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

\displaystyle \hat H = {\color{red}J} \left (\sum_p \vec{S}_p \cdot \vec{S}_{p+1} + {\color{red}\beta} (\vec{S}_p \cdot \vec{S}_{p+1})^2 \right )

BL-BQ model

\displaystyle \hat H = \sum_p \vec{S}_p \cdot \vec{S}_{p+1} + \frac{1}{3} (\vec{S}_p \cdot \vec{S}_{p+1})^2

Affleck, Kennedy, Lieb, Tasaki Phys. Rev. Lett. 59, 799 (1987)

\displaystyle H=\sum_p \vec{S}_p\cdot\vec{S}_{p+1}

\(S=\frac{1}{2}\rightarrow\) 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:

J=18 \mathrm{meV}\, ,\beta=0.09

Kicking a black box to learn about its contents

\displaystyle \mathcal{H}=-\frac{1}{2}\sum_{i\ne j}J_{ij}\,\vec{e}_{i}\vec{e}_{j}
J_{ij}=?
\delta E(\vec{e}_{i})=E(\vec{e}_{i})-E_{0}=\left(1-\vec{e}_{i}\vec{e}_{0}\right)\sum\limits _{k\left(\neq i\right)}J_{ik}
\delta E(\vec{e}_{i},\vec{e}_{j})=E(\vec{e}_{i},\vec{e}_{j})-E_{0}=\left(1-\vec{e}_{i}\vec{e}_{j}\right)J_{ij} +\left(1-\vec{e}_{i}\vec{e}_{0}\right)\sum\limits _{k\left(\neq i,j\right)}J_{ik}+\left(1-\vec{e}_{j}\vec{e}_{0}\right)\sum\limits _{k\left(\neq i,j\right)}J_{jk}\, \\ =\delta E(\vec{e}_{i})+\delta E(\vec{e}_{j})-\left(\vec{e}_{i}-\vec{e}_{0}\right)\left(\vec{e}_{j}-\vec{e}_{0}\right)J_{ij}\,.
\displaystyle E_{0}=-\frac{1}{2}\sum_{i\ne j}J_{ij}

Assume a ferromagnetic arrangement:

E_{ij}^{\mathrm{int}} =\delta E(\vec{e}_{i},\vec{e}_{j})-\delta E(\vec{e}_{i})-\delta E(\vec{e}_{j}) =-J_{ij}\,\delta\vec{e}_{i}\delta\vec{e}_{j}

Ab initio spin model parameters

\displaystyle \delta E^{int}_{nm} = -\frac{1}{\pi} \int \mathrm{Im} \mathrm{Tr} [G\delta V_n G \delta V_m] \mathrm{d}E \rightarrow \mathbb{E}_{nm}\, \delta\mathbf{S}_n\cdot\delta\mathbf{S}_m
\mathbb{E}_{nm}=J_{nm}\,\left(\,1+2\,\beta_{nm}\left(\mathbf{S}_n\cdot\mathbf{S}_m\right)\,\right)
J_{nm} = \left(\mathbb{E}_{nm}^{FM}+ \mathbb{E}_{nm}^{AFM}\right)/2\\\,\\ \beta_{nm} = \dfrac{1}{2}\,\dfrac{\mathbb{E}_{nm}^{FM}- \mathbb{E}_{nm}^{AFM}}{\mathbb{E}_{nm}^{FM}+\mathbb{E}_{nm}^{AFM}}
\displaystyle \hat H = \sum_{nm} {\color{red}J_{nm}} \left (\vec{S}_n \cdot \vec{S}_{m} + {\color{red}\beta_{nm}} (\vec{S}_n \cdot \vec{S}_{m})^2 \right )

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
H(\{\mathbf{S}_i\}) = \frac{1}{2} \sum_{i \neq j} \mathbf{S}_i \mathcal{J}_{ij} \mathbf{S}_j + \sum_i \mathbf{S}_i K_i \mathbf{S}_i

Number of orbitals: 8276

UNDER 1 Hour on 8 GPUs

pip install grogupy

Measurement 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

H=J\vec{S}_1\cdot\vec{S}_2+\beta\left ( \vec{S}_1\cdot\vec{S}_2 \right )^2
\sigma_2=\frac{|E_0-E_1|}{2t}

Effective model for spins from QDPT!

Day, et al. Phys. Codebases 50 (2025)

 pymablock.readthedocs.io

H_0 + p H_1 \Rightarrow \tilde{H}_0+\sum_n p^n \tilde{H}^{(n)}_1

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

\underbrace{H_0 + p H_1}_{c_{n\sigma}} \Rightarrow \underbrace{\tilde{H}_0+\sum_n p^n \tilde{H}^{(n)}_1}_{S_i}
\left(S_i S_j\right)^n=a_nI+b_n\left(S_i S_j\right)+c_n\left(S_i S_j\right)^2
\tilde{H}=A(t)I+f(t)\left(S_1 S_2\right)+g(t)\left(S_1 S_2\right)^2
f(t^*)=3g(t^*)

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