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Neutron Star Structure from Pulsar Observations∗

Published online by Cambridge University Press:  14 August 2015

David Pines ,
Jacob Shaham  and
Malvin A. Ruderman
David Pines
Affiliation:
Dept. of Physics, University of Illinois at Urbana-Champaign
Jacob Shaham*
Affiliation:
Dept. of Physics, University of Illinois at Urbana-Champaign
Malvin A. Ruderman
Affiliation:
Dept. of Physics, Columbia University, New York, N.Y., U.S.A.
*
∗∗ Present address: Racah Institute of Physics, Hebrew University, Jerusalem, Israel.

Abstract

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We examine what inferences can be made regarding neutron star structure from observations of micro- and macroglitch behavior. After considering various theories it seems plausible that crustquakes offer an explanation for the Crab microglitches, while corequakes can explain the Vela macroglitches. It is concluded that the Crab pulsar has a mass of less than 0.5 M ⊙ and is ∼ 90% superfluid neutrons while the Vela pulsar may possess a solid neutron core and have a mass of ∼ 0.7 M ⊙ with a superfluid neutron abundance of ∼ 15%.

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 53: Physics of Dense Matter , 1974 , pp. 189 - 207
Copyright
Copyright © Reidel 1974 

Footnotes

∗

Presented by D. Pines

References

Baym, G., Pethick, C. J., and Pines, D.: 1969a, Nature 223, 673.CrossRefGoogle Scholar
Baym, G., Pethick, C. J., Pines, D., and Ruderman, M.: 1969b, Nature 224, 872.CrossRefGoogle Scholar
Baym, G., Pethick, C. J., and Sutherland, P.: 1971, Astrophys. J. 170, 299.CrossRefGoogle Scholar
Baym, G. and Pines, D.: 1971, Ann. Phys. 66, 816.CrossRefGoogle Scholar
Boynton, P. E., Groth, E. J., Hutchinson, D. P., Nanos, G. P. Jr., Partridge, R. B., and Wilkinson, D. T.: 1972, Astrophys. J. 175, 217.CrossRefGoogle Scholar
Colgate, S.: 1972 (private communication).Google Scholar
Dyson, F. J.: 1969, Nature 223, 486.CrossRefGoogle Scholar
Dyson, F. J.: 1970, Lectures at the Scuola Normale Superiore, Pisa.Google Scholar
Feibelman, P. J.: 1971, Phys. Rev. 4, 1589D.Google Scholar
Greenstein, G. S.: 1970, Nature 227, 791.CrossRefGoogle Scholar
Greenstein, G. S. and Cameron, A. G. W.: 1969, Nature 222, 862.CrossRefGoogle Scholar
Groth, E.: 1971, .Google Scholar
Lamb, F., Pethick, C. J., and Pines, D.: 1973, Astrophys. J. 184, 271.CrossRefGoogle Scholar
Lohsen, E.: 1971, IAU Circ. No. 2368.Google Scholar
Lohsen, E.: 1972, Nature Phys. Sci. 236, 70.CrossRefGoogle Scholar
Michel, F. C.: 1970, Astrophys. J. 159, 225.CrossRefGoogle Scholar
Nelson, J., Hills, R., Cudaback, D., and Wampler, J.: 1970, Astrophys. J. Letters 161, L235.CrossRefGoogle Scholar
Packard, R. E.: 1972, Phys. Rev. Letters 28, 1080.CrossRefGoogle Scholar
Papliolios, C., Carleton, N. P., and Horowitz, P.: 1970, Nature 228, 445.CrossRefGoogle Scholar
Papliolios, C., Carleton, N. P., and Horowitz, P.: 1971, IAU Circ. No. 2368.Google Scholar
Pines, D. and Shaham, J.: 1972a, Nature Phys. Sci. 235, 43.CrossRefGoogle Scholar
Pines, D. and Shaham, J.: 1972b, Phys. Earth Planetary Interiors 6, 103.CrossRefGoogle Scholar
Pines, D., Shaham, J., and Ruderman, M.: 1972, Nature Phys. Sci. 237, 83.CrossRefGoogle Scholar
Radhakrishnan, V. and Manchester, R. N.: 1969, Nature 222, 228.CrossRefGoogle Scholar
Rees, M. J., Trimble, V. L., and Cohen, J. M.: 1971, Nature 229, 395.CrossRefGoogle Scholar
Reichley, P. E.: 1970, talk at URSI Meeting, Washington.Google Scholar
Reichley, P. E. and Downs, G. S.: 1969, Nature 222, 229.CrossRefGoogle Scholar
Reichley, P. E. and Downs, G. S.: 1971, Nature Phys. Sci. 234, 48.CrossRefGoogle Scholar
Richards, D. W., Pettengill, G. H., Roberts, J. A., Counselman, C. C. III, and Rankin, J. M.: 1969, IAU Circ. No. 2181.Google Scholar
Roberts, D. H. and Sturrock, P. A.: 1971, Bull. Am. Astron. Soc. 3, 463.Google Scholar
Rosenbluth, M.: 1972 (private communication).Google Scholar
Ruderman, M.: 1969, Nature 223, 597.CrossRefGoogle Scholar
Ruderman, M.: 1972, Ann. Rev. Astron. Astrophys. 10, 427.CrossRefGoogle Scholar
Sawyer, R. F.: 1972, Phys. Rev. Letters 29, 382.CrossRefGoogle Scholar
Sawyer, R. F. and Scalapino, P. J.: 1973, Phys. Rev. D7, 1579.Google Scholar
Scalapino, P. J.: 1972, Phys. Rev. Letters 29, 386.CrossRefGoogle Scholar
Scargle, J. D. and Pacini, F.: 1971, Nature Phys. Sci. 232, 144.CrossRefGoogle Scholar
Shvartzman, V. F.: 1971, Soviet Astron. 15, 342.Google Scholar