activity
20242026
collaborators

5 papers

astro-ph.CO2026

Simulating a Gaussian stochastic gravitational wave background signal in pulsar timing arrays

Reginald Christian Bernardo, Kin-Wang Ng

We revisit the theoretical modeling and simulation of a Gaussian stochastic gravitational wave background (SGWB) signal in a pulsar timing array (PTA). We show that the correlation…

hep-ph2026

Four-point correlation functions in axion inflation

Hing-Tong Cho, Kin-Wang Ng

We study parity violation in the early universe by examining the four-point correlation function within the axion inflation model. Using an open quantum system formalism from our p…

astro-ph.CO2025

Accurate pulsar timing array residual variances and correlation of the stochastic gravitational wave background

Reginald Christian Bernardo, Kin-Wang Ng

Pulsar timing arrays have reported a compelling evidence of a nanohertz stochastic gravitational wave background. However, the origin of the signal remains undetermined, largely be…

astro-ph.CO2024

Toward a test of Gaussianity of a gravitational wave background

Reginald Christian Bernardo, Stephen Appleby, Kin-Wang Ng

The degree of Gaussianity of a field offers insights into its cosmological nature, and its statistical properties serve as indicators of its Gaussianity. In this work, we examine t…

gr-qc2024

Beyond the Hellings-Downs curve: Non-Einsteinian gravitational waves in pulsar timing array correlations

Reginald Christian Bernardo, Kin-Wang Ng

The recent astronomical milestone by the pulsar timing arrays (PTA) has revealed galactic-size gravitational waves (GW) in the form of a stochastic gravitational wave background (S…