activity
20072026
most citedScience with the Cherenkov Telescope Array

241 citations · 2.6k across the 97 of their papers we have counts for

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Showing astro-ph.COShow all

14 papers · 1 filter

astro-ph.CO2026

A Dark-matter Origin of Little Red Dots: Early Seeding and Super-Bondi Accretion

Hua-Peng Gu, Fangzhou Jiang, Xian Chen +2

The "Little red dots" (LRDs) are a population of accreting supermassive black holes (SMBHs) in the early Universe which often exhibit undermassive or even undetectable stellar host…

astro-ph.CO2026

Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass

Hua-Peng Gu, Fangzhou Jiang, Xian Chen +1

Recent observations of supermassive black holes (SMBHs) at high redshifts pose challenges to standard seeding mechanisms. Among competing models, the collapse of self-interacting d…

astro-ph.CO2024★ 14 cited

Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals

Liang-Gui Zhu, Hui-Min Fan, Xian Chen +2

Extreme-mass-ratio inspirals (EMRIs) could be detected by space-borne gravitational-wave (GW) detectors, such as the Laser Interferometer Space Antenna (LISA), TianQin and Taiji. L…

astro-ph.CO2024

An Opacity-Free Method of Testing the Cosmic Distance Duality Relation Using Strongly Lensed Gravitational Wave Signals

Shun-Jia Huang, En-Kun Li, Jian-dong Zhang +4

The cosmic distance duality relation (CDDR), expressed as DL(z) = (1 + z)2DA(z), plays an important role in modern cosmology. In this paper, we propose a new method of testing CDDR…

astro-ph.CO2024★ 45 cited

LISA Definition Study Report

Monica Colpi, Karsten Danzmann, Martin Hewitson +108

The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves…

astro-ph.CO2023★ 15 cited

Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals

Shun-Jia Huang, Yi-Ming Hu, Xian Chen +4

The measurement of the Hubble constant plays an important role in the study of cosmology. In this letter, we propose a new method to constrain the Hubble constant using the s…

astro-ph.CO2023★ 18 cited

The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant

Liang-Gui Zhu, Xian Chen

Dark sirens, i.e., gravitational-wave (GW) sources without electromagnetic counterparts, are new probes of the expansion of the universe. The efficacy of this method relies on corr…

astro-ph.CO2022★ 14 cited

Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant

Alejandro Torres-Orjuela, Xian Chen

Standard sirens - GW sources with an EM counterpart - can be used to measure H_0 directly which should help to ease the existing Hubble tension. However, if the source has a relati…

astro-ph.CO2021★ 38 cited

A Higher Probability of Detecting Lensed Supermassive Black Hole Binaries by LISA

Zucheng Gao, Xian Chen, Yi-Ming Hu +2

Gravitational lensing of gravitational waves (GWs) is a powerful probe of the matter distribution in the universe. Here we revisit the wave-optics effects induced by dark matter (D…

astro-ph.CO2020★ 27 cited

Excitation of gravitational wave modes by a center-of-mass velocity of the source

Alejandro Torres-Orjuela, Xian Chen, Pau Amaro Seoane

Most gravitational wave (GW) sources are moving relative to us. This motion is often closely related to the environment of the source and can thus provide crucial information about…

astro-ph.CO2015★ 66 cited

Relativistic mergers of black hole binaries have large, similar masses, low spins and are circular

Pau Amaro-Seoane, Xian Chen

Gravitational waves are a prediction of general relativity, and with ground-based detectors now running in their advanced configuration, we will soon be able to measure them direct…

astro-ph.CO2013★ 35 cited

The fragmenting past of the disk at the Galactic Center : The culprit for the missing red giants

Pau Amaro-Seoane, Xian Chen

Since 1996 we have known that the Galactic Center (GC) displays a core-like distribution of red giant branch (RGB) stars starting at ~ 10", which poses a theoretical problem, becau…

astro-ph.CO2013★ 30 cited

Enhanced off-center stellar tidal disruptions by supermassive black holes in merging galaxies

F. K. Liu, Xian Chen

Off-center stellar tidal disruption flares have been suggested to be a powerful probe of recoiling supermassive black holes (SMBHs) out of galactic centers due to anisotropic gravi…

astro-ph.CO2011★ 10 cited

Recoiling Supermassive Black Holes in Spin-flip Radio Galaxies

F. K. Liu, Dong Wang, Xian Chen

Numerical relativity simulations predict that coalescence of supermassive black hole (SMBH) binaries not only leads to a spin flip but also to a recoiling of the merger remnant SMB…