The components of the binary model that describe the second-order motion of a pulsar and companion (e.g., a white dwarf) orbiting around each other, due not from simple Newtonian gravity but from Einstein’s General Relativity.
The components of the binary model that describe the second-order motion of a pulsar and companion (e.g., a white dwarf) orbiting around each other, due not from simple Newtonian gravity but from Einstein’s General Relativity.