Compact Dark Matter with Globular Cluster Pulsars
Abstract
Pulsars are exceptionally stable clocks, and a compact dark-matter object passing near the line of sight to a pulsar delays its pulses through the Shapiro effect. The number of detectable transits is set by the integral over the dark-matter density along the line of sight connecting the Earth and the pulsar. Established pulsars in pulsar timing arrays are typically within one kiloparsec of the Earth and hence sit in a dark-matter density comparable to our local value. In this work, we explore globular clusters in the inner Galaxy as targets to search for compact dark matter. These high-pulsar-density environments can be cheaply observed with a single telescope beam and enjoy a large dark-matter crossing rate. Additionally, since the recently detected nanohertz gravitational-wave background is nearly common to the cluster's pulsars, a multi-pulsar analysis can remove much of its contribution. Ranking known clusters, we find that Terzan 5, with 49 pulsars, offers the best reach. A forty-year campaign of weekly four-hour visits at the sensitivity envisioned for the second phase of the Square Kilometre Array (SKA) would probe compact objects making up 6% of the dark matter at 0.02 M⊙. Finally, we estimate the foreground from stars and stellar remnants in Terzan 5 and along the sightline. It is subdominant near the most sensitive low-mass part of the SKA benchmark, but becomes important over parts of the stellar mass range.
Related
- Constraints on the fuzzy dark matter mass using globular clusters in dwarf galaxies from Euclid ERO data
- The Origin of Isolated Millisecond Pulsars in Non-core-collapsed Globular Clusters
- Two-Fluid Radial Stability of Dark-Matter-Admixed Compact Objects: Dark Compact Planets, Dark White Dwarfs, Dark Neutron Stars, and Dark Oysters
- Reconstructing the Dark Matter Equation of State with Compact Object Inspirals
- Radial stress in rotating ACKN/KSZ continuations of Einstein-cluster dark matter halos
BibTeX
@misc{chung2026compact,
title = {{Compact Dark Matter with Globular Cluster Pulsars}},
author = {Soobeom Chung and Jeff A. Dror},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.20732},
eprint = {2610.20732},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.20732},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Compact Dark Matter with Globular Cluster Pulsars
AU - Soobeom Chung
AU - Jeff A. Dror
PY - 2026
DA - 2026/10/14
PB - arXiv
DO - 10.48550/arxiv.2610.20732
UR - https://arxiv.org/abs/2610.20732
AB - Pulsars are exceptionally stable clocks, and a compact dark-matter object passing near the line of sight to a pulsar delays its pulses through the Shapiro effect. The number of detectable transits is set by the integral over the dark-matter density along the line of sight connecting the Earth and the pulsar. Established pulsars in pulsar timing arrays are typically within one kiloparsec of the Earth and hence sit in a dark-matter density comparable to our local value. In this work, we explore globular clusters in the inner Galaxy as targets to search for compact dark matter. These high-pulsar-density environments can be cheaply observed with a single telescope beam and enjoy a large dark-matter crossing rate. Additionally, since the recently detected nanohertz gravitational-wave background is nearly common to the cluster's pulsars, a multi-pulsar analysis can remove much of its contribution. Ranking known clusters, we find that Terzan 5, with 49 pulsars, offers the best reach. A forty-year campaign of weekly four-hour visits at the sensitivity envisioned for the second phase of the Square Kilometre Array (SKA) would probe compact objects making up 6% of the dark matter at 0.02 M_⊙. Finally, we estimate the foreground from stars and stellar remnants in Terzan 5 and along the sightline. It is subdominant near the most sensitive low-mass part of the SKA benchmark, but becomes important over parts of the stellar mass range.
ER -