Spin 1 physics in molecules and quantum dots
Department of Physics of Complex Systems
Eötvös Loránd University
László Oroszlány




Haldane's conjecture and the AKLT model
BL-BQ model

Affleck, Kennedy, Lieb, Tasaki Phys. Rev. Lett. 59, 799 (1987)
\(S=\frac{1}{2}\rightarrow\) gapless
\(S=1\rightarrow\) gapped
F. D. M. Haldane Phys. Rev. Lett. 50, 1153 (1983)
How to realize S=1 and the Haldane phase


Renard, Regnault, Verdaguer, in
Magnetism: Molecules to Materials I: Models and Experiments
- inelastic neutron-scattering experiments on bulk samples
- interchain interaction
- anisotropy
Can we realize with S=1 with carbon?



Su, Telychko, Song, Lu Angewandte Chemie 59 7658 (2020)
YES!
E. Lieb,
Phys. Rev. Lett. 62 1201 (1989)
Making a chain!

Mishra et al. Nature 598, 287 (2021).

fit to BL-BQ model:
Kicking a black box to learn about its contents
Assume a ferromagnetic arrangement:
Ab initio spin model parameters


DFT through
| Dimer | Infinite chain | Experiment | |
|---|---|---|---|
| 17.7 meV | 19.75 meV | 18 meV | |
| 0.03 | 0.05 | 0.09 |
The proof of the pudding
\( \beta \)
\( J \)
Singlet-Triplet transition in odd-length chains
Bridgeing with a sulfur atom \(\Rightarrow\)
there is a dipole!

Singlet-Triplet transition through electric field



Get Grogu(py)!
- Very early release !!
- https://github.com/danielpozsar/grogu
- post. proc. for single DFT calculation
- parallel BZ integral with MPI or CUDA
- Generalised Heisenberg model

Number of orbitals: 8276
UNDER 1 Hour on 8 GPUs

pip install grogupyMeasurement based quantum computing



Raussendorf, Briegel Phys. Rev. Lett. 86, 5188 (2001)
Raussendorf
Looking for resource states
Wei, Affleck, Raussendorf Phys. Rev. Lett. 106, 070501 (2011)

Tzu-Chieh Wei
Ian Affleck




Looking for higher spins




Lieb Phys. Rev. Lett. 62, 1927 (1989)
Elliott Lieb
Stars are quite resilient!

S=1 AKLT: How to couple two stars?

AFM
AFM
FM



Effective model for spins from QDPT!
Day, et al. Phys. Codebases 50 (2025)
pymablock.readthedocs.io


S=1 AKLT: How to couple two stars, PT


S=1 AKLT: How to couple many stars?
This is
promising!





We do not want:
\( \vec{S}_1\cdot\vec{S}_3 \Rightarrow \) long range
\( (\vec{S}_1\cdot\vec{S}_2) (\vec{S}_2\cdot\vec{S}_3) \) \(\Rightarrow\) multi spin
Experimental realization

V. John et al. Nat. Commun. 16, 10560 (2025)
Thanks!
C. Benjamin, D. Varjas, G. Széchenyi, J. Romhányi, LO
https://arxiv.org/abs/2603.06455





G. Martínez-Carracedo, LO, A. García-Fuente, L. Szunyogh, J. Ferrer
Phys. Rev. B 107, 035432 (2023)




S=1
By László Oroszlány
S=1
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