Journal of the Korean Physical Society

, Volume 65, Issue 6, pp 876–878 | Cite as

The Double Pulsar PSR J0737-3039

  • Chunglee Kim


The Double Pulsar (PSR J0737-3039) consists of two active radio pulsars (labeled as A and B) that are bound in a slightly eccentric, tight orbit. This is one of the best astrophysical laboratories to test Einstein’s theory of general relativity. All five post-Keplerian parameters are measured independently for the A and the B pulsars, and they are consistent with predictions from general relativity. The Double Pulsar is also useful for understanding the formation and the coalescence of double-neutron-star systems. We summarize the properties of the Double Pulsar and discuss their implications for testing general relativity and for detecting gravitational waves.


Pulsars Binary Gravitational Waves Ratio Observations 


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Copyright information

© The Korean Physical Society 2014

Authors and Affiliations

  1. 1.Astronomy Program, Department of Physics and AstronomySeoul National UniversitySeoulKorea

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