Draft:Orbital Rashba effect

• Comment: While this topic may be appropriate, this page currently appears to contain mainly citations to the editor's own work. That is not acceptable, a broad and general description is needed. Ldm1954 (talk) 07:01, 14 September 2025 (UTC)

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The orbital Rashba effect refers to the emergence of finite orbital angular momentum (OAM) Bloch states at solid surfaces, driven by the confining electric field that breaks inversion symmetry. The formation of chiral OAM states is the primary energy-lowering mechanism of Rashba states. In turn, chiral spin angular momentum (SAM) arises from these preexisting chiral OAM structures through spin–orbit coupling, linking the orientations of the two angular momenta. Thus, the OAM structure plays the central role in Rashba phenomena, while the spin texture appears as a concomitant effect. The orbital Rashba effect has been observed on the surfaces of a wide range of materials, including Au, Bi, Sb, Al, and the topological insulator Bi₂Se₃.^{[1][2][3][conflicted source?]}.

Theory

The formation of chiral OAM can be demonstrated with a tight-binding Hamiltonian of electrons with ${\displaystyle p_{x}}$, ${\displaystyle p_{y}}$, ${\displaystyle p_{z}}$ orbitals^[4]. In the presence of electric field perpendicular to the plane (assumed along the ${\displaystyle z}$-direction), hybridization between (${\displaystyle p_{x}}$, ${\displaystyle p_{y}}$) orbitals and ${\displaystyle p_{z}}$ orbital can take place and the Bloch states can be constructed accordingly. The Bloch state ${\displaystyle |{\bf {k}}\rangle }$ carries an internal angular orientation given by the average of the orbital angular momentum ${\displaystyle {\bf {L}}}$, ${\displaystyle {\bf {L}}_{\bf {k}}=\langle {\bf {k}}|{\bf {L}}|{\bf {k}}\rangle }$. The electrostatic energy gain for the Bloch state can be expressed as

${\displaystyle \Delta E_{\bf {k}}=\alpha _{\rm {OR}}{\hat {z}}\cdot ({\bf {k}}\times {\bf {L}}_{\bf {k}})}$

in the vicinity of the ${\displaystyle \Gamma }$ (${\displaystyle {\bf {k}}={\bf {0}}}$) point. It is analogous to the Rashba Hamiltonian for spins, with the SAM replaced by OAM. The coefficient ${\displaystyle \alpha _{\rm {OR}}}$ is proportional to the work function, reflecting the electrostatic confinement at the surface. To minimize Coulomb energy, the angular momentum (including both spin and orbital parts) must be perpendicular both to ${\displaystyle {\bf {k}}}$ and the surface normal:

${\displaystyle {\bf {L}}_{\bf {k}}\propto {\hat {z}}\times {\bf {k}}.}$

In contrast to the conventional Rashba state showing spin polarization

${\displaystyle {\bf {S}}_{\bf {k}}\propto {\hat {z}}\times {\bf {k}}~~({\bf {S}}_{\bf {k}}=\langle {\bf {k}}|{\bf {S}}|{\bf {k}}\rangle )}$

with spin operator ${\displaystyle {\bf {S}}}$, the orbital Rashba state develops chiral structure in momentum space for the orbital polarization.

The constant ${\displaystyle \alpha _{\rm {OR}}}$ is determined by the surface work function, independent of the atomic spin-orbit coupling. In the extreme case, even with no spin polarization, the energy can be lowered solely by orbital angular momentum. This means the orbital Rashba effect precedes the spin Rashba effect. The electric dipole moment of each Bloch state is proportional to ${\displaystyle {\bf {k}}\times {\bf {L}}_{\bf {k}}}$, which couples to the confining electric field at the surface. To lower the energy, the orientation of ${\displaystyle {\bf {L}}_{\bf {k}}}$ assumes the direction perpendicular to both the confining electric field ${\displaystyle {\hat {z}}}$ and the Bloch momentum ${\displaystyle {\bf {k}}}$, as confirmed in several tight-binding and first-principles calculations^[5][6].

Experimental confirmation of chiral OAM through circular dichroism

Experimental observation of chiral OAM in orbital Rashba states has been achieved using circular dichroism angle-resolved photoemission spectroscopy (CD-ARPES)^[1]. This technique measures the difference in photoemission intensities obtained with left- and right-circularly polarized light. The CD-ARPES intensity was shown to be proportional to the OAM, providing a direct probe of orbital textures^[1][6]

The surface states of Bi₂Se₃, a prototypical topological insulator, have also been identified as orbital Rashba states. CD-ARPES measurements on Bi₂Se₃ revealed dichroism patterns consistent with the expected chiral OAM structure^[1]. Similar experiments have been carried out on the Au(111) surface, the best-known example of Rashba states^[2][3]. The observed CD-ARPES patterns display the OAM texture predicted by the orbital Rashba effect, demonstrating that orbital angular momentum is an intrinsic and ubiquitous feature of Rashba states.

The surface states of Bi₂Se₃, a prototypical topological insulator, have also been identified as orbital Rashba states. CD-ARPES measurements on Bi₂Se₃ revealed dichroism patterns consistent with the expected chiral OAM structure^[1]. Similar experiments have been carried out on the surface states of Au(111), the best-known example of Rashba states^[2][3]. CD-ARPES experiments have also been performed in the bulk Rashba states of PtCoO₂ and BiTeI, both of which lack inversion symmetry in their crystal structures^[7][8]. These Rashba states can also be well explained within the framework of the orbital Rashba effect. The observed CD-ARPES patterns display the OAM texture predicted by the orbital Rashba effect, demonstrating that orbital angular momentum is an intrinsic and ubiquitous feature of Rashba states. Furthermore, ARPES measurements combined with first-principles calculations have confirmed the presence of the orbital Rashba state in the binary honeycomb monolayer AgTe^[9].

See also

• Rashba effect

References

1. Park, Seung Ryong; Han, Jinhee; Kim, Chul; Koh, Yoon Young; Kim, Changyoung; Lee, Hyungjun; Choi, Hyoung Joon; Han, Jung Hoon; Lee, Kyung Dong; Hur, Nam Jung; Arita, Masashi; Shimada, Kenya; Namatame, Hirofumi; Taniguchi, Masaki (2012-01-25). "Chiral Orbital-Angular Momentum in the Surface States of Bi 2 Se 3". Physical Review Letters. 108 (4) 046805. arXiv:1103.0805. doi:10.1103/PhysRevLett.108.046805. ISSN 0031-9007. PMID 22400876.
2. Kim, Beomyoung; Kim, Choong H.; Kim, Panjin; Jung, Wonsig; Kim, Yeongkwan; Koh, Yoonyoung; Arita, Masashi; Shimada, Kenya; Namatame, Hirofumi; Taniguchi, Masaki; Yu, Jaejun; Kim, Changyoung (2012-05-02). "Spin and orbital angular momentum structure of Cu(111) and Au(111) surface states". Physical Review B. 85 (19) 195402. arXiv:1112.2469. Bibcode:2012PhRvB..85s5402K. doi:10.1103/PhysRevB.85.195402. ISSN 1098-0121.
3. Ryu, Hanyoung; Song, Inkyung; Kim, Beomyoung; Cho, Soohyun; Soltani, Shoresh; Kim, Timur; Hoesch, Moritz; Kim, Choong H.; Kim, Changyoung (2017-03-24). "Photon energy dependent circular dichroism in angle-resolved photoemission from Au(111) surface states". Physical Review B. 95 (11) 115144. Bibcode:2017PhRvB..95k5144R. doi:10.1103/PhysRevB.95.115144. ISSN 2469-9950. Retrieved 2025-09-14.
4. Petersen, L.; Hedegård, P. (2000). "A simple tight-binding model of spin–orbit splitting of sp-derived surface states". Surface Science. 459 (1–2). Elsevier BV: 49–56. Bibcode:2000SurSc.459...49P. doi:10.1016/s0039-6028(00)00441-6. ISSN 0039-6028.
5. Park, Seung Ryong; Kim, Choong H.; Yu, Jaejun; Han, Jung Hoon; Kim, Changyoung (2011-10-06). "Orbital-Angular-Momentum Based Origin of Rashba-Type Surface Band Splitting". Physical Review Letters. 107 (15) 156803. arXiv:1107.1554. Bibcode:2011PhRvL.107o6803P. doi:10.1103/PhysRevLett.107.156803. ISSN 0031-9007. PMID 22107313.
6. Park, Jin-Hong; Kim, Choong H.; Rhim, Jun-Won; Han, Jung Hoon (2012-05-02). "Orbital Rashba effect and its detection by circular dichroism angle-resolved photoemission spectroscopy". Physical Review B. 85 (19) 195401. arXiv:1112.1821. Bibcode:2012PhRvB..85s5401P. doi:10.1103/PhysRevB.85.195401. ISSN 1098-0121.
7. Sunko, Veronika; Rosner, H.; Kushwaha, P.; Khim, S.; Mazzola, F.; Bawden, L.; Clark, O. J.; Riley, J. M.; Kasinathan, D.; Haverkort, M. W.; Kim, T. K.; Hoesch, M.; Fujii, J.; Vobornik, I.; Mackenzie, A. P.; King, P. D. C. (2017). "Maximal Rashba-like spin splitting via kinetic-energy-coupled inversion-symmetry breaking". Nature. 549 (7673). Springer Science and Business Media LLC: 492–496. arXiv:1708.03887. Bibcode:2017Natur.549..492S. doi:10.1038/nature23898. ISSN 0028-0836. PMID 28959958.
8. Bawden, Lewis; Riley, Jonathan M.; Kim, Choong H.; Sankar, Raman; Monkman, Eric J.; Shai, Daniel E.; Wei, Haofei I.; Lochocki, Edward B.; Wells, Justin W.; Meevasana, Worawat; Kim, Timur K.; Hoesch, Moritz; Ohtsubo, Yoshiyuki; Le Fèvre, Patrick; Fennie, Craig J.; Shen, Kyle M.; Chou, Fangcheng; King, Phil D. C. (2015-09-04). "Hierarchical spin-orbital polarization of a giant Rashba system" (PDF). Science Advances. 1 (8) e1500495. arXiv:1507.08588. Bibcode:2015SciA....1E0495B. doi:10.1126/sciadv.1500495. ISSN 2375-2548. PMC 4643772. PMID 26601268. Retrieved 2025-09-22.
9. Ünzelmann, Maximilian; Bentmann, Hendrik; Eck, Philipp; Kißlinger, Tilman; Geldiyev, Begmuhammet; Rieger, Janek; Moser, Simon; Vidal, Raphael C.; Kißner, Katharina; Hammer, Lutz; Schneider, M. Alexander; Fauster, Thomas; Sangiovanni, Giorgio; Di Sante, Domenico; Reinert, Friedrich (2020-04-29). "Orbital-Driven Rashba Effect in a Binary Honeycomb Monolayer AgTe". Physical Review Letters. 124 (17) 176401. arXiv:1912.05210. Bibcode:2020PhRvL.124q6401U. doi:10.1103/PhysRevLett.124.176401. ISSN 0031-9007. PMID 32412286.