Nancy Neal Headquarters Washington July 2 2003 Phone 202/358-1547 Bill Steigerwald Goddard Space Flight Center Greenbelt Md Phone 301/286-5017 RELEASE 03-224 EINSTEIN GRAVITATIONAL WAVES MAY SET SPEED LIMIT FOR PULSAR SPIN Gravitational radiation ripples in the fabric of space predicted by Albert Einstein may serve as a cosmic traffic enforcer protecting reckless pulsars from spinning too fast and blowing apart according to a report published in the July 3 issue of Nature Pulsars the fastest spinning stars in the Universe are the core remains of exploded stars containing the mass of our Sun compressed into a sphere about 10 miles across Some pulsars gain speed by pulling in gas from a neighboring star reaching spin rates of nearly one revolution per millisecond or almost 20 percent light speed These millisecond pulsars would fly apart if they gained much more speed Using NASA Rossi X-ray Timing Explorer scientists have found a limit to how fast a pulsar spins and speculate that the cause is gravitational radiation The faster a pulsar spins the more gravitational radiation it might release as its exquisite spherical shape becomes slightly deformed This may restrain the pulsar rotation and save it from obliteration Nature has set a speed limit for pulsar spins said Prof Deepto Chakrabarty of the Massachusetts Institute of Technology MIT in Cambridge lead author on the journal article Just like cars speeding on a highway the fastest spinning pulsars could technically go twice as fast but something stops them before they break apart It may be gravitational radiation that prevents pulsars from destroying themselves Chakrabarty co-authors are Drs Edward Morgan Michael Muno and Duncan Galloway of MIT Rudy Wijnands University of St Andrews Scotland Michiel van der Klis University of Amsterdam and Craig Markwardt NASA Goddard Space Flight Center Greenbelt Md Wijnands also leads a second Nature letter complementing this finding Gravitational waves analogous to waves upon an ocean are ripples in four-dimensional spacetime These exotic waves predicted by Einstein theory of relativity are produced by massive objects in motion and have not yet been directly detected Created in a star explosion a pulsar is born spinning perhaps 30 times per second and slows down over millions of years Yet if the dense pulsar with its strong gravitational potential is in a binary system it can pull in material from its companion star This influx can spin up the pulsar to the millisecond range rotating hundreds of times per second In some pulsars the accumulating material on the surface occasionally is consumed in a massive thermonuclear explosion emitting a burst of X-ray light lasting only a few seconds In this fury lies a brief opportunity to measure the spin of otherwise faint pulsars Scientists report in Nature that a type of flickering found in these X-ray bursts called burst oscillations serves as a direct measure of the pulsars spin rate Studying the burst oscillations from 11 pulsars they found none spinning faster than 619 times per second The Rossi Explorer is capable of detecting pulsars spinning as fast as 4,000 times per second Pulsar breakup is predicted to occur at 1,000 to 3,000 revolutions per second Yet scientists have found none that fast From statistical analysis of 11 pulsars they concluded that the maximum speed seen in nature must be below 760 revolutions per second This observation supports the theory of a feedback mechanism involving gravitational radiation limiting pulsar speeds proposed by Prof Lars Bildsten of the University of California Santa Barbara As the pulsar picks up speed through accretion any slight distortion in the star dense half-mile-thick crust of crystalline metal will allow the pulsar to radiate gravitational waves Envision a spinning oblong rugby ball in water which would cause more ripples than a spinning spherical basketball An equilibrium rotation rate is eventually reached where the angular momentum shed by emitting gravitational radiation matches the angular momentum being added to the pulsar by its companion star Bildsten said that accreting millisecond pulsars could eventually be studied in greater detail in an entirely new way through the direct detection of their gravitational radiation LIGO the Laser Interferometer Gravitational-Wave Observatory now in operation in Hanford Wash and in Livingston La. will eventually be tunable to the frequency at which millisecond pulsars are expected to emit gravitational waves The waves are subtle altering spacetime and the distance between objects as far apart as the Earth and the Moon by much less than the width of an atom said Prof Barry Barish LIGO director from the California Institute of Technology Pasadena As such gravitational radiation has not been directly detected yet We hope to change that soon For animation images and more information visit the Internet at http://www.gsfc.nasa.gov/topstory/2003/0702pulsarspeed.html