Astronomers have developed a new technique to accurately determine the ages of millisecond pulsars, the fastest-spinning stars in the universe. The standard method for estimating pulsar ages is known to yield unreliable results, especially for the fast-spinning millisecond pulsars, said Bülent Kiziltan, a graduate student in astronomy and astrophysics at University of California Sant a Cruz. “An accurate determination of pulsar ages is of fundamental importance, because it has ramifications for understanding the formation and evolution of pulsars, the physics of neutron stars, and other areas,” he said.
Kiziltan has been working with Stephen Thorsett, professor of astronomy and astrophysics at UCSC, to study the evolution of millisecond pulsars. He presented their findings at the American Astronomical Society meeting in Pasadena on Monday, June 8.
A pulsar is a rapidly rotating neutron star, the collapsed core that remains after a massive star explodes as a supernova. The pulsar emits beams of radio waves (as well as x-rays and gamma-rays) from the magnetic poles of the neutron star. Because the magnetic poles are not aligned with the star’s spin axis, the beams sweep around like a lighthouse beacon, sending pulses of radio waves toward observers on Earth. The period between each pulse of radio waves corresponds to the rotation rate of the neutron star.
“In most cases, the only information we have is the radio pulse we receive from these compact stars. From these pulses we are trying to determine the ages, masses, and orbital parameters–a very challenging task indeed,” Kiziltan said.
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Ordinary pulsars tend to rotate a few times per second, and they gradually slow down with age, eventually becoming too faint to detect. Millisecond pulsars, however, rotate hundreds of time per second. They achieve these extraordinary spin rates by pulling in material from a binary companion star, a process that transfers angular momentum from the companion to the pulsar.
“This spin-up process is essentially like giving CPR to a dead or dying pulsar, giving it a second lease on life,” Kiziltan said.
The standard approach to determine the “characteristic” or “spin-down” age of a pulsar is based on two parameters: the period between pulses and the rate at which they slow down. Kiziltan and Thorsett showed that this method may over- or under-estimate the age of a pulsar by a factor of 10 when applied to millisecond pulsars.
To improve the accuracy of the standard technique, they incorporated additional constraints that arise from the spin-up process and physical limits on the maximum spin period. “We modified the age calculations to be consistent with these constraints and showed that this approach can achieve estimates closer to the true age of the pulsar,” Kiziltan said.
They show that, in some cases, millisecond pulsars that appear to be young can, in fact, be several billion years older. In other cases, young millisecond pulsars may mimic the characteristics of pulsars that are as old as the galaxy itself.
Sources: AAS, UCSC
3 Replies to “New Technique Reveals Ages of Millisecond Pulsars”
Coincidentally, an article appeared in the June 6th issue of Science News concerning the use of millisecond pulsars to detect long-period gravity waves (like those produced by the merger of two supermassive black holes). As explained in the article “A gravitational wave passing by the pulsar would warp spacetime, altering the arrival time of the radio waves at Earth ever so slightly. First the pulses would appear a little earlier, then a little later. The changes in arrival time would depend predictably on the phase and direction of propagation of the gravitational wave, as well as its distance from the pulsar. ”
“To detect a general background of gravitational waves, [it is estimated] astronomers would need to monitor 20 millisecond pulsars for five to 10 years, with the arrival time of the radio waves determined to an accuracy of 100 nanoseconds. Recording gravitational waves from a pair of merging supermassive black holes would require five pulsars with radio wave arrival times known to an even higher accuracy, [of about]10 nanoseconds.” It is pointed out that this is not a new idea, indeed dating back to the 1970’s. Even the head of the LISA project (the planned space-based GW observatory) is enthusiastic about the technique as it complements LISA and, as he points out, the hardware is already in place! Check out the NANOGrav site : http://www.nanograv.org/ . Amazing what astronomers can tease out of millisecond pulsars. Who knows, maybe this technique will be the first to detect this elusive radiation.
Forgot to mention the associated overview paper “Gravitational Wave Astronomy Using Pulsars” can be found here: http://nanograv.org/Files/Demorest_NANOGrav_CFP_GCT.pdf . Interesting stuff, indeed 🙂
Indeed! But I am still fascinated about the fact that we are able to “see” so many things in outer space. And we are just detecting a little amount of light!
We are able to time pulsars with such an accuracy that we can even check for delays of about 100ns. Wow!
Astronomy is really amazing!
Milli-second pulsars are a great topic. I love all these extream things, like black holes (including AGN) and neutron stars (with all the things that belong to them).
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