Electronic structure evolution at DBBA/Au(111) interface W/O Bismuth insertion layer
•Revealing the electronic structure evolution of self-assembled DBBA on Au(111) and Bi-3×3-Au(111).•Showing structural difference of DBBA on Au(111) and Bi-3×3-Au(111) at molecule level.•Explaining why 7-GNRs could not be formed on Bi-3×3-Au(111). Atomically precise graphene nanoribbons (GNRs) can b...
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Published in | Synthetic metals Vol. 251; pp. 24 - 29 |
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Main Authors | , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Lausanne
Elsevier B.V
01.05.2019
Elsevier BV |
Subjects | |
Online Access | Get full text |
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Summary: | •Revealing the electronic structure evolution of self-assembled DBBA on Au(111) and Bi-3×3-Au(111).•Showing structural difference of DBBA on Au(111) and Bi-3×3-Au(111) at molecule level.•Explaining why 7-GNRs could not be formed on Bi-3×3-Au(111).
Atomically precise graphene nanoribbons (GNRs) can be on-surface synthesized from halogen containing molecular precursors. Here, we investigated the electronic structure evolution of 10,10′-dibromo-9,9′-bianthracene (DBBA), a famous precursor to 7-AGNRs, on both Au(111) and Bi-3×3-Au(111) as a function of film thickness and post-annealing temperature using photoemission spectroscopy, low temperature scanning tunneling microscopy and density functional theories. No obvious changes in electronic structure of DBBA in three STM-observed configurations can be detected, indicating that nonplanar π -conjugated DBBA is physisorbed on both surfaces. The energy level alignments at the DBBA-substrate interfaces are demonstrated. Bismuth(Bi) insertion layer makes molecular−substrate interaction weaker, and makes the energy levels of DBBA thin film rigidly shift by ˜0.70 eV away from Fermi level, which enlarges the hole injection barrier and results in DBBA desorption at ˜470 K before dehalogenation occuring. The surface work function reduction can be explained by the push back effect and charge transfer induced interface dipole. Our findings explain why 7-GNRs could not be formed on Bi-3×3-Au(111). |
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ISSN: | 0379-6779 1879-3290 |
DOI: | 10.1016/j.synthmet.2019.03.016 |