collaborators

10 papers

astro-ph.CO2026

A data-driven prediction for the primordial deuterium abundance

Timothy Launders, Cara Giovanetti, Hongwan Liu

We predict the primordial deuterium abundance using a novel, fully data-driven approach, where we use Gaussian process regression to fit experimental nuclear reaction data for ,…

astro-ph.CO2026

ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum

Zilu Zhou, Cara Giovanetti, Hongwan Liu

We present ABCMB, a differentiable Einstein-Boltzmann solver for the cosmic microwave background (CMB). ABCMB is a complete code capturing important effects to linear order in $Λ{…

astro-ph.CO2025

Constraining Dark Acoustic Oscillations with the High-Redshift UV Luminosity Function

Jared Barron, David Curtin, Hongwan Liu +2

Dark acoustic oscillations (DAOs) in the matter power spectrum can arise in many different dark sector models, and can imprint on a variety of cosmological observables. In this wor…

astro-ph.CO2025

Dynamical Heating from Dark Compact Objects and Axion Minihalos: Implications for the 21-cm Signal

Badal Bhalla, Aurora Ireland, Hongwan Liu +2

The temperature of baryons at the end of the cosmic dark ages can be inferred from observations of the 21-cm hyperfine transition in neutral hydrogen. Any energy injection from the…

astro-ph.CO2025

LINX: A Fast, Differentiable, and Extensible Big Bang Nucleosynthesis Package

Cara Giovanetti, Mariangela Lisanti, Hongwan Liu +2

We introduce LINX (Light Isotope Nucleosynthesis with JAX), a new differentiable public Big Bang Nucleosynthesis (BBN) code designed for fast parameter estimation. By leveraging JA…

astro-ph.CO2025

Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis

Cara Giovanetti, Mariangela Lisanti, Hongwan Liu +2

We present the first joint-likelihood analysis of Big Bang Nucleosynthesis (BBN) and Cosmic Microwave Background (CMB) data. Bayesian inference is performed on the baryon abundance…