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The Hall Effect LL8 Section 22. A conductor in an external magnetic field H Onsager’s principle doesn’t hold Instead v.5 section 120, and v.2: Time- reversal.

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Presentation on theme: "The Hall Effect LL8 Section 22. A conductor in an external magnetic field H Onsager’s principle doesn’t hold Instead v.5 section 120, and v.2: Time- reversal."— Presentation transcript:

1 The Hall Effect LL8 Section 22

2 A conductor in an external magnetic field H Onsager’s principle doesn’t hold Instead v.5 section 120, and v.2: Time- reversal symmetry only if H -H

3 Separate conductivity tensor into symmetric and antisymmetric parts. This is always possible for a rank 2 tensor. But

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5 a ik has only 3 components, like a vector. Any antisymmetric a ik is dual to an axial vector, which has no sigh change under inversion

6 Joule heat Determined for given E only by the symmetrical part of  ik.

7 External H-fields are usually weak. Expand  (H) in powers of H. a(H) is odd, so it contains only odd powers of H. axial Ordinary polar tensor, product of components that change sign under inversion, x -> -x, etc. axial

8 s ik (H) is even. Expansion of s ik has only even powers Zero-field conductivity tensor Symmetrical in (i,k) and in (l,m)

9 First order effect of H-field is linear in H. This term might also have a component perpendicular to E.

10 Inverse formula Symmetric part Resistivity tensor Antisymmetric part

11 Math arguments repeat First term is ordinary Ohm’s law Second term gives Hall effect – The axial vector b – dual to b ik – Linear in H for small H

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13 For isotropic conductor, including cubic semiconductors Axial vectors a and b must be parallel to H More generally,

14 Symmetry: All tensors that characterize an isotropic medium must be invariant under all rotations about H

15 Likewise, symmetric parts of conductivity and resistivity tensors must be invariant under rotations about H

16 Let j lie in the xz plane x

17 In an isotropic conductor, the Hall field is the only E-field that is perpendicular to both j and H.

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19 Next terms in expansion of  ik j k must be – quadratic in H, – linear in j, – And be a vector Only possible combinations of H & J are

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