迈斯纳效应由瓦尔特-迈斯纳(Walther Meissner)和罗伯特-奥克森菲尔德(Robert Ochsenfeld)于 1933 年发现,是指超导体在过渡到超导状态的过程中,磁场从超导体中被驱除。当材料冷却到临界温度([latex]T_c[/latex])以下并存在微弱的外部磁场时,它会主动抵消其内部的所有磁通量,成为一个完美的二元磁体。.

(图片仅供参考)
迈斯纳效应由瓦尔特-迈斯纳(Walther Meissner)和罗伯特-奥克森菲尔德(Robert Ochsenfeld)于 1933 年发现,是指超导体在过渡到超导状态的过程中,磁场从超导体中被驱除。当材料冷却到临界温度([latex]T_c[/latex])以下并存在微弱的外部磁场时,它会主动抵消其内部的所有磁通量,成为一个完美的二元磁体。.
The Meissner effect is a defining characteristic of superconductivity, distinguishing it from a hypothetical perfect conductor. A perfect conductor, according to Lenz’s law, would trap any existing magnetic field inside it as it cools, because changing the flux would induce currents to oppose the change. In contrast, a superconductor actively expels the field. This expulsion is achieved by the generation of screening currents on the surface of the material. These currents create a magnetic field that perfectly cancels the external field within the bulk of the superconductor. The magnetic field penetrates only a small distance into the surface, known as the London penetration depth ([latex]\lambda[/latex]). This discovery was crucial because it showed that superconductivity is a true thermodynamic phase transition, not just a case of infinite conductivity. It provided a key piece of the puzzle that any microscopic theory of superconductivity would have to explain. The effect is the basis for the dramatic levitation demonstrations where a magnet floats above a high-temperature superconductor cooled with liquid nitrogen. The expulsion of the magnet’s field by the superconductor creates a repulsive force strong enough to counteract gravity.
当施加的磁场过强时,迈斯纳效应会失效。对于I型超导体,超导性在超过临界磁场[latex]H_c[/latex]后会突然消失。对于II型超导体,在超过较低临界磁场[latex]H_{c1}[/latex]后,磁场开始以量子化磁通涡旋的形式渗透到材料内部,而材料则保持超导状态直至超过更高的较高临界磁场[latex]H_{c2}[/latex]。
迈斯纳效应
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