activity
20222026
most citedGamma ray burst constraints on cosmological models from the improved Amati correlation

40 citations · 217 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.CO2026

Reassessing Evidence for Dark-Sector Interactions with Dynamical Dark Energy and DESI DR2

Jincheng Wang, Hongwei Yu, Puxun Wu

Recent baryon acoustic oscillation measurements from DESI Data Release 2, when combined with CMB and supernova data, strengthen the motivation for exploring departures from CDM…

astro-ph.CO2026

Estimating Cosmological Parameters from Localized Fast Radio Bursts: A Method for Removing Milky Way Dispersion-Measure Contributions

Yuchen Zhang, Yang Liu, Hongwei Yu +1

Fast radio bursts (FRBs) are emerging as powerful probes for cosmology. However, cosmological inference based on FRB dispersion measures (DMs) is limited by uncertainties in the Mi…

gr-qc2026

Primordial Black Holes from Vector-Induced Curvature Perturbations Sourced by Primordial Magnetic Fields

Chang Han, Zu-Cheng Chen, Hongwei Yu +1

Generating an appreciable abundance of primordial black holes (PBHs) requires a substantial enhancement of primordial curvature perturbations on small scales. In this work, we prop…

astro-ph.CO2026

Phantom-Divide Crossing in Exponentially Coupled Quintessence and the Role of Neutrino-Mass Freedom

Jincheng Wang, Hongwei Yu, Puxun Wu

We investigate a quintessence dark-energy model with an exponential potential and an exponential coupling to cold dark matter (CDM), hereafter referred to as the CQ-EXP model, usin…

astro-ph.GA2026

The Steep-spectrum Radio-loud AGN Luminosity Function and Its Implications for Black Hole Growth and Star Formation

Wenjie Wang, Zunli Yuan, B. Šlaus +2

We study the cosmic evolution of radio-loud active galactic nuclei (AGNs) using a beaming-minimized sample of 4{,}555 steep-spectrum sources over , compiled from the…

astro-ph.CO2025

Photon rest mass from localized fast radio bursts with improved distribution of dispersion measure from extragalactic gas

Yuchen Zhang, Yang Liu, Hongwei Yu +1

The assumption that photons are massless is a foundational postulate of modern physics, yet it remains subject to experimental verification. Fast radio bursts (FRBs), with their co…

astro-ph.GA2025

Revisiting the 150 MHz Radio Luminosity Function of Star-Forming Galaxies with LOFAR Deep Fields through a Refined Statistical Framework

Wenjie Wang, Zunli Yuan, Hongwei Yu +3

We present a comprehensive analysis of the 150~MHz radio luminosity function (LF) of star-forming galaxies (SFGs) using deep observations from the LOFAR Two-metre Sky Survey in the…

astro-ph.CO2025★ 11 cited

Revisiting cosmic acceleration with DESI BAO

Jincheng Wang, Hongwei Yu, Puxun Wu

We revisit the evolution of cosmic acceleration in a spatially flat CDM universe, in which the equation of state of dark energy takes the CPL parametrization, using the lat…

astro-ph.CO2025

Primordial Gravitational Waves in Parity-violating Symmetric Teleparallel Gravity

Rongrong Zhai, Chengjie Fu, Xiangyun Fu +2

In this paper, we investigate the inflationary phenomenology of parity-violating (PV) extensions of symmetric teleparallel gravity by applying this PV gravity theory to axion infla…

astro-ph.CO2025

Constraining the Baryon Fraction in Extragalactic Diffuse Ionized Gas with 124 Localized Fast Radio Bursts

Yang Liu, Yuchen Zhang, Jun-Jie Wei +3

Fast radio bursts (FRBs) are increasingly recognized as powerful cosmological tools for constraining the baryon fraction in extragalactic diffuse ionized gas, presenting a promisin…

astro-ph.CO2025

Probability density function for dispersion measure of fast radio burst from extragalactic medium

Yuchen Zhang, Yang Liu, Hongwei Yu +1

Fast Radio Bursts (FRBs) have emerged as powerful probes in cosmology. An optimized method was recently proposed to extract the cosmic baryon density from localized FRBs by maximiz…

gr-qc2025★ 2 cited

Infrared Behavior of Induced Gravitational Waves from Isocurvature Perturbations

Chang Han, Zu-Cheng Chen, Hongwei Yu +1

Induced gravitational waves provide a powerful probe of primordial perturbations in the early universe through their distinctive spectral properties. We analyze the spectral energy…

astro-ph.CO2024★ 20 cited

Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample

Yang Liu, Hongwei Yu, Puxun Wu

We establish a cosmological-model-independent method to extract the apparent magnitude and its derivative at different redshifts from the Pantheon+ type Ia supernova sample, and fi…

astro-ph.CO2024★ 15 cited

Constraints on Cosmological Models from Quasars Calibrated with Type Ia Supernova by a Gaussian Process

Haixiang Zhang, Yang Liu, Hongwei Yu +3

In this paper, we use quasars calibrated from type Ia supernova (SN Ia) to constrain cosmological models. We consider three different X-ray luminosity () - ultraviolet lumin…

gr-qc2024★ 12 cited

Resonant amplification of curvature perturbations in inflation model with periodical derivative coupling

Li-Yang Chen, Hongwei Yu, Puxun Wu

In this paper, we introduce a weak, transient and periodical derivative coupling between the inflaton field and gravity, and find that the square of the sound speed of the curvatur…

astro-ph.CO2024★ 32 cited

NANOGrav hints for first-order confinement-deconfinement phase transition in different QCD-matter scenarios

Zu-Cheng Chen, Shou-Long Li, Puxun Wu +1

Recent observations from several pulsar timing array (PTA) collaborations have unveiled compelling evidence for a stochastic signal in the nanohertz band. This signal aligns remark…

astro-ph.CO2024★ 1 cited

Observations favor the redshift-evolutionary - relation of quasars from copula

Bao Wang, Yang Liu, Hongwei Yu +1

We compare, with data from the quasars, the Hubble parameter measurements, and the Pantheon+ type Ia supernova, three different relations between X-ray luminosity () and ultra…

astro-ph.GA2023

Constraints on cosmic star formation history via a new modeling of the radio luminosity function of star-forming galaxies

Wenjie Wang, Zunli Yuan, Hongwei Yu +1

Radio wavelengths offer a unique possibility to trace the total star-formation rate (SFR) in galaxies, both obscured and unobscured. To probe the dust-unbiased star-formation histo…

gr-qc2023

Power spectrum with growth for primordial black holes

Rongrong Zhai, Hongwei Yu, Puxun Wu

The decrease of both the rolling speed of the inflaton and the sound speed of the curvature perturbations can amplify the curvature perturbations during inflation so as to generate…

astro-ph.CO2023

Probing Cosmic Background Dynamics with a Cosmological-model-independent Method

Yang Liu, Bao Wang, Hongwei Yu +1

The Hubble constant tension has emerged as the most serious crisis in modern cosmology, potentially indicating that the CDM model may not describe our universe accurately.…

gr-qc2022★ 1 cited

Cosmological Complexity from initial thermal state

Jincheng Wang, Hongwei Yu, Puxun Wu

The cosmological scalar perturbations should satisfy the thermal distribution at the beginning of inflation since the cosmic temperature is presumably very high. In this paper, we…

astro-ph.CO2022★ 13 cited

Redshift-evolutionary X-ray and UV luminosity relation of quasars from Gaussian copula

Bao Wang, Yang Liu, Zunli Yuan +3

We construct a three-dimensional and redshift-evolutionary X-ray and ultraviolet () luminosity relation for quasars from the powerful statistic tool called copula, and…

astro-ph.CO2022★ 39 cited

Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements

Yang Liu, Hongwei Yu, Puxun Wu

We establish a cosmological-model-independent method to determine the Hubble constant from the localized fast radio bursts (FRBs) and the Hubble parameter measurements from c…

astro-ph.CO2022★ 40 cited

Gamma ray burst constraints on cosmological models from the improved Amati correlation

Yang Liu, Nan Liang, Xiaoyao Xie +3

An improved Amati correlation was constructed in (ApJ 931 (2022) 50) by us recently. In this paper, we further study constraints on the CDM and CDM models from the gamma ray…