activity
20042026
most citedA Three-Loop Model of Neutrino Mass with Dark Matter

79 citations · 862 across the 36 of their papers we have counts for

collaborators

37 papers

hep-ph2026

-Mode oscillations and the gravitational response of compact stars with analytic equations of state

Kilar Zhang, Alessandro Parisi, C. Vásquez Flores +2

We use a simple holographic model to study the property of cold and dense neutron stars (NSs) and deconfined QCD matter. With the aim of investigating the global properties of comp…

astro-ph.HE2023★ 14 cited

Dark Stars and Gravitational Waves: Topical Review

Kilar Zhang, Ling-Wei Luo, Jie-Shiun Tsao +2

Motivated by recent observations of compact binary gravitational wave events reported by LIGO/Virgo/KAGRA, we review the basics of dark and hybrid stars and examine their probabili…

astro-ph.HE2021★ 22 cited

Self-interacting Dark Scalar Spikes around Black Holes via Relativistic Bondi Accretion

Wei-Xiang Feng, Alessandro Parisi, Chian-Shu Chen +1

We consider the spike mass density profile in a dark halo by self-consistently solving the relativistic Bondi accretion of dark matter onto a non-spining black hole of mass . We…

astro-ph.HE2020

Hybrid stars in the light of the merging event GW170817

Alessandro Parisi, C. Vásquez Flores, C. Henrique Lenzi +2

We study quark-hadron hybrid stars with sharp phase transitions assuming that phase conversions at the interface are slow. Hadronic matter is described by a set of equations of sta…

hep-ph2019★ 16 cited

Fundamental oscillation modes of scalar bosonic dark stars

C. Vásquez Flores, Alessandro Parisi, Chian-Shu Chen +1

We perform a detailed analysis of the fundamental -mode frequencies and damping times of nonrotating boson stars in general relativity by solving the nonradial perturbation equa…

hep-ph2018★ 3 cited

On the evolution process of two-component dark matter in the Sun

Chian-Shu Chen, Yen-Hsun Lin

We introduce dark matter (DM) evolution process in the Sun under a two-component DM (2DM) scenario. Both DM species and with masses heavier than 1 GeV are considered. In th…