Discovery Of 'Cosmic Chords' May Support Prediction Of Einstein's Theory

April 20, 1998

COLUMBUS, Ohio -- At a meeting of the American Physical Society today (April 20) astrophysicists announced that the discovery of very rapid oscillations in the brightness of some X-ray-emitting neutron stars has yielded important new constraints on the properties of the superdense matter at the centers of these stars. The data also may represent the first evidence for a unique effect of strongly curved space-time predicted by Einstein's theory of gravity but never before observed. The new measurements were made using NASA's Rossi X-Ray Timing Explorer satellite.

"The Rossi Explorer was designed to probe closer than ever before the strongly curved space-time near neutron stars and black holes," said Frederick Lamb, a professor of physics and of astronomy at the University of Illinois at Urbana-Champaign. "These new results are based on the earlier dramatic discovery by Rossi that the brightness of many neutron stars varies more than a thousand times each second. These variations are the highest frequency oscillations ever detected in any astrophysical object."

Neutron stars are the dense cinders left behind when stars of about 10 times the mass of the sun explode in violent events called supernovae. Neutron stars have masses about the same as the sun but are only about 10 miles in diameter.

Consequently, the matter at their centers is much denser even than the matter in atomic nuclei. According to Einstein's theory of gravity, space-time near neutron stars is strongly curved.

Observation of the effects of strongly curved space-time would be the first confirmation of a strong-field prediction of general relativity.

Many neutron stars are found in binary systems with ordinary stars like the sun, but the stars orbit so closely that the neutron stars are devouring their companion stars. The strong gravitational field of the neutron star literally pulls gas off the surface of the companion star. The gas then spirals toward the neutron star.

The high-frequency brightness oscillations are thought to be caused by clumps of gas hurtling around the neutron star just above its surface at speeds approaching the speed of light, Lamb said.

When gas from these clumps collides with the surface of the star, the gas reaches temperatures of 100 million degrees and emits X-rays. The neutron star becomes brighter when the heated gas is on the side facing us and dimmer when the heated gas is on the other side.

Some of the neutron stars that produce high frequency X-ray oscillations radiate more energy in a second that the sun radiates in a week. These stars can be seen all the way across the galaxy, using X-ray telescopes like those on the Rossi Explorer.

"We had expected to see a cacophony of frequencies in the X-ray emission from this violent caldron of hot gas, somewhat like the discord that results when you press your hands randomly on a piano keyboard," Lamb said. "Instead, scientists using the Rossi satellite found that these neutron stars are playing cosmic chords, with two or three nearly pure tones."

"The clockwork of the universe is much more orderly than we had dreamed," Lamb said. "The pureness of these tones makes it possible to use them to investigate how matter moves in the strongly curved space-time near these neutron stars."

At the meeting, Lamb presented calculations carried out with Coleman Miller, a research scientist at the University of Chicago, and Dimitrios Psaltis, a research scientist at the Harvard-Smithsonian Center for Astrophysics.

These calculations showed how the X-ray brightness oscillations could be used to determine the masses and dimensions of neutron stars and to look for evidence of the innermost stable orbit, a key prediction of general relativity.

The innermost stable orbit is a qualitatively new prediction of Einstein's theory of gravity. According to Newton's theory, gas can orbit a compact star at any distance. In contrast, Einstein's theory predicts that if the star is sufficiently massive and compact, there is a region of space around it where space-time is so strongly curved that there are no stable circular orbits. Gas orbiting this close to the star unavoidably plunges to its surface.

The calculations of Miller, Lamb and Psaltis show that the frequency of the X-ray brightness variations should increase as the gas flow onto the neutron star -- and hence its X-ray power -- rises, until the clumps producing the oscillations are at the innermost stable orbit. At this point the oscillation frequency should become constant as the X-ray power continues to rise. A paper describing the team's results has been accepted for publication in the Astrophysical Journal.

William Zhang, a research scientist at NASA's Goddard Space Flight Center, presented new observations obtained with the Rossi Explorer that appear consistent with the effects predicted by Miller, Lamb and Psaltis. Zhang and his colleagues observed the neutron star called 4U 1820-30 over several months and found that as its X-ray power rises, the frequency of its brightness oscillation increases until it is oscillating about 1,050 times a second. As the X-ray power increases further, the frequency remains constant, indicating that the innermost stable orbit has been reached. The results obtained by Zhang's team also have been accepted for publication in the Astrophysical Journal.

"There is a good possibility that the Rossi Explorer has provided the first evidence supporting the predictions of Einstein's theory of gravity about how matter moves in strongly curved space-time," Lamb said. "All previous tests of general relativity have been made in regions where space-time is curved only very, very weakly. Searching for effects of strong gravitational fields is of fundamental importance. If this evidence for the existence of an innermost stable orbit is confirmed, it will be a major advance."

"Studying how matter moves in the strongly curved space-time near neutron stars also has allowed us to extract interesting new bounds on the masses and dimensions of these stars and on the stiffness of the superdense matter inside them," Lamb said. "The new evidence reported today suggests that the strong nuclear force is more repulsive than many nuclear physicists had expected and that the superdense matter in neutron stars is rather stiff."

While these new findings represent a very important and exciting development, they will require confirmation, Lamb cautioned.
-end-
CONTACT: Frederick Lamb can be contacted at the University of Illinois, department of physics, (217) 333-6363 or f-lamb@uiuc.edu, until noon Friday (April 17). Lamb can be contacted at (937) 390-2176 on Saturday (April 18). Lamb will be staying at the Hyatt Regency Columbus Hotel, 350 N. High St., (614) 463-1234, from Sunday to Tuesday (April 19-21).

Color pictures available on the WWW at: http://www.physics.uiuc.edu/groups/tastro/movies/spm/



University of Illinois at Urbana-Champaign

Related Neutron Star Articles from Brightsurf:

Black hole or no black hole: On the outcome of neutron star collisions
A new study lead by GSI scientists and international colleagues investigates black-hole formation in neutron star mergers.

UMD astronomers find x-rays lingering years after landmark neutron star collision
It's been three years since the landmark detection of a neutron star merger from gravitational waves.

Microscopic deformation of a neutron star inferred from a distance of 4500 light-years
Gravitational waves, which are ripples in spacetime, have recently provided a new window to the universe.

Method proposed for more accurate determinations of neutron star radii
Neutron stars are the smallest and densest astrophysical objects with visible surfaces in the Universe.

Unequal neutron-star mergers create unique "bang" in simulations
In a series of simulations, an international team of researchers determined that some neutron star collisions not only produce gravitational waves, but also electromagnetic radiation that should be detectable on Earth.

ALMA finds possible sign of neutron star in supernova 1987A
Based on ALMA observations and a theoretical follow-up study, scientists suggest that a neutron star might be hiding deep inside the remains of Supernova 1987A.

Scientists discover pulsating remains of a star in an eclipsing double star system
Scientists from the University of Sheffield have discovered a pulsating ancient star in a double star system, which will allow them to access important information on the history of how stars like our Sun evolve and eventually die.

How big is the neutron?
The size of neutrons cannot be measured directly: it can only be determined from experiments involving other particles.

The force is strong in neutron stars
Physicists at MIT and elsewhere have for the first time characterized the strong nuclear force, and the interactions between protons and neutrons, at extremely short distances.

New neutron detector can fit in your pocket
Researchers at Northwestern University and Argonne National Laboratory have developed a new material that opens doors for a new class of neutron detectors.

Read More: Neutron Star News and Neutron Star Current Events
Brightsurf.com is a participant in the Amazon Services LLC Associates Program, an affiliate advertising program designed to provide a means for sites to earn advertising fees by advertising and linking to Amazon.com.