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Quantum phase transitions in random spin systems

T. Senthil

Published Jan 1, 1997• 0 citations
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After reviewing the basics of the cavity method in classical systems, we show how its quantum version, with some appropriate approximation scheme, can be used to study a system of spins with random ferromagnetic interactions and a random transverse field. The quantum cavity equations describing the ferromagnetic-paramagnetic phase transition can be transformed into the well-known problem of a classical directed polymer in a random medium. The glass transition of this polymer problem translates into the existence of a 'Griffiths phase' close to the quantum phase transition of the quantum spin problem, where the physics is dominated by rare events. The physical behaviour of random transverse-field ferromagnets on the Bethe lattice is found to be very similar to that found in finite-dimensional systems, and the quantum cavity method gets back the known exact results of the one-dimensional problem.
We study the effects of random fluctuations on quantum phase transitions by the energy gap analysis. For the infinite-ranged spin-glass models with a transverse field, we find that a strong sample-to-sample fluctuation effect leads to broad distributions of the energy gap. As a result, the linear, spin-glass, and nonlinear susceptibilities behave differently from each other. The power-law tail of the distribution implies a quantum Griffiths-like effect that could be observed in various random quantum systems. We also discuss the mechanisms of the phase transition in terms of the energy gap by comparing the Sherrington-Kirkpatrick model and random energy model, which demonstrate the difference between the continuous and discontinuous phase transitions.
Random spin-32\frac{3}{2}23​ antiferromagnetic Heisenberg chains are investigated using an asymptotically exact renormalization group. Randomness is found to induce a quantum phase transition between two random-singlet phases. In the strong randomness phase the effective spins at low energies are Seff=32,{S}_{\mathrm{eff}}=\frac{3}{2},Seff​=23​, while in the weak randomness phase the effective spins are Seff=12.{S}_{\mathrm{eff}}=\frac{1}{2}.Seff​=21​. Separating them is a quantum critical point near which there is a nontrivial mixture of spin-12,\frac{1}{2},21​, spin-1,1,1, and spin-32\frac{3}{2}23​ effective spins at low temperatures.