JULY 11, 2024 by Netherlands Research School for Astronomy
Collected at: https://phys.org/news/2024-07-nearest-millisecond-pulsar-radius-kilometers.html
The nearest millisecond pulsar PSR J0437-4715 has a radius of 11.4 kilometers and a mass 1.4 times that of the sun. These are the results of precision measurements made by a team of researchers led by the University of Amsterdam (the Netherlands). The measurements reveal more about the composition and magnetic field of this neutron star. The researchers are publishing their findings in a series of scientific papers.
PSR J0437 is a pulsar, a rotating neutron star that emits electromagnetic radiation. It is located about 510 light-years from Earth in the southern constellation of Pictor. PSR J0437 rotates 174 times per second around its axis and has a white dwarf companion.
Like an out of control lighthouse, the pulsar sends a beam of radio waves and X-rays toward Earth every 5.75 milliseconds. This makes it the closest millisecond pulsar to Earth. It is also, in part because it is so close, the brightest millisecond pulsar. And it is a more stable clock than man-made atomic clocks.
Dutch national supercomputer
For their research, the scientists used data from the NICER X-ray telescope aboard the ISS. They combined the X-ray data with a technique called pulse profile modeling. To do this, they computed complex statistical models on the Dutch national supercomputer Snellius.
In the end, they were able to calculate the star’s radius, with the help of mass measurements made by Daniel Reardon (Swinburne University of Technology, Australia) and colleagues at the Parkes Pulsar Timing Array. They also mapped the temperature distribution of the magnetic poles.
Principal investigator Devarshi Choudhury (University of Amsterdam, the Netherlands) is pleased with the measurements: “Before, we were hoping to be able to calculate the radius accurately. And it would be great if we could show that the hot magnetic poles are not directly opposite each other on the stellar surface. And we just managed to do both.”
The researchers report that the new measurements indicate a “softer equation of state” than previously thought. By that, they mean that the maximum mass of neutron stars must be lower than some theories predict. “And that, in turn, fits nicely with what observations of gravitational waves seem to suggest,” said co-author and neutron star expert Anna Watts (University of Amsterdam).
Multiple scientific papers
The paper by Devarshi Choudhury and colleagues has been accepted for publication in The Astrophysical Journal Letters and appears on the preprint server arXiv.
It is part of a series of papers on millisecond pulsars. Among others, there is a forthcoming publication on an update to the radius measurement for the heavy pulsar PSR J0740+6620 led by Tuomo Salmi (University of Amsterdam), one on the equation of state by Nathan Rutherford (University of New Hampshire, U.S.), and one on mass determination by Daniel Reardon (Swinburne University of Technology, Australia). All three of these papers are currently available on the arXiv preprint server.
In addition, a paper on the mass and radius of PSR J0030 by Serena Vinciguerra (University of Amsterdam) appeared in early 2024 in The Astrophysical Journal.
More information: Devarshi Choudhury et al, A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437−4715, arXiv (2024). DOI: 10.48550/arxiv.2407.06789
Tuomo Salmi et al, The Radius of the High Mass Pulsar PSR J0740+6620 With 3.6 Years of NICER Data, arXiv (2024). DOI: 10.48550/arxiv.2406.14466
Nathan Rutherford et al, Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs, arXiv (2024). arxiv.org/abs/2407.06790
Daniel J. Reardon et al, The neutron star mass, distance, and inclination from precision timing of the brilliant millisecond pulsar J0437-4715, arXiv (2024). DOI: 10.48550/arxiv.2407.07132
Serena Vinciguerra et al, An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451, The Astrophysical Journal (2024). DOI: 10.3847/1538-4357/acfb83
Journal information: Astrophysical Journal , Astrophysical Journal Letters , arXiv
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