fast radio bursts

D. H. Gao, Q. Wu, J. P. Hu +4

The Hubble constant () is one of the most important parameters in the standard model. The measurements given by the main two methods show a gap larger than ,…