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- W2021880802 abstract "In huge magnetic fields ($Bensuremath{gtrsim}{10}^{12}$ G) matter forms a tightly bound, dense ($ensuremath{gtrsim}{10}^{4}$ g ${mathrm{cm}}^{ensuremath{-}3}$) solid with properties of a one-dimensional metal and a work function of the order of a keV. Electron field emission from the sharp surface of a pulsar is much easier than ion emission; it is estimated to be cut off when the stellar rotation period exceeds several seconds." @default.
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- W2021880802 date "1971-11-08" @default.
- W2021880802 modified "2023-10-18" @default.
- W2021880802 title "Matter in Superstrong Magnetic Fields: The Surface of a Neutron Star" @default.
- W2021880802 cites W1970867611 @default.
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- W2021880802 doi "https://doi.org/10.1103/physrevlett.27.1306" @default.
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