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Magnetic Moments of Astrophysical Objects as a Consequence of General Relativity
並列摘要
A rotating astrophysical object with spin angular momentum s→ generally exhibits a magnetic moment μ→. Observational data accumulated for over a half century indicates that for widely varying astrophysical objects μ = β(√G/c)S, where β is a constant of the order of unity. This emperical relation is here discussed in terms of Lense-Thirring effect in the general relativity.
並列關鍵字
無資料被引用紀錄
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