The
only known binary system of two detectable pulsars ("The Double
Pulsar") was discovered in 2003. Since that time, this remarkable binary
has been used to test general relativity, probe pulsar emission physics,
constrain fundamental properties of neutron stars, and calculated expected
event rates for ground-based gravitational wave detectors. In this talk, I will
review 10 years of sensitive GBT observations of this system and how these
observations have been used in all of these ways.
Array Operations Center Auditorium
All NRAO employees are invited to attend via video, available in Charlottesville Room 209, Green Bank Auditorium, Tucson N525 and VLA Video Conference Room.
Local Host: Paul Demorest