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Pulsars: The universe's gift to physics

Astronomers are using pulsars throughout the Milky Way Galaxy as a giant scientific instrument to directly detect gravitational waves.
By NRAO, Socorro, New Mexico Published: February 20, 2012
pulsar-graphic
Pulsars are spinning neutron stars. Credit: Bill Saxton, NRAO/AUI/NSF
Pulsars, superdense neutron stars, are perhaps the most extraordinary physics laboratories in the universe. Research on these extreme and exotic objects already has produced two Nobel Prizes. Pulsar researchers now are poised to learn otherwise-unavailable details of nuclear physics to test general relativity in conditions of extremely strong gravity, and to directly detect gravitational waves with a “telescope” nearly the size of our galaxy.

Neutron stars are the remnants of massive stars that exploded as supernovae. They pack more than the mass of the Sun into a sphere no larger than a medium-sized city, making them the densest objects in the universe, except for black holes, for which the concept of density is theoretically irrelevant. Pulsars are neutron stars that emit beams of radio waves outward from the poles of their magnetic fields. When their rotation spins a beam across Earth, radio telescopes detect that as a “pulse” of radio waves.

By precisely measuring the timing of such pulses, astronomers can use pulsars for unique “experiments” at the frontiers of modern physics.

Pulsars are at the forefront of research on gravity. Albert Einstein published his general theory of relativity in 1916, and his description of the nature of gravity has, so far, withstood numerous experimental tests. However, there are competing theories.

“Many of these alternate theories do just as good a job as general relativity of predicting behavior within our solar system. One area where they differ, though, is in the extremely dense environment of a neutron star,” said Ingrid Stairs from the University of British Columbia in Canada.

In some of the alternate theories, gravity’s behavior should vary based on the internal structure of the neutron star.

“By carefully timing pulsar pulses, we can precisely measure the properties of the neutron stars. Several sets of observations have shown that pulsars’ motions are not dependent on their structure, so general relativity is safe so far,” Stairs said.

Recent research on pulsars in binary-star systems with other neutron stars, and, in one case, with another pulsar, offers the best tests yet of general relativity in strong gravity. The precision of such measurements is expected to get even better in the future, Stairs said.

Another prediction of general relativity is that motions of masses in the universe should cause disturbances of space-time in the form of gravitational waves. Such waves have yet to be directly detected, but study of pulsars in binary-star systems have given indirect evidence for their existence. That work won a Nobel Prize in 1993.

Now, astronomers are using pulsars throughout our Milky Way Galaxy as a giant scientific instrument to directly detect gravitational waves.

“Pulsars are such extremely precise timepieces that we can use them to detect gravitational waves in a frequency range to which no other experiment will be sensitive,” said Benjamin Stappers from the University of Manchester in the United Kingdom.

By carefully timing the pulses from pulsars widely scattered within our galaxy, the astronomers hope to measure slight variations caused by the passage of the gravitational waves. The scientists hope such pulsar timing arrays can detect gravitational waves caused by the motions of supermassive pairs of black holes in the early universe, cosmic strings, and possibly from other exotic events in the first few seconds after the Big Bang.

“At the moment, we can only place limits on the existence of the very low-frequency waves we’re seeking, but planned expansion and new telescopes will, we hope, result in a direct detection within the next decade,” Stappers said.

With densities as much as several times greater than that in atomic nuclei, pulsars are unique laboratories for nuclear physics. Details of the physics of such dense objects are unknown.

“By measuring the masses of neutron stars, we can put constraints on their internal physics,” said Scott Ransom from the National Radio Astronomy Observatory in Socorro, New Mexico. “Just in the past three to four years, we’ve found several massive neutron stars that, because of their large masses, rule out some exotic proposals for what’s going on at the centers of neutron stars.”

The work is ongoing, and more measurements are needed. “Theorists are clever, so when we provide new data, they tweak their exotic models to fit what we’ve found,” Ransom said.

Pulsars were discovered in 1967, and that discovery earned the Nobel Prize in 1974.

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JOHN MOES from MICHIGAN said:
Pulsar periods and gravity waves from our own galaxy won't be stretched by expanding space, but won't both be greatly lengthened through 10 to 13 billion light years of expanding space?
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CHRIS R BAKER from CALIFORNIA said:
So has anyone actually detected gravity waves of any frequency? I don't see how the sensors I've seen described can possibly work since they depend on the speed of light relative to us not changing when the space they are traveling through changes from the passing gravity wave. What if the speed of the light changes with the length of the arm of the detector?
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MICHAEL HAMBURG from NEW YORK said:
It is interesting to note that it was a young English grad student, Jocelyn Bell, and her mentor, Anthony Hewish, who first feared they stumbled onto intelligent alien signals upon first detecting the pulses. They insisted on refering to the signals as "LGMs" (little green men). Only when they had detected the fourth source did they rightly conclude that the odds of four (!) alien civilizations simultaneously contacting the Earth was zero.
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SAM NAUMAN from TEXAS said:
Electromagnetic waves are generated when there are movements of electrical charges in magnetic fields or when the electrons in atoms are excited to a higher orbits and then they decay back giving their quantas of energy. The higher the energy, the higher the frequency of the waves. Now if the atoms are compressed what happens to the orbits of those electrons? Also how are the electromagnetic waves affected by the high density of the neutron stars. Then there is the spinning which is explained by the conservation of momentum. The smaller they shrink to the faster they spin. Why is it that the gravity waves have not been detected yet. Could it be that they do not exist?.
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LUCAS SANT'ANNA from CALIFORNIA said:
I wonder if these beams from pulsars would be harmful if they were closer to Earth, if of course they're not harmful now, in a miniscule amount.
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