Publication Abstracts

Canuto and Chitre 1973

Canuto, V., and S.M. Chitre, 1973: Solid core in neutron stars. Nat. Phys. Sci., 243, no. 126, 63-65, doi:10.1038/physci243063a0.

The identification of pulsars as rotating neutron stars has led to an increased interest in the structure calculation of neutron stars. It may be said with reasonable confidence that the state of matter in the outer regions of a neutron star is relatively well understood, while our knowledge of the equation of state in the density range upwards of 1015 g/cm3 is still far from clear.

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BibTeX Citation

  author={Canuto, V. and Chitre, S. M.},
  title={Solid core in neutron stars},
  journal={Nature Physical Science},

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RIS Citation

ID  - ca07920l
AU  - Canuto, V.
AU  - Chitre, S. M.
PY  - 1973
TI  - Solid core in neutron stars
JA  - Nat. Phys. Sci.
JO  - Nature Physical Science
VL  - 243
IS  - 126
SP  - 63
EP  - 65
DO  - 10.1038/physci243063a0
ER  -

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