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A two-solar-mass neutron star measured using Shapiro delay

Open access
Demorest, P. B., Pennucci, T., Ransom, S. M., Roberts, M. S. E., Hessels, J. W. T.·2010·Nature

Abstract

Neutron stars are composed of the densest form of matter known to exist in our universe, and thus provide a unique laboratory for exploring the properties of cold matter at supranuclear density. Measurements of the masses or radii of these objects can strongly constrain the neutron-star matter equation of state, and consequently the interior composition of neutron stars[1, 2]. Neutron stars that are visible as millisecond radio pulsars are especially useful in this respect, as timing observations of the radio pulses provide an extremely precise probe of both the pulsar’s motion and the surrounding space-time metric. In particular, for a pulsar in a binary system, detection of the general relativistic Shapiro delay allows us to infer the masses of both the neutron star and its binary

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Metadata

Authors
Demorest, P. B., Pennucci, T., Ransom, S. M., Roberts, M. S. E., & Hessels, J. W. T.
Venue
Nature
Published
2010-10
Volume
467
Issue
7319
Pages
1081-1083
ISSN
  • 0028-0836 (ISSN-L)
  • 1476-4687
OpenAlex
W2092350553
Cited by
3,905
References
1
FWCI
107.59
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: A two-solar-mass neutron star measured using Shapiro delay. https://app.cochat.ai/papers/10.1038/nature09466
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Demorest, P. B., Pennucci, T., Ransom, S. M., Roberts, M. S. E., & Hessels, J. W. T. (2010). A two-solar-mass neutron star measured using Shapiro delay. Nature. https://doi.org/10.1038/nature09466

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