activity
20222026
most citedHydrodynamic sound shell model

41 citations · 152 across the 22 of their papers we have counts for

collaborators

23 papers

astro-ph.CO2026

Cross-correlating Squared kSZ and HI Intensity Fields: A Map-level ACT--MeerKAT Forecast

Yu-Er Jiang, Yun Liu, Yan Gong +5

The kinetic Sunyaev--Zel'dovich (kSZ) effect probes the line-of-sight momentum of free electrons, but its blackbody spectrum and velocity-dependent sign make it difficult to isolat…

astro-ph.HE2026

Constraints on Axion-like Dark Matter from Cosmic Birefringence with a Polarization Array of Repeating Fast Radio Bursts

Xiaohui Liu, Zi-Yan Yuwen, Yun-Long Zhang +5

Axion-like dark matter (ALDM) is a well-motivated dark matter candidate whose Chern-Simons coupling to photons can induce cosmic birefringence, producing temporal oscillations and…

gr-qc2026

Cosmological Vacuum Decays from Schwinger-Keldysh Formalism

Zi-Yan Yuwen

In this work, we take a first step to a stochastic real-time description of the vacuum phase transitions in a radiation-dominated FLRW universe from the Schwinger-Keldysh formalism…

gr-qc2026

Primordial black hole formation in bulk-viscous cosmology

Zi-Yan Yuwen, Cristian Joana, Shao-Jiang Wang +1

We investigate primordial black hole (PBH) formation in a cosmological background with bulk viscosity. Using numerical simulations, we determine the collapse threshold and the resu…

astro-ph.HE2026

The MeerKAT Thousand-Pulsar Polarisation Array II: Searches for Ultralight Axion-Like Dark Matter

Zi-Yan Yuwen, Michael Sarkis, Yin-Zhe Ma +4

We construct Pulsar Polarisation Arrays (PPA), using regular pulsars monitored in MeerKAT's Thousand Pulsar Array (TPA) Programme, to search for Axion-like Dark Matter (ALDM) withi…

astro-ph.HE2026

The MeerKAT Thousand-Pulsar Polarization Array I: Properties of the Polarization and Rotation Measure Time Series Data

Michael Sarkis, Zi-Yan Yuwen, Yin-Zhe Ma +4

The polarimetry of recent pulsar observations has provided a wealth of observational data with which to test physical theories of emission mechanisms, radiative transfer and even t…

hep-ph2026

Vacuum bubbles from cosmic ripples

Zi-Yan Yuwen, Rong-Gen Cai, Shao-Jiang Wang

We investigate vacuum decays in the early Universe in the presence of curvature perturbations. For sufficiently large perturbations associated with over-densities, we find that the…

astro-ph.CO2026

Squared-field cross-correlation between kinetic Sunyaev-Zel'dovich effect and 21-cm intensity mapping

Zi-Yan Yuwen, Yu-Er Jiang, Yin-Zhe Ma +3

Neutral hydrogen (HI) 21-cm intensity mapping is an effective method to track the distribution of baryonic matter, and extract astrophysical and cosmological information. The 21-cm…

gr-qc2025

Acoustic gravitational waves from primordial curvature perturbations

Zhuan Ning, Zi-Yan Yuwen, Xiang-Xi Zeng +2

Standard perturbative calculations of scalar-induced gravitational waves (SIGWs) have neglected nonperturbative effects in the large-amplitude regime. We develop a hybrid numerical…

astro-ph.CO2025

Primordial Black Holes from Primordial Voids

Cristian Joana, Zi-Yan Yuwen

Primordial black holes (PBHs) are a compelling dark matter candidate and a unique probe of small-scale cosmological fluctuations. Their formation is usually attributed to large pos…

astro-ph.CO2025

Cosmological Prediction from the joint observation of MeerKAT and CSST at = 0.4 1.2

Yu-Er Jiang, Yan Gong, Qi Xiong +10

Cross-correlating neutral hydrogen (HI) 21cm intensity mapping with galaxy surveys provides an effective probe of astrophysical and cosmological information. This work presents a c…

gr-qc2025★ 4 cited

Sound waves from primordial black hole formations

Zhuan Ning, Xiang-Xi Zeng, Zi-Yan Yuwen +3

We present a numerical investigation of primordial black hole (PBH) formation from super-horizon curvature perturbations and the subsequent generation and propagation of sound wave…

gr-qc2025

Relic gravitational waves from primordial gravitational collapses

Xiang-Xi Zeng, Zhuan Ning, Zi-Yan Yuwen +3

A large primordial density perturbation of the Hubble scale will gravitationally collapse, generating an outgoing sound shell, whether or not a primordial black hole (PBH) is forme…

gr-qc2025★ 4 cited

Gravitational waves from vacuum bubbles: Ultraviolet dependence on wall thickness

Jun-Chen Wang, Shao-Jiang Wang, Zi-Yan Yuwen

The gravitational wave (GW) spectrum from the first-order phase transition can be characterized by a few phenomenological parameters but with high degeneracies in model/data distin…

astro-ph.CO2024★ 7 cited

Anisotropies of cosmological gravitational wave backgrounds in non-flat spacetime

Rong-Gen Cai, Shao-Jiang Wang, Zi-Yan Yuwen +1

Recent reports of stochastic gravitational wave background from four independent pulsar-timing-array collaborations have renewed the interest in the cosmological gravitational wave…

hep-ph2024

Bubble wall velocity from number density current in (non)equilibrium

Zi-Yan Yuwen, Jun-Chen Wang, Shao-Jiang Wang

Cosmological first-order phase transitions (FOPTs) serve as comprehensive probes into our early Universe with associated generations of stochastic gravitational waves and superhori…

gr-qc2024★ 2 cited

Bubbles kick off primordial black holes to form more binaries

Zi-Yan Yuwen, Cristian Joana, Shao-Jiang Wang +1

Primordial black holes (PBHs) may form before cosmological first-order phase transitions, leading to inevitable collisions between PBHs and bubble walls. In this Letter, we have si…

hep-ph2023★ 10 cited

General bubble expansion at strong coupling

Jun-Chen Wang, Zi-Yan Yuwen, Yu-Shi Hao +1

The strongly coupled system like the quark-hadron transition (if it is of first order) is becoming an active play yard for the physics of cosmological first-order phase transitions…

hep-ph2023★ 6 cited

General backreaction force of cosmological bubble expansion

Jun-Chen Wang, Zi-Yan Yuwen, Yu-Shi Hao +1

The gravitational-wave energy-density spectra from cosmological first-order phase transitions crucially depend on the terminal wall velocity of asymptotic bubble expansion when the…

gr-qc2023★ 41 cited

Hydrodynamic sound shell model

Rong-Gen Cai, Shao-Jiang Wang, Zi-Yan Yuwen

For a cosmological first-order phase transition in the early Universe, the associated stochastic gravitational wave background is usually dominated by sound waves from plasma fluid…

hep-th2023★ 22 cited

Bubble expansion at strong coupling

Li Li, Shao-Jiang Wang, Zi-Yan Yuwen

The cosmological first-order phase transition (FOPT) can be of strong dynamics but with its bubble wall velocity difficult to be determined due to lack of detailed collision terms.…

hep-ph2022★ 25 cited

The energy budget of cosmological first-order phase transitions beyond the bag equation of state

Shao-Jiang Wang, Zi-Yan Yuwen

The stochastic gravitational-wave backgrounds (SGWBs) from the cosmological first-order phase transitions (FOPTs) serve as a promising probe for the new physics beyond the standard…

hep-ph2022★ 31 cited

Hydrodynamic backreaction force of cosmological bubble expansion

Shao-Jiang Wang, Zi-Yan Yuwen

As a promising probe for the new physics beyond the standard model of particle physics in the early Universe, the predictions for the stochastic gravitational wave background from…