The observed large rates of spinning down after glitches in some radio pulsars have been previously explained in terms of a long-term spin-up behavior of a superfluid part of the crust of neutron stars. We argue that the suggested mechanism is not viable; being inconsistent with the basic requiremen
On the genesis of Post constraint in modern electromagnetism
β Scribed by Akhlesh Lakhtakia
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 795 KB
- Volume
- 115
- Category
- Article
- ISSN
- 0030-4026
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