collaborators

6 papers

astro-ph.GA2026

Stellar microlensing surveys as a probe of Primordial Black Holes: status and prospects

Anne M. Green

Stellar microlensing surveys are a powerful tool for probing dark matter in the form of planetary and stellar mass compact objects (COs), in particular primordial black holes (PBHs…

astro-ph.GA2025

findAbar: how astronomers may perceive the bar in galaxies differently

Elizabeth J. Iles, Joss Bland-Hawthorn, Courtney Crawford +18

Bars are ubiquitous morphological features in the observed distribution of galaxies. There are similarly many methods for classifying these features and, without a strict theoretic…

astro-ph.CO2025

The History of Primordial Black Holes

Bernard J. Carr, Anne M. Green

We overview the history of primordial black hole (PBH) research from the first papers around 50 years ago to the present epoch. The history may be divided into four periods, the di…

astro-ph.GA2025

Primordial Black Hole stellar microlensing constraints: understanding their dependence on the density and velocity distributions

Anne M. Green

Microlensing surveys of stars in the Large Magellanic Cloud constrain the fraction of the Milky Way halo in Primordial Black Holes (PBHs) with mass $10^{-9} \lesssim M/M_{\odot} \l…

astro-ph.CO2025

A Fast and Accurate Implementation of the Effective Fluid Approximation for Ultralight Axions

Adam Moss, Lauren Gaughan, Anne M. Green

We present a numerically efficient and accurate implementation of the Passaglia-Hu effective fluid approximation for ultralight axions (ULAs) within the Boltzmann code CAMB. This m…

astro-ph.CO2024

How open is the asteroid-mass primordial black hole window?

Matthew Gorton, Anne M. Green

Primordial black holes (PBHs) can make up all of the dark matter (DM) if their mass, , is in the so-called 'asteroid-mass window', $10^{17} \, {\rm g} \lesssim m \lesssim 10^{22…