2017
DOI: 10.1103/physrevlett.119.106401
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Strong Linear Dichroism in Spin-Polarized Photoemission from Spin-Orbit-Coupled Surface States

Abstract: A comprehensive understanding of spin-polarized photoemission is crucial for accessing the electronic structure of spin-orbit coupled materials. Yet, the impact of the final state in the photoemission process on the photoelectron spin has been difficult to assess in these systems. We present experiments for the spin-orbit split states in a Bi-Ag surface alloy showing that the alteration of the final state with energy may cause a complete reversal of the photoelectron spin polarization. We explain the effect on… Show more

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Cited by 41 publications
(30 citation statements)
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“…For the as-deposited sample (300 K), we observed a single spin-orbit split peak (red) at binding energies of ∼23.74 eV (Bi-5d 5/2 ) and ∼26.79 eV (Bi-5d 3/2 ), i.e., the magnitude of the spin-orbit split amounts to ∼3.05 eV. Irrespective of the (p × √ 3)-Bi traces and the Ag film thickness, their energetic positions are always found at (23.70 ± 0.05) eV and (26.75 ± 0.05) eV, being consistent with the reported values for the well-defined BiAg 2 alloy on Ag(111) [21]. At 340 K, the intensity of BiAg 2 core levels decreases and a new spin-orbit split peak (blue) appears at ∼23.95 eV (Bi-5d 5/2 ), i.e., ∼210 meV shifted towards higher binding energy with respect to the energetic position obtained for the BiAg 2 alloy, being now consistent with the reported value for the elemental bismuth [22,23].…”
Section: Experimental Methodssupporting
confidence: 88%
“…For the as-deposited sample (300 K), we observed a single spin-orbit split peak (red) at binding energies of ∼23.74 eV (Bi-5d 5/2 ) and ∼26.79 eV (Bi-5d 3/2 ), i.e., the magnitude of the spin-orbit split amounts to ∼3.05 eV. Irrespective of the (p × √ 3)-Bi traces and the Ag film thickness, their energetic positions are always found at (23.70 ± 0.05) eV and (26.75 ± 0.05) eV, being consistent with the reported values for the well-defined BiAg 2 alloy on Ag(111) [21]. At 340 K, the intensity of BiAg 2 core levels decreases and a new spin-orbit split peak (blue) appears at ∼23.95 eV (Bi-5d 5/2 ), i.e., ∼210 meV shifted towards higher binding energy with respect to the energetic position obtained for the BiAg 2 alloy, being now consistent with the reported value for the elemental bismuth [22,23].…”
Section: Experimental Methodssupporting
confidence: 88%
“…Ritchie [5], Cherepkov [6], and Lee [7] generalized the phenomenon of dichroism to angular-resolved photoemission and termed it circular (or linear) dichroism in the angular distribution (CDAD or LDAD). At first, the studied objects were mostly oriented molecules and adsorbate systems [8], while later it was proven that photoemission from non-magnetic solids in fact also yields sizeable CDAD asymmetries in angular-resolved observation [9][10][11][12]. A necessary precondition is a definite handedness in the photoemission geometry [13].…”
Section: Introductionmentioning
confidence: 99%
“…Along either +k x or −k x , the state α shows complete intensity suppressions over several intervals of photon energy. Such a pronounced linear dichroism can be attributed to the sizable in-plane p x orbital component of α, 23,24 mainly coupling to the in-plane component E x of the light electric field. By contrast, E x is expected to couple less strongly to out-of-plane d z 2 and p z orbitals, as reflected by the weaker dichroism for γ.…”
mentioning
confidence: 99%