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Toroidal configuration of the orbit of the electron of the hydrogen ...

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For example, at small intensities, B ≃ 2.4 · 10 4 Gauss = 2.4 Tesla, <strong>the</strong>parameter γ = eH/2¯hc ≃ 1.7·10 11 cm −2 so that for 〈r〉 ≃ 0.5·10 −8 cm we get<strong>the</strong> estimation γ 2 〈r 2 〉 ≃ 10 6 cm −2 and Landau energy ¯hΩ/2 is <strong>of</strong> <strong>the</strong> order<strong>of</strong> 10 −4 eV, while at high intensities, B ≃ B 0 = 2.4 · 10 9 Gauss = 2.4 · 10 5Tesla, <strong>the</strong> parameter γ = γ 0 ≃ 1.7 · 10 16 cm −2 so that <strong>the</strong> estimations are:γ 2 〈r 2 〉 ≃ 10 16 cm −2 (greater by ten orders) and <strong>the</strong> ground Landau energy isabout 13.6 eV (greater by five orders).Below, we turn to approximate ground state solution <strong>of</strong> Eq. (3.1) for <strong>the</strong>case <strong>of</strong> very strong magnetic field.3.1 Very strong magnetic fieldLet us consider <strong>the</strong> approximation <strong>of</strong> a very strong magnetic field,B ≫ B 0 = 2.4 · 10 9 Gauss. (3.2)Under <strong>the</strong> above condition, in <strong>the</strong> transverse plane <strong>the</strong> Coulomb interaction<strong>of</strong> <strong>the</strong> <strong>electron</strong> with <strong>the</strong> nucleus is not important in comparison with <strong>the</strong>interaction <strong>of</strong> <strong>the</strong> <strong>electron</strong> with <strong>the</strong> external magnetic field. So, in accord to<strong>the</strong> exact solution (2.6) for a single <strong>electron</strong>, one can seek for an approximateground state solution <strong>of</strong> Eq. (3.1) in <strong>the</strong> form (see, e.g. [1]) <strong>of</strong> factorizedtransverse and longitudinal parts,ψ = e −γr2 /2 χ(z), (3.3)where we have used Landau wave function (2.14), s = 0, l = 0, and χ(z)denotes <strong>the</strong> longitudinal wave function to be found. This is so called adiabaticapproximation. The charge distribution <strong>of</strong> <strong>the</strong> <strong>electron</strong> in <strong>the</strong> (r, ϕ) planeis thus characterized by <strong>the</strong> Landau wave function ∼ e −γr2 /2 , i.e. by <strong>the</strong>azimuthal symmetry.In general, <strong>the</strong> adiabatic approximation corresponds to <strong>the</strong> case when <strong>the</strong>transverse motion <strong>of</strong> <strong>electron</strong> is totally determined by <strong>the</strong> intense magneticfield, which makes it ”dance” at its cyclotron frequency. Specifically, <strong>the</strong>radius <strong>of</strong> <strong>the</strong> <strong>orbit</strong> is <strong>the</strong>n much smaller than <strong>the</strong> Bohr radius, R 0 ≪ a 0 , or,equivalently, <strong>the</strong> Landau energy <strong>of</strong> <strong>electron</strong> is much bigger than <strong>the</strong> Bohrenergy E0⊥ ≫ |E0 Bohr | = 13.6 eV. In o<strong>the</strong>r words, this approximation meansthat <strong>the</strong> interaction <strong>of</strong> <strong>electron</strong> with <strong>the</strong> nucleus in <strong>the</strong> transverse plane isignorably small (it is estimated to make about 2% correction at B ≃ 10 1211

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