[9f60c06] | 1 | .. _magnetism: |
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| 2 | |
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| 3 | Polarisation/Magnetic Scattering |
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[990d8df] | 4 | ================================ |
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[9f60c06] | 5 | |
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[990d8df] | 6 | Models which define a scattering length density parameter can be evaluated |
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| 7 | as magnetic models. In general, the scattering length density (SLD = |
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| 8 | $\beta$) in each region where the SLD is uniform, is a combination of the |
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| 9 | nuclear and magnetic SLDs and, for polarised neutrons, also depends on the |
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| 10 | spin states of the neutrons. |
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[9f60c06] | 11 | |
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| 12 | For magnetic scattering, only the magnetization component $\mathbf{M_\perp}$ |
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[524e5c4] | 13 | perpendicular to the scattering vector $\mathbf{Q}$ contributes to the magnetic |
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[9f60c06] | 14 | scattering length. |
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| 15 | |
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| 16 | |
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| 17 | .. figure:: |
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[0cd9158] | 18 | mag_img/mag_vector.png |
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[9f60c06] | 19 | |
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| 20 | The magnetic scattering length density is then |
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| 21 | |
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| 22 | .. math:: |
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| 23 | \beta_M = \dfrac{\gamma r_0}{2\mu_B}\sigma \cdot |
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| 24 | \mathbf{M_\perp} = D_M\sigma \cdot \mathbf{M_\perp} |
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| 25 | |
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| 26 | where $\gamma = -1.913$ is the gyromagnetic ratio, $\mu_B$ is the |
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| 27 | Bohr magneton, $r_0$ is the classical radius of electron, and $\sigma$ |
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| 28 | is the Pauli spin. |
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| 29 | |
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| 30 | Assuming that incident neutrons are polarized parallel (+) and anti-parallel (-) |
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| 31 | to the $x'$ axis, the possible spin states after the sample are then |
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| 32 | |
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[2c108a3] | 33 | Non spin-flip (+ +) and (- -) |
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[9f60c06] | 34 | |
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[2c108a3] | 35 | Spin-flip (+ -) and (- +) |
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[9f60c06] | 36 | |
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| 37 | .. figure:: |
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[0cd9158] | 38 | mag_img/M_angles_pic.png |
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[9f60c06] | 39 | |
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| 40 | If the angles of the $Q$ vector and the spin-axis $x'$ to the $x$ - axis are |
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| 41 | $\phi$ and $\theta_{up}$, respectively, then, depending on the spin state of the |
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| 42 | neutrons, the scattering length densities, including the nuclear scattering |
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[2c108a3] | 43 | length density $(\beta{_N})$ are |
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[9f60c06] | 44 | |
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| 45 | .. math:: |
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| 46 | \beta_{\pm\pm} = \beta_N \mp D_M M_{\perp x'} |
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[2c108a3] | 47 | \text{ for non spin-flip states} |
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[9f60c06] | 48 | |
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| 49 | and |
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| 50 | |
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| 51 | .. math:: |
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| 52 | \beta_{\pm\mp} = -D_M (M_{\perp y'} \pm iM_{\perp z'}) |
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[2c108a3] | 53 | \text{ for spin-flip states} |
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[9f60c06] | 54 | |
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| 55 | where |
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| 56 | |
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| 57 | .. math:: |
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[2c108a3] | 58 | M_{\perp x'} &= M_{0q_x}\cos(\theta_{up})+M_{0q_y}\sin(\theta_{up}) \\ |
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| 59 | M_{\perp y'} &= M_{0q_y}\cos(\theta_{up})-M_{0q_x}\sin(\theta_{up}) \\ |
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| 60 | M_{\perp z'} &= M_{0z} \\ |
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| 61 | M_{0q_x} &= (M_{0x}\cos\phi - M_{0y}\sin\phi)\cos\phi \\ |
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| 62 | M_{0q_y} &= (M_{0y}\sin\phi - M_{0x}\cos\phi)\sin\phi |
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[9f60c06] | 63 | |
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| 64 | Here, $M_{0x}$, $M_{0x}$, $M_{0z}$ are the x, y and z components |
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| 65 | of the magnetization vector given in the laboratory xyz frame given by |
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| 66 | |
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| 67 | .. math:: |
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[2c108a3] | 68 | M_{0x} &= M_0\cos\theta_M\cos\phi_M \\ |
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| 69 | M_{0y} &= M_0\sin\theta_M \\ |
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| 70 | M_{0z} &= -M_0\cos\theta_M\sin\phi_M |
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[9f60c06] | 71 | |
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| 72 | and the magnetization angles $\theta_M$ and $\phi_M$ are defined in |
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| 73 | the figure above. |
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| 74 | |
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| 75 | The user input parameters are: |
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| 76 | |
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| 77 | =========== ================================================================ |
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| 78 | M0_sld = $D_M M_0$ |
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[1f058ea] | 79 | Up_theta = $\theta_\mathrm{up}$ |
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[9f60c06] | 80 | M_theta = $\theta_M$ |
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| 81 | M_phi = $\phi_M$ |
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| 82 | Up_frac_i = (spin up)/(spin up + spin down) neutrons *before* the sample |
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| 83 | Up_frac_f = (spin up)/(spin up + spin down) neutrons *after* the sample |
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| 84 | =========== ================================================================ |
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| 85 | |
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| 86 | .. note:: |
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| 87 | The values of the 'Up_frac_i' and 'Up_frac_f' must be in the range 0 to 1. |
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| 88 | |
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[59485a4] | 89 | *Document History* |
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[990d8df] | 90 | |
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[59485a4] | 91 | | 2015-05-02 Steve King |
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[990d8df] | 92 | | 2017-05-08 Paul Kienzle |
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