Pulsar Timing Sensitivity to Dark Matter Substructure in the Presence of a Stochastic Gravitational-Wave Background
Abhiram Cherukupalli, Vincent S. H. Lee, Kim Berghaus, Kathryn M. Zurek
astro-ph.CO, hep-ph
Submitted: 2026-07-03
Comments: 50 pages, 7 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Axion Miniclusters and Bose Stars
- Astrophysical Effects of Scalar Dark Matter Miniclusters
- Early-Universe Simulations of the Cosmological Axion
- First Simulations of Axion Minicluster Halos
- Simulations of Axion Minihalos
- The first WIMPy halos
- Probing Dark Matter Substructure with Pulsar Timing
- Prospects for Detecting Dark Matter Halo Substructure with Pulsar Timing
- Investigating dark matter substructure with pulsar timing: I. Constraints on ultracompact minihalos
- Pulsar timing can constrain primordial black holes in the LIGO mass window
- Detectability of Small-Scale Dark Matter Clumps with Pulsar Timing Arrays
- Pulsar Timing Probes of Primordial Black Holes and Subhalos
- Observability of Dark Matter Substructure with Pulsar Timing Correlations
- Probing Small-Scale Power Spectra with Pulsar Timing Arrays
- Bayesian Forecasts for Dark Matter Substructure Searches with Mock Pulsar Timing Data
- Astrophysical Observations of a Dark Matter-Baryon Fifth Force
- The NANOGrav 15-year Data Set: Search for Signals from New Physics
- Physics beyond the Standard Model with the DSA-2000
- The Nanohertz Gravitational Wave Astronomer
- A Practical Theorem on Gravitational Wave Backgrounds
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