activity
20132026
most citedGalactic cosmic-ray model in the light of AMS-02 nuclei data

28 citations · 283 across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.SR2026

Pulsation harmonics reveal the origin of the century-old Blazhko effect

Jia-Shu Niu

The Blazhko effect -- a quasi-periodic modulation of pulsation amplitude and phase observed in all subtypes of RR Lyrae stars -- has defied physical explanation for over a century.…

astro-ph.SR2026

Harmonics as a Hidden Window into the Turbulent Convective Envelope of non-Blazhko RRab Stars

Jia-Shu Niu

Harmonics in pulsating stars have traditionally been regarded as mere Fourier artifacts, fully determined by their parent mode. Recent observations of high-amplitude Scuti star…

astro-ph.SR2026

BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion

Jia-Shu Niu, Ying Zhang, Hui-Fang Xue

We report the discovery of an exceptionally eccentric binary system, BE Lyncis (BE Lyn), which might host a compact companion with mass . By combining TESS p…

astro-ph.SR2025★ 4 cited

Discovery of resonating integration modes in triple-mode high-amplitude Scuti stars: A new evolutionary phase indicator

Jia-Shu Niu, Hui-Fang Xue

High-amplitude Scuti stars (HADS) that pulsate in their first three radial modes are rare in current samples. Here, we analyse five such triple-mode HADS observed by the Transi…

astro-ph.SR2025

Period Variation Rates of Four Radial Single-Mode High-Amplitude Delta Scuti Stars

Tian-Fang Ma, Jia-Shu Niu, Hui-Fang Xue

In this work, we present a study on the long time-scale period variations of four single-mode high-amplitude delta Scuti stars (HADS) via the classical analysis. The target H…

hep-ph2024

Exploring the Dark Frontier: White Dwarf-Based Constraints on Light Dark Matter

Jia-Shu Niu

In the vast expanse of our galaxy, white dwarfs (WDs) are natural sentinels, capturing the enigmatic dark matter (DM) particles that incessantly traverse their interiors. These cel…

astro-ph.SR2024★ 2 cited

Exploring the unexpected: Disharmonized harmonic pulsation modes in high-amplitude Scuti stars

Hui-Fang Xue, Jia-Shu Niu

Harmonics are a ubiquitous feature across various pulsating stars. They are traditionally viewed as mere replicas of the independent primary pulsation modes and have thus been excl…

hep-ex2024

Calibration of the Cryogenic Measurement System of a Resonant Haloscope Cavity

Dong He, Jie Fan, Xin Gao +23

Possible light bosonic dark matter interactions with the Standard Model photon have been searched by microwave resonant cavities. In this paper, we demonstrate the cryogenic readou…

hep-ex2024★ 9 cited

Dark photon constraints from a 7.139 GHz cavity haloscope experiment

Dong He, Jie Fan, Xin Gao +23

The dark photon is a promising candidate for the dark matter which comprises most of the matter in our visible Universe. Via kinetic mixing with the Standard Model it can also be r…

hep-ph2024★ 1 cited

Possible Dark Matter Signals from White Dwarfs

Jia-Shu Niu, Hui-Fang Xue

In our galaxy, the white dwarfs (WDs) will inevitably capture the dark matter (DM) particles streaming through them, if there exist interactions between DM particles and nuclei/ele…

astro-ph.SR2023★ 14 cited

Unveiling the Intricate Symphony of Nonlinear Pulsation Mode Interactions in High-Amplitude Scuti Stars

Jia-Shu Niu, Hui-Fang Xue

People can diagnose the interiors of stars by sensing their pulsations. Pulsation modes, which are determined by the internal state and structure of a star, are typically considere…

astro-ph.SR2023★ 12 cited

Pulsation Analysis of High-Amplitude Scuti Stars with TESS

Wangjunting Xue, Jia-Shu Niu, Hui-Fang Xue +1

In this work, the pulsation analysis is performed on 83 high-amplitude Scuti stars, which have been observed by the Transiting Exoplanet Survey Satellite (TESS). The results sh…

astro-ph.SR2023★ 6 cited

Uncorrelated Amplitude and Frequency Variations of the Harmonics in SX Phoenicis Star XX Cygni

Jia-Shu Niu, Yue Liu, Hui-Fang Xue

Harmonics are quite common in pulsating stars, and they are always considered to mimic the behaviors of their independent parent pulsation modes and not taken as the key informatio…

astro-ph.HE2022★ 1 cited

Quantitative study of the hardening in the Alpha Magnetic Spectrometer nuclei spectra at a few hundred GV

Jia-Shu Niu, Jing Liu

The most significant feature in the cosmic-ray (CR) nuclei spectra is the spectral hardening at a few hundred GV. It is important to know whether the hardening of different nuclei…

astro-ph.SR2022★ 11 cited

Precise Evolutionary Asteroseismology of High-Amplitude δ Scuti Star AE Ursae Majoris

Hui-Fang Xue, Jia-Shu Niu, Jian-Ning Fu

Stellar structure and evolution theory is one of the basis in modern astronomy. Stellar inner structures and their evolutionary states can be precisely tested by asteroseismology,…

astro-ph.IM2022★ 18 cited

ET White Paper: To Find the First Earth 2.0

Jian Ge, Hui Zhang, Weicheng Zang +163

We propose to develop a wide-field and ultra-high-precision photometric survey mission, temporarily named "Earth 2.0 (ET)". This mission is designed to measure, for the first time,…

astro-ph.HE2021★ 7 cited

Hybrid origins of the cosmic-ray nuclei spectral hardening at a few hundred GV

Jia-Shu Niu

Many experiments have confirmed the spectral hardening at a few hundred GV of cosmic-ray (CR) nuclei spectra, and three general different origins have been proposed: the primary so…

astro-ph.SR2021★ 13 cited

A rapidly evolving high-amplitude Scuti star crossing the Hertzsprung Gap

Jia-Shu Niu, Hui-Fang Xue

In this work, we report the discovery of the rapidly evolving high-amplitude Scuti star KIC 6382916 (J19480292+4146558) which is crossing the Hertzsprung gap. According to the…

astro-ph.HE2020★ 8 cited

Origin of hardening in spectra of cosmic ray nuclei at a few hundred GeV using AMS-02 data

Jia-Shu Niu

Many experiments have confirmed the spectral hardening in a few hundred GV of cosmic ray (CR) nuclei spectra, and 3 different origins have been proposed: the primary source acceler…

astro-ph.SR2020★ 18 cited

DY Pegasi: An SX Phoenicis Star in a Binary System with an Evolved Companion

Hui-Fang Xue, Jia-Shu Niu

In this work, the photometric data from the American Association of Variable Star Observers are collected and analyzed on the SX Phoenicis star DY Pegasi (DY Peg). From the frequen…

hep-ph2019

Comment on "Probing the Dark Matter-Electron Interactions via Hydrogen-Atmosphere Pulsating White Dwarfs''

Jia-Shu Niu, Hui-Fang Xue

In Phys. Rev. D 98, 103023 (2018), a novel scenario was proposed to probe the interactions between dark matter (DM) particles and electrons, via hydrogen-atmosphere pulsating white…

astro-ph.HE2019★ 8 cited

Some new hints on cosmic-ray propagation from AMS-02 nuclei spectra

Jia-Shu Niu, Hui-Fang Xue

In this work, we considered 2 schemes (a high-rigidity break in primary source injections and a high-rigidity break in diffusion coefficient) to reproduce the newly released AMS-02…

astro-ph.SR2018★ 4 cited

NGC 1893: a young open cluster rich in multi-type variable stars

Hui-Fang Xue, Jian-Ning Fu, Nami Mowlavi +4

In this work, we have studied the variable stars in the young open cluster NGC 1893 based on a multi-year photometric survey covering a sky area around the cluster up to $31' \time…

astro-ph.HE2018★ 15 cited

Bayesian analysis of the hardening in AMS-02 nuclei spectra

Jia-Shu Niu, Tianjun Li, Hui-Fang Xue

Based on the precise nuclei data released by AMS-02, we study the spectra hardening of both the primary (proton, helium, carbon, oxygen, and the primary component of nitrogen) and…