A Pulsar-Based Map of Galactic Acceleration
arXiv:2306.13137 · doi:10.1103/PhysRevD.109.123015
Abstract
Binary pulsars can be used to probe Galactic potential gradients through calculating their line-of-sight accelerations. We present the first data release of direct line-of-sight acceleration measurements for 29 binary pulsars. We validate these data with a local acceleration model, and compare our results to those from earlier works. We find evidence for an acceleration gradient in agreement with these values, with our results indicating a local disk density of . We also find evidence for unmodeled noise of unknown origin in our data set.
12 pages, 7 figures
References in corpus (19)
- Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars
- On the local dark matter density
- The second data release from the European Pulsar Timing Array I. The dataset and timing analysis
- Strong-field Gravity Tests with the Double Pulsar
- Pulsar Timing Probes of Primordial Black Holes and Subhalos
- The Parkes pulsar timing array second data release: Timing analysis
- A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations
- Closing a spontaneous-scalarization window with binary pulsars
- PSR J2222--0137. I. Improved physical parameters for the system
- Neutron Stars with Baryon Number Violation, Probing Dark Sectors
- Implications of a time-varying Galactic potential for determinations of the dynamical surface density
- Why are pulsar planets rare?
- Eclipse timing the Milky Way's gravitational potential
- A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme
- Seeing the gravitational wave universe
- Non-equilibrium in the Solar Neighbourhood using dynamical modelling with Gaia DR2
- Galactic Orbital Effects on Pulsar Timing