Astronomers have discovered a unique stellar system of two white dwarf stars and a superdense neutron star, all packed within a space smaller than Earth’s orbit around the Sun. The closeness of the stars allows the scientists to make the most accurate measurements yet of the system’s complex gravitational interactions, measurements that might resolve one of the principal outstanding problems of fundamental physics – the true nature of gravity.
“This triple system gives us a natural cosmic laboratory far better than anything found before for learning exactly how such three-body systems work and potentially for detecting problems with General Relativity that physicists expect to see under extreme conditions,” said Scott Ransom of the National Radio Astronomy Observatory. He was part of an international team of researchers that reported their observations of the system in the journal Nature.
Ransom explained that the neutron star in the system is a pulsar, emitting lighthouse-like beams of radio waves that rapidly sweep through space as the object spins around on its axis 21,000 times per minute. Such rapidly-spinning pulsars can be used by astronomers as precision tools for studying a variety of phenomena, including searches for the elusive gravitational waves.
By very accurately recording the time of arrival of the pulsar’s pulses, the scientists were able to calculate the geometry of the triple system and the masses of the stars with unparalleled precision.
The scientists believe that this unique stellar laboratory will provide the best opportunity yet to discover a violation of a concept called the Equivalence Principle. This principle states that the effect of gravity on a body does not depend on the nature or internal structure of that body.
The most famous experiments illustrating the equivalence principle are Galileo’s reputed dropping of two balls of different weights from the Leaning Tower of Pisa and Apollo 15 astronaut Dave Scott’s dropping of a hammer and a feather while standing on the airless surface of the Moon in 1971.
When a massive star explodes as a supernova and its remains collapse into a superdense neutron star, some of its mass is converted into gravitational binding energy that holds the dense star together. The Strong Equivalence Principle says that this binding energy still will react gravitationally as if it were mass. Virtually all alternatives to General Relativity hold that it will not. “This system offers the best test yet of which is the case,” Ransom said.
Under the strong equivalence principle, the gravitational effect of the outer white dwarf would be identical for both the inner white dwarf and the neutron star. If the strong equivalence principle is invalid under the conditions in this system, the outer star’s gravitational effect on the inner white dwarf and the neutron star would be slightly different and the high-precision pulsar timing observations could easily show that.
“By doing very high-precision timing of the pulses coming from the pulsar, we can test for such a deviation from the strong equivalence principle at a sensitivity several orders of magnitude greater than ever before available,” said co-researcher Ingrid Stairs, from the University of British Columbia. “Finding a deviation from the Strong Equivalence Principle would indicate a breakdown of General Relativity and would point us toward a new, correct theory of gravity.”
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