Constraining the dense matter equation-of-state with radio pulsars Article Swipe
H. Hu
,
M. Krämer
,
Norbert Wex
,
D. J. Champion
,
M. S. Kehl
·
YOU?
·
· 2020
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staa2107
YOU?
·
· 2020
· Open Access
·
· DOI: https://doi.org/10.1093/mnras/staa2107
Radio pulsars provide some of the most important constraints for our understanding of matter at supranuclear densities. So far, these constraints are mostly given by precision mass measurements of neutron stars (NS). By combining single measurements of the two most massive pulsars, J0348+0432 and J0740+6620, the resulting lower limit of 1.98 M⊙ (99 per cent confidence) of the maximum NS mass, excludes a large number of equations of state (EOSs). Further EOS constraints, complementary to other methods, are likely to come from the measurement of the moment of inertia (MOI) of binary pulsars in relativistic orbits. The Double Pulsar, PSR J0737−3039A/B, is the most promising system for the first measurement of the MOI via pulsar timing. Reviewing this method, based in particular on the first MeerKAT observations of the Double Pulsar, we provide well-founded projections into the future by simulating timing observations with MeerKAT and the SKA. For the first time, we account for the spin-down mass-loss in the analysis. Our results suggest that an MOI measurement with 11 per cent accuracy (68 per cent confidence) is possible by 2030. If by 2030 the EOS is sufficiently well known, however, we find that the Double Pulsar will allow for a 7 per cent test of Lense–Thirring precession, or alternatively provide a ∼3σ-measurement of the next-to-leading order gravitational wave damping in GR. Finally, we demonstrate that potential new discoveries of double NS systems with orbital periods shorter than that of the Double Pulsar promise significant improvements in these measurements and the constraints on NS matter.
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- Language
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- Landing Page
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- https://academic.oup.com/mnras/article-pdf/497/3/3118/33647350/staa2107.pdf
- OA Status
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- OpenAlex ID
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All OpenAlex metadata
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- DOI
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https://doi.org/10.1093/mnras/staa2107Digital Object Identifier
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Constraining the dense matter equation-of-state with radio pulsarsWork title
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articleOpenAlex work type
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enPrimary language
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2020Year of publication
- Publication date
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2020-07-16Full publication date if available
- Authors
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H. Hu, M. Krämer, Norbert Wex, D. J. Champion, M. S. KehlList of authors in order
- Landing page
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https://doi.org/10.1093/mnras/staa2107Publisher landing page
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https://academic.oup.com/mnras/article-pdf/497/3/3118/33647350/staa2107.pdfDirect link to full text PDF
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://academic.oup.com/mnras/article-pdf/497/3/3118/33647350/staa2107.pdfDirect OA link when available
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Physics, Pulsar, Equation of state, Astrophysics, Astronomy, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
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57Total citation count in OpenAlex
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2025: 5, 2024: 18, 2023: 16, 2022: 7, 2021: 10Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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