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20142026
most citedAcoustic Dark Energy: Potential Conversion of the Hubble Tension

263 citations · 751 across the 16 of their papers we have counts for

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11 papers · 1 filter

astro-ph.CO2026

Realization Variance of Gravitational Wave Background Anisotropies from Shot Noise for Pulsar Timing Arrays

Meng-Xiang Lin, Adam Lidz, Chung-Pei Ma

Shot-noise anisotropies in the nHz gravitational wave background (GWB) are a promising target for pulsar timing arrays (PTAs). If the nHz GWB is sourced by merging supermassive bla…

astro-ph.CO2026

Analytical Estimates of Gravitational Wave Background Anisotropies from Shot Noise and Large-Scale Structure in Pulsar Timing Arrays

Meng-Xiang Lin, Adam Lidz, Chung-Pei Ma

An important next step for pulsar timing arrays (PTAs) is to measure anisotropies in the gravitational wave background (GWB) at nano-Hz frequencies. We calculate the expecte…

astro-ph.CO2025

Consistent Initial Conditions for Early Modified Gravity in Effective Field Theory

Jiaming Pan, Meng-Xiang Lin, Gen Ye +2

Precise initial conditions (ICs) are crucial for accurate computation in cosmological perturbation theory. We derive the consistent ICs for Horndeski theory in the Effective Field…

astro-ph.CO2023★ 10 cited

Late Time Modification of Structure Growth and the S8 Tension

Meng-Xiang Lin, Bhuvnesh Jain, Marco Raveri +5

The tension between low-redshift galaxy surveys and the primary CMB signals a possible breakdown of the CDM model. Recently differing results have been obtained using low-…

astro-ph.CO2023★ 28 cited

A Test of Gravity with Pulsar Timing Arrays

Qiuyue Liang, Meng-Xiang Lin, Mark Trodden

A successful measurement of the Stochastic Gravitational Wave Background (SGWB) in Pulsar Timing Arrays (PTAs) would open up a new window through which to test the predictions of G…

astro-ph.CO2022★ 34 cited

A Dark Matter Trigger for Early Dark Energy Coincidence

Meng-Xiang Lin, Evan McDonough, J. Colin Hill +1

Early dark energy (EDE), whose cosmological role is localized in time around the epoch of matter-radiation equality in order to resolve the Hubble tension, introduces a new coincid…

astro-ph.CO2021★ 64 cited

The Early Dark Sector, the Hubble Tension, and the Swampland

Evan McDonough, Meng-Xiang Lin, J. Colin Hill +2

We consider the interplay of the Early Dark Energy (EDE) model, the Swampland Distance Conjecture (SDC), and cosmological parameter tensions. EDE is a proposed resolution of the Hu…

astro-ph.CO2021★ 1 cited

Gravitational wave propagation beyond general relativity: waveform distortions and echoes

Jose Maria Ezquiaga, Wayne Hu, Macarena Lagos +1

We study the cosmological propagation of gravitational waves (GWs) beyond general relativity (GR) across homogeneous and isotropic backgrounds. We consider scenarios in which GWs i…

astro-ph.CO2020★ 64 cited

Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization

Meng-Xiang Lin, Wayne Hu, Marco Raveri

The canonical acoustic dark energy model (cADE), which is based on a scalar field with a canonical kinetic term that rapidly converts potential to kinetic energy around matter radi…

astro-ph.CO2019★ 263 cited

Acoustic Dark Energy: Potential Conversion of the Hubble Tension

Meng-Xiang Lin, Giampaolo Benevento, Wayne Hu +1

We discuss the ability of a dark fluid becoming relevant around the time of matter radiation equality to significantly relieve the tension between local measurements of the Hubble…

astro-ph.CO2018★ 79 cited

Phenomenology of Modified Gravity at Recombination

Meng-Xiang Lin, Marco Raveri, Wayne Hu

We discuss the phenomenological imprints of modifications to gravity in the early universe with a specific focus on the time of recombination. We derive several interesting results…