# Merits of using density matrices instead of wave functions in the   stationary Schr\"odinger equation for systems with symmetries

**Authors:** E. Shpagina, F. Uskov, N. Il'in, O. Lychkovskiy

arXiv: 1812.03056 · 2020-02-18

## TL;DR

This paper advocates using density matrices in the stationary Schrödinger equation for systems with symmetries, highlighting advantages in handling degeneracies and symmetry properties, with applications to spin systems.

## Contribution

It introduces the formulation of the stationary Schrödinger equation using density matrices, demonstrating benefits in symmetry considerations and degeneracy handling in many-body quantum systems.

## Key findings

- Density matrices can always be chosen to respect all Hamiltonian symmetries.
- The approach simplifies understanding of eigenstate structures.
- Analytical solutions for spin systems are provided.

## Abstract

The stationary Schr\"odinger equation can be cast in the form $H \rho = E \rho$, where $H$ is the system's Hamiltonian and $\rho$ is the system's density matrix. We explore the merits of this form of the stationary Schr\"odinger equation, which we refer to as~SSE$_\rho$, applied to many-body systems with symmetries. For a nondegenerate energy level, the solution $\rho$ of the SSE$_\rho$ is merely a projection on the corresponding eigenvector. However, in the case of degeneracy $\rho$ is non-unique and not necessarily pure. In fact, it can be an arbitrary mixture of the degenerate pure eigenstates. Importantly, $\rho$ can always be chosen to respect all symmetries of the Hamiltonian, even if each pure eigenstate in the corresponding degenerate multiplet spontaneously breaks the symmetries. This and other features of the solutions of the SSE$_\rho$ can prove helpful by easing the notations and providing an unobscured insight into the structure of the eigenstates. We work out the SSE$_\rho$ for a general system of spins $1/2$ with Heisenberg interactions, and address simple systems of spins $1$. Eigenvalue problem for quantum observables other than Hamiltonian can also be formulated in terms of density matrices. As an illustration, we provide an analytical solution to the eigenproblem ${\bf S}^2 \rho=S(S+1) \rho$, where $\bf S$ is the total spin of $N$ spins $1/2$, and $\rho$ is chosen to be invariant under permutations of spins. This way we find an explicit form of projections to the invariant subspaces of ${\bf S}^2$.

## Full text

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## Figures

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## References

21 references — full list in the complete paper: https://tomesphere.com/paper/1812.03056/full.md

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Source: https://tomesphere.com/paper/1812.03056