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Wednesday, April 06, 2022
4:00 PM - 5:00 PM
Online Event

Astronomy Colloquium

Precision Strong-Field Gravity Tests with the Double Pulsar
Ingrid Stairs, Professor, Division of Physics and Astronomy, University of British Columbia,

The only known double-pulsar system has a number of unique features, including an extremely relativistic 2.5-hour orbit and an orbital inclined nearly edge-on to the line of sight. Our collaboration has been timing this system for over 16 years with various telescopes and now need to take into account higher-order relativistic effects when modelling and interpreting the data. The new phenomena observed include relativistic deformation of the orbit and next-to-leading-order effects on the Shapiro delay (retardation) and the aberration (gravitational signal deflection). It is also necessary to account for the Lense-Thirring effect (relativistic spin-orbit coupling) when interpreting the advance of periastron, leading to a constraint on the equation of state of super-dense matter. We have achieved the most precise test to date of the general-relativistic quadrupolar description of gravitational waves, finding agreement with GR at a level of 0.013% with 95% confidence.

To view this talk via YouTube, please visit:

For more information, please contact Jim Fuller by email at [email protected] or visit