activity
20152025
most citedAxion dark matter: strings and their cores

117 citations · 191 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2025

Axion Constraints from White Dwarf Cooling in 47 Tucanae

Leesa Fleury, Alysa Obertas, Harvey Richer +1

We analyse the cooling of white dwarfs in the globular cluster 47 Tucanae to look for evidence of axion emission affecting the rate of white dwarf cooling. If axions exist and coup…

astro-ph.SR2025

The Cooling of Old White Dwarfs in 47 Tucanae

Leesa Fleury, Harvey Richer, Jeremy Heyl

We analyse the cooling of white dwarfs in the globular cluster 47 Tucanae (47 Tuc) using deep observations from the Hubble Space Telescope that resolve the white dwarf cooling sequ…

astro-ph.HE2022★ 3 cited

Constraining Axions with ZTF J1901+1458

Leesa Fleury, Ilaria Caiazzo, Jeremy Heyl

The axion-nucleon coupling enables the production of axions through the decay of excited isotopes, and axions produced in the Sun through this process are ofte…

astro-ph.SR2022★ 5 cited

The origin of ultramassive white dwarfs: hints from Gaia EDR3

Leesa Fleury, Ilaria Caiazzo, Jeremy Heyl

Gaia Data Release 2 revealed a population of ultramassive white dwarfs on the Q branch that are moving anomalously fast for a local disc population with their young photometric age…

astro-ph.SR2021★ 21 cited

The Cooling of Massive White Dwarfs from Gaia EDR3

Leesa Fleury, Ilaria Caiazzo, Jeremy Heyl

We determine the distribution of cooling ages of massive Gaia EDR3 white dwarfs identified with over 90% probability within 200 pc and with mass in the range 0.95-1.25 . U…

astro-ph.SR2020★ 15 cited

Intermediate-Mass Stars Become Magnetic White Dwarfs

Ilaria Caiazzo, Jeremy Heyl, Harvey Richer +8

When a star exhausts its nuclear fuel, it either explodes as a supernova or more quiescently becomes a white dwarf, an object about half the mass of our Sun with a radius of about…

hep-ph2016★ 30 cited

Axion String Dynamics I: 2+1D

Leesa M. Fleury, Guy D. Moore

If the axion exists and if the initial axion field value is uncorrelated at causally disconnected points, then it should be possible to predict the efficiency of cosmological axion…

hep-ph2015★ 117 cited

Axion dark matter: strings and their cores

Leesa Fleury, Guy D. Moore

Axions constitute a well-motivated dark matter candidate, and if PQ symmetry breaking occurred after inflation, it should be possible to make a clean prediction for the relation be…