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Role of Hyperons in Neutron Stars · Around

2010

Role of Hyperons in Neutron Stars

Stone, J. R., Guichon, P. A. M., Thomas, A. W.

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The latest observation of a Shapiro delay of the binary millisecond pulsar J1614-2230 by Demorest et al.

Nature 467 1081 (2010) yielded the pulsar gravitational mass to be 1.97 +/- 0.04 solar mass, the heaviest observed pulsar to-date.
This result produces a stringent constraint on Equation(s) of State (EoS) of high density neutron star matter.
One of the main conclusions of Demorest et al.

Built on

P. A. M. Guichon, A. W. Thomas and K. Tsushima, Nucl. Phys. A814, 66 (2008) [arXiv:0712.1925 [nucl-th]]
Original
1925
Earlier work this paper cites.
B. D. Lackey, M. Nayyar and B. J. Owen, Phys. Rev. D 73, 024021 (2006)
2006
Earlier work this paper cites.

Similar

P. A. M. Guichon, H. H. Matevosyan, N. Sandulescu and A. W. Thomas, Nucl. Phys. A 772, 1 (2006)
2006
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J. R. Stone, P. A. M. Guichon, H. H. Matevosyan and A. W. Thomas, Nucl. Phys. A 792, 341(2007)
2007
Cited alongside, same era.
M. Dutra, O. Lourenco, J. S. S. Martins, A. Delfino, J. R. Stone, P. D. Stevenson and C. Providencia, to be submitted to Phys. Rev. C
Cited in the paper.

Then

P. B. Demorest, T. Pennucci, S. M. Ransom, M. S. E. Roberts and J. W. T. Hessels, Nature 467, 1081 (2010)
2010
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