activity
20152022
most citedHubble Sinks In The Low-Redshift Swampland

205 citations · 1.6k across the 33 of their papers we have counts for

collaborators

33 papers

gr-qc2022★ 9 cited

Importance of eccentricities in parameter estimation of compact binary inspirals with decihertz gravitational-wave detectors

Han Gil Choi, Tao Yang, Hyung Mok Lee

During its inspiral stage, a binary black hole (BBH) produces characteristic gravitational wave (GW) signals. The waveform of the GW signals can be described by the physical parame…

gr-qc2022★ 16 cited

Space-borne atom interferometric gravitational wave detections. Part III. Eccentricity on dark sirens

Tao Yang, Rong-Gen Cai, Hyung Mok Lee

Eccentricity of the inspiraling compact binaries can greatly improve the distance inference and source localization of dark sirens. In this paper, we continue the research for the…

astro-ph.SR2022★ 12 cited

Frequency analysis of KIC 1573174 : shedding light on the nature of HADS stars

Chenglong Lv, Ali Esamdin, Javier Pascual-Granado +2

We propose that KIC 1573174 is a quadruple-mode Scuti star with pulsation amplitudes between those of the HADS (high-amplitude Delta Scuti star) group and average low-amplitude…

gr-qc2022★ 30 cited

Eccentricity of Long Inspiraling Compact Binaries Sheds Light on Dark Sirens

Tao Yang, Rong-Gen Cai, Zhoujian Cao +1

The localization and distance inference of gravitational waves are two crucial factors for dark sirens as precise probes of cosmology, astrophysics, and fundamental physics. In thi…

astro-ph.SR2021★ 2 cited

A catalogue of double-mode high amplitude Scuti stars in the Galaxy and their statistical properties

Tao-Zhi Yang, Zhao-Yu Zuo, Xin-Yue Wang +2

We present the first catalogue of double-mode and multi-mode high amplitude Scuti star (HADS) in the Galaxy. The catalogue contains source name, coordinates, radial modes such…

astro-ph.SR2021★ 10 cited

KIC 12602250: A low-amplitude Double-mode Scuti star with Amplitude Modulation

Chenlong Lv, Ali Esamdin, Xiangyun Zeng +3

We propose for the first time that KIC 12602250 is a low-amplitude radial double-mode Scuti star with amplitude modulation. The detailed frequency analysis is given for the lig…

gr-qc2021★ 10 cited

Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one

Tao Yang, Hyung Mok Lee, Rong-Gen Cai +2

In this paper, we investigate the potential of dark sirens by the space-borne atom interferometric gravitational-wave detectors to probe the Hubble constant. In the mid-frequency b…

astro-ph.SR2021★ 17 cited

TIC 308396022: a Scuti-- Doradus hybrid with large-amplitude radial fundamental mode and regular g-mode period spacing

Tao-Zhi Yang, Zhao-Yu Zuo, Gang Li +3

We analyse the pulsating behaviour of TIC 308396022 observed by the TESS mission. The star is a high-amplitude Sct star (HADS) that shows a very rich amplitude spectrum using t…

gr-qc2021★ 13 cited

Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology

Rong-Gen Cai, Tao Yang

Atom interferometers (AIs) as gravitational-wave (GW) detectors have been proposed a decade ago. Both ground and space-based projects will be in construction and preparation in the…

gr-qc2021★ 109 cited

The Gravitational-Wave Physics II: Progress

Ligong Bian, Rong-Gen Cai, Shuo Cao +15

It has been a half-decade since the first direct detection of gravitational waves, which signifies the coming of the era of the gravitational-wave astronomy and gravitational-wave…

astro-ph.CO2021★ 44 cited

Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory

Tao Yang

We construct the catalogues of standard sirens (StS) based on the future gravitational wave (GW) detector networks, i.e., the second-generation ground-based advanced LIGO+advanced…

astro-ph.SR2020★ 9 cited

KIC 10975348: A double-mode or triple-mode high-amplitude Scuti star?

Tao-Zhi Yang, Xiao-Ya Sun, Zhao-Yu Zuo +1

In this paper, we analyze the light variations of KIC 10975348 using photometric data delivered from mission. This star is exceptionally faint ( = 18.6 mag), compar…

astro-ph.CO2020★ 171 cited

Running Hubble Tension and a H0 Diagnostic

Chethan Krishnan, Eoin Ó Colgáin, M. M. Sheikh-Jabbari +1

Hubble tension is routinely presented as a mismatch between the Hubble constant determined locally and a value inferred from the flat CDM cosmology. In essence, the tensio…

astro-ph.CO2020★ 10 cited

Model-Independent Perspectives on Coupled Dark Energy and the Swampland

Tao Yang

We present a general model-independent approach to study the coupled dark energy and the string Swampland criteria. We show how the dark sector interaction is degenerated with the…

astro-ph.CO2020★ 205 cited

Hubble Sinks In The Low-Redshift Swampland

Aritra Banerjee, Haiying Cai, Lavinia Heisenberg +3

Local determinations of the Hubble constant favour a higher value than Planck based on CMB and CDM. Through a model-independent expansion, we show that low redshift ($z \l…

astro-ph.CO2020★ 39 cited

The first simultaneous measurement of Hubble constant and post-Newtonian parameter from Time-Delay Strong Lensing

Tao Yang, Simon Birrer, Bin Hu

Strong gravitational lensing has been a powerful probe of cosmological models and gravity. To date, constraints in either domain have been obtained separately. We propose a new met…

astro-ph.CO2020★ 164 cited

Is there an early Universe solution to Hubble tension?

Chethan Krishnan, Eoin Ó Colgáin, Ruchika +3

We consider a low redshift cosmological dataset comprising megamasers, cosmic chronometers, type Ia SNe and BAO, which we bin according to their redshift. For each bin, w…

astro-ph.SR2019

KIC 8840638: A new eclipsing binary consisting of Scuti-type oscillations with an extremely cold companion star

Tao-Zhi Yang, Zhao-Yu Zuo, Jun-Hui Liu +1

In this paper, we analyze the light variation of KIC 8840638 using high-precision time-series data from mission. The analysis reveals this target is a new Algol-type eclip…

astro-ph.CO2019★ 54 cited

Gaussian processes reconstruction of modified gravitational wave propagation

Enis Belgacem, Stefano Foffa, Michele Maggiore +1

Recent work has shown that modified gravitational wave (GW) propagation can be a powerful probe of dark energy and modified gravity, specific to GW observations. We use the techniq…

astro-ph.CO2019★ 103 cited

Cosmography and flat CDM tensions at high redshift

Tao Yang, Aritra Banerjee, Eoin Ó Colgáin

Risaliti, Lusso \& collaborators have constructed a high-redshift Hubble diagram of supernovae (SNe); quasars (QSO) and gamma-ray bursts (GRB) that shows a " tension w…

astro-ph.SR2019★ 14 cited

A double-modulation effect detected in a double-mode high-amplitude Scuti star: KIC 10284901

Tao-Zhi Yang, Ali Esamdin

In this paper, we present an analysis of the pulsating behavior of target KIC 10284901. The Fourier transform of the high-precision light curve reveals seven independent f…

astro-ph.SR2019★ 8 cited

Pulsations of the SX Phe Star BL Camelopardalis

Peng Zong, Ali Esamdin, Jian Ning Fu +6

We carried out photometric observations of the SX Phe star BL Cam in 2014, 2017 and 2018 using Nanshan 1-m telescope. In addition to the dominated frequency of 25.5790(3) cd…

astro-ph.CO2018★ 22 cited

New probe of gravity: strongly lensed gravitational wave multi-messenger approach

Tao Yang, Bin Hu, Rong-Gen Cai +1

Strong gravitational lensing by galaxies provides us with a unique opportunity to understand the nature of gravity on galactic and extra-galactic scales. In this paper, we propose…

astro-ph.CO2018★ 5 cited

Super-Eddington accreting massive black holes explore high- cosmology: Monte-Carlo simulations

Rong-Gen Cai, Zong-Kuan Guo, Qing-Guo Huang +1

In this paper, we simulate Super-Eddington accreting massive black holes (SEAMBHs) as the candles to probe cosmology for the first time. SEAMBHs have been demonstrated to be able t…