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Magnetic Neutron Scattering and Spin-Polarized Neutrons

Magnetic Neutron Scattering and Spin-Polarized Neutrons

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Use trick to simplify this expression:1dp ip rcos22 eipr d p e d cosp0 1 2 sin p r 22 d p p r r0Here, p is an auxiliary variable without physical meaning.1 1 dp iprse 2 2 se re 2p1 ipr ˆ2 pse pˆe dp2 1 1 k s k dre dp p s p er 24Qˆs ˆe Q iQriprf e i ˆ 2 eˆs e The last line follows by doing the r -integration first <strong>and</strong> using 1 ipQr dr e 3 p Q2Q s esecollect all prefactors:2 2 mn 2 0 2 2 2 2NB 4 r024 15where r 02.810m is the “classical electron radius” that also appeared in theThompson cross section for x-ray scattering.d2 2r0 mf semidFor an unpolarized neutron beam, one has to average over the neutron spinstates m . For convenience, take the neutron spin quantization axis ẑ to beparallel to se. Then m s m s m mf ei ef z iseif mf mi 0 otherwiseThe cross section for a single electron at rest for an unpolarized neutron beamis therefored 2 r20sedwith the projection of the electron spin perpendicular to Q .se2


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Hax0where0ha ~ is theH2emagnetic flux quantuma~ 500Å for H 1TThe periodic magnetic field distribution generated by the flux line lattice insidethe superconductor can be revealed by magnetic neutron scattering. Becausethe lattice constant a is large, the scattering angle ~ is small. Even for cold2aneutrons ~5Å <strong>and</strong> relatively high magnetic fields H~ 1 T, is less than1°. In order to obtain the resolution required to separate the Bragg reflectionsfrom the unscattered beam, one uses a dedicated Small Angle <strong>Neutron</strong><strong>Scattering</strong> (SANS) diffractometer with a long distance (>10 m) between sample<strong>and</strong> detector:Small angle neutron diffraction patterns from flux lines lattice in a type-II superconductorNote that the structure of the flux line lattice changes as a function of magnetic field(M.R. Eskildsen et al., PRL 86, 320 (2001))As we have seen, nuclear <strong>and</strong> magnetic neutron scattering have comparablestrengths. They can be distinguished experimentally through three differentmethods:1 The magnetic form factor reduces the intensity of magnetic Bragg reflectionswith large K , whereas there is no form factor for nuclear scattering. Strongreflections with large K must therefore be nuclear in origin.2 <strong>Magnetic</strong> Bragg peaks vanish at the magnetic ordering temperature (theCurie temperature T C for ferromagnets, or the Néel temperature T N forantiferromagnets). Nuclear Bragg peaks vanish at the melting temperature,which is typically larger than T N or T C .3 The neutron spin operator does not appear the the cross section for coherentnuclear scattering. The neutron spin state is therefore unaffected by nuclearscattering. By contrast, magnetic neutron scattering can be (but does nothave to be) associated with a spin-flip of the neutron.5


For C C, only spin-up neutrons are reflected:ferromagnetic mirrornonmagnetic filmsmagnetic films<strong>Neutron</strong> reflectivity from nonmagnetic <strong>and</strong> magnetic filmshttp://www.orau.org/council/02presentations/klose.pdfFerromagnetic “supermirrors” with larger critical angles (see chapter on neutronreflectivity) are commonly used to produce spin-polarized neutrons in modernneutron scattering instruments:<strong>Polarized</strong>-beam reflectometerhttp://www.orau.org/council/02presentations/klose.pdf8


2 A method that has been developed in the past few years is the neutron spinfilter. A spin-polarized 3 He gas absorbs neutrons through the reaction3 4 3n He He ( S 0) pH .H 3 HeBecause the reaction proceeds via an intermediate state with S 0 , theabsorption cross section for neutrons with spins antiparallel to those of the3 Henuclei is therefore about three orders of magnitude larger than if neutron <strong>and</strong>3 He spins are parallel.9

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