36 citations · 97 across the 11 of their papers we have counts for
11 papers
Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era
Zeyuan Xuan, Smadar Naoz, Kyle Kremer +3
Eccentric binary black holes (BBHs) formed through dynamical interactions can significantly contribute to gravitational wave (GW) detections. In this work, we present a simulated c…
From Wide Triples to UCXBs: Multimessenger Signatures of Dynamically-formed Black Hole-White Dwarf Systems in the LISA Band
Zeyuan Xuan, Cheyanne Shariat, Smadar Naoz
Ultracompact X-ray binaries (UCXBs) are a subclass of low-mass X-ray binaries characterized by tight orbits and degenerate donors, which pose significant challenges to our understa…
Resonant Locking Between Binary Systems Induced by Gravitational Waves
Charlie Sharpe, Yonadav Barry Ginat, Zeyuan Xuan +1
The interaction of gravitational waves (GWs) with matter is thought to be typically negligible in the Universe. We identify an exception in the case of resonant interactions, where…
Localizing Dynamically-Formed Black Hole Binaries in Milky Way Globular Clusters with LISA
Zeyuan Xuan, Kyle Kremer, Smadar Naoz
The dynamical formation of binary black holes (BBHs) in globular clusters (GCs) may contribute significantly to the observed gravitational wave (GW) merger rate. Furthermore, LISA…
Extracting Astrophysical Information of Highly-Eccentric Binaries in the Millihertz Gravitational Wave Band
Zeyuan Xuan, Smadar Naoz, Alvin K. Y. Li +6
Wide, highly eccentric () compact binaries can naturally arise as progenitors of gravitational wave (GW) mergers. These systems are expected to have a significant population…
Stochastic Gravitational Wave Background from Highly-Eccentric Stellar-Mass Binaries in the Milli-hertz Band
Zeyuan Xuan, Smadar Naoz, Bence Kocsis +1
Many gravitational wave (GW) sources are expected to have non-negligible eccentricity in the millihertz band. These highly eccentric compact object binaries may commonly serve as a…
Detecting Gravitational Wave Bursts From Stellar-Mass Binaries in the Milli-hertz Band
Zeyuan Xuan, Smadar Naoz, Bence Kocsis +1
The dynamical formation channels of gravitational wave (GW) sources typically involve a stage when the compact object binary source interacts with the environment, which may excite…
Detecting Accelerating Eccentric Binaries in the LISA Band
Zeyuan Xuan, Smadar Naoz, Xian Chen
Many gravitational wave (GW) sources in the LISA band are expected to have non-negligible eccentricity. Furthermore, many of them can undergo acceleration because they reside in th…
Degeneracy between mass and peculiar acceleration for the double white dwarfs in the LISA band
Zeyuan Xuan, Peng Peng, Xian Chen
Mass and distance are fundamental quantities to measure in gravitational-wave (GW) astronomy. However, recent studies suggest that the measurement may be biased due to the accelera…
Exciting modes due to the aberration of gravitational waves: Measurability for extreme-mass-ratio inspirals
Alejandro Torres-Orjuela, Pau Amaro Seoane, Zeyuan Xuan +3
Gravitational waves from a source moving relative to us can suffer from special-relativistic effects such as aberration. The required velocities for these to be significant are on…
Fake massive black holes in the milli-Hertz gravitational-wave band
Xian Chen, Ze-Yuan Xuan, Peng Peng
In gravitational wave (GW) astronomy accurate measurement of the source parameters, such as mass, relies on accurate waveform templates. Currently, the templates are developed assu…