The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
Journal Article
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· The Astrophysical Journal. Letters
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- Univ. of Maryland, College Park, MD (United States); Stony Brook University
- Univ. of Illinois at Urbana-Champaign, IL (United States)
- Univ. of Maryland, College Park, MD (United States)
- Columbia Univ., New York, NY (United States)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- IRAP, CNRS (France); Univ. de Toulouse (France)
- Haverford College, PA (United States)
- Stony Brook Univ., NY (United States)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland, College Park, MD (United States)
- Univ. of Alberta, Edmonton, AB (Canada)
- U.S. Naval Research Lab., Washington, DC (United States)
- Univ. d'Orleans, Nancay (France); CNRS (France)
- Cornell Univ., Ithaca, NY (United States)
- McGill Univ., Montreal, QC (Canada); West Virginia Univ., Morgantown, WV (United States); Naval Research Lab., Washington, DC (United States)
- Naval Research Lab., Washington, DC (United States)
- Max-Planck-Inst. für Radioastronomie, Bonn (Germany)
- National Radio Astronomy Observatory, Charlottesville, VA (United States); Eötvös Loránd Univ., Budapest (Germany)
- National Radio Astronomy Observatory, Charlottesville, VA (United States)
- Univ. of British Columbia, Vancouver, BC (Canada)
PSR J0740+6620 has a gravitational mass of 2.08 ± 0.07 M⊙, which is the highest reliably determined mass of any neutron star. As a result, a measurement of its radius will provide unique insight into the properties of neutron star core matter at high densities. Here we report a radius measurement based on fits of rotating hot spot patterns to Neutron Star Interior Composition Explorer (NICER) and X-ray Multi-Mirror (XMM-Newton) X-ray observations. We find that the equatorial circumferential radius of PSR J0740+6620 is 13.7$$^{+2.6}_{–1.5}$$ km (68%). We apply our measurement, combined with the previous NICER mass and radius measurement of PSR J0030+0451, the masses of two other ~2 M⊙ pulsars, and the tidal deformability constraints from two gravitational wave events, to three different frameworks for equation-of-state modeling, and find consistent results at ~1.5-5 times nuclear saturation density. For a given framework, when all measurements are included, the radius of a 1.4 M⊙ neutron star is known to ±4% (68% credibility) and the radius of a 2.08 M⊙ neutron star is known to ±5%. The full radius range that spans the ±1σ credible intervals of all the radius estimates in the three frameworks is 12.45 ± 0.65 km for a 1.4 M⊙ neutron star and 12.35 ± 0.75 km for a 2.08 M⊙ neutron star.
- Research Organization:
- Research Foundation of New York, NY (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- Grant/Contract Number:
- FG02-87ER40317
- OSTI ID:
- 1864768
- Alternate ID(s):
- OSTI ID: 23154407
- Journal Information:
- The Astrophysical Journal. Letters, Journal Name: The Astrophysical Journal. Letters Journal Issue: 2 Vol. 918; ISSN 2041-8205
- Publisher:
- IOP PublishingCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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