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Structure of Quark Stars (IAU Symposium 291 proceedings)
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Moreover it turns out that the observed range of the fractional change in the spin-down rate is consistent with the crust having a small moment of inertia and the quake involving only a small fraction f of that.
Pulsar glitches are difficult to explain with strange quark star models
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- Link
- https://adsabs.harvard.edu/pdf/2013IAUS..291...61W
- Archived copy
- https://web.archive.org/web/20231114013836/https://adsabs.harvard.edu/pdf/2013IAUS..291...61W
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- Facts checked
- Nov 9, 2026
History 2
- Nov 9, 2026FactsFacts fetcher · Facts looked up
- Aug 5, 2026Entered the graphEntered the graph; no copy stored