1 Introduction

We consider weakly interacting quantum spin systems on finite subsets \(\varLambda \) of the lattice \({\mathbb {Z}} ^\nu \), \(\nu \in {\mathbb {N}} \), described by a self-adjoint Hamiltonian

$$\begin{aligned} H= H_0 + H_{\mathrm{int}} \,, \end{aligned}$$
(1)

which is composed of a non-interacting part \(H_0\) and an interacting part \(H_{\mathrm{int}}\). The non-interacting Hamiltonian \(H_0\) is a sum of non-negative on-site Hamiltonians \(h_x\), \(x\in \varLambda \). Each \(h_x\) is assumed to have a non-degenerate ground state with ground state energy \(0\) and spectral gap of size at least \(g\) above the ground state. The interaction Hamiltonian \(H_{\mathrm{int}}\) is a sum of interaction terms \(\varPhi _x\) of finite range \(R\) and of small uniformly bounded norm \(\left\Vert {\varPhi _x} \right\Vert \). We show that for such Hamiltonians a strong version of the local perturbations perturb locally (LPPL) principle holds: For any self-adjoint perturbation \(P\)  supported in a region \(X \subset \varLambda \), any ground state \(\rho _P\) of the perturbed Hamiltonian \(H + P\) agrees with the ground state \(\rho \) of the unperturbed Hamiltonian \(H\) when tested against observables \(A\) supported in a region \(Y\subset \varLambda \) up to an error that is exponentially small in the distance \({{\,\mathrm{dist}\,}}(Y,X)\). More precisely, Theorem 3 states that there are positive constants \(c, c_1, c_2>0 \) depending only on \(R\) and \(g\), but not on \(\varLambda \), \(A\), \(H\) or \(P\), such that whenever \(\left\Vert {\varPhi _x} \right\Vert \le c\) for all \(x\in \varLambda \), it holds that

$$\begin{aligned} \left|{{\mathrm{tr}}\big (( \rho _P - \rho )A\big )} \right| \, \le \, {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2 {{\,\mathrm{dist}\,}}(Y,X) } \,. \end{aligned}$$
(2)

Note that the uniformity of the error estimate with respect to the system size \(\left|{\varLambda } \right|\) is one key aspect which makes this estimate non-trivial. Note also, that the bound on \(\left\Vert {\varPhi _x} \right\Vert \) implies that \(H\) has a gap above its unique ground state \(\rho \) as we discuss below. However, for our result we neither require nor actually have any uniform lower bound on the gap above the possibly non-unique ground state \(\rho _P\) of the perturbed Hamiltonian \(H + P\).

As a corollary of our main theorem, we show that a bound of the form (2) also holds for systems that have the appropriate structure of gapped on-site terms and weak interactions only locally in some region of space. In particular, this shows that the notion of a locally gapped ground state, which is completely insensitive to the form of the Hamiltonian elsewhere, is perfectly valid in this setup.

The LPPL-principle was coined by Bachmann, Michalakis, Nachtergaele, and Sims in [1], where a similar estimate with subexponential decay was proven. While their result covers much more general interacting quantum spin systems, it requires the gap above the ground state to remain open also for the perturbed Hamiltonian \(H + P\). More precisely, it relies on connecting \(H(0) := H\) with \(H(1) := H + P\) by a continuous path \([0,1] \ni t \mapsto H (t)\) in the space of Hamiltonians, such that the gap above the ground state of \(H (t)\) remains open uniformly along the whole path. Then the locality of the quasi-adiabatic evolution introduced by Hastings and Wen in [11] can be used to prove the result. Their subexponential bound was improved to exponential precision for finite-range interactions by De Roeck and Schütz in [8]. See also [14, 15] for recent developments.

While we prove the strong version of the LPPL-principle only for weakly interacting spin systems, we expect it to hold somewhat more generally. For example, we expect it to hold for fermions on the lattice with weak finite range interactions, a physical setup where the strong LPPL-principle would have important consequences. It would imply that a gapped ground state for such a system with periodic boundary conditions remains unchanged in the bulk when introducing open boundary conditions that may close the global gap due to the emergence of edge states. And as a consequence, it would also explain why the adiabatic response to external fields in the bulk of such systems is not affected by edge states that close the gap, see [2, 12, 13, 18, 20] for related results. However, it is known that the strong LPPL-principle cannot hold in general, but requires further conditions on the unperturbed ground state sector such as local topological quantum order (LTQO) [16, 17].

Shortly before resubmitting the final version of this article, Bachmann et al. published a preprint containing a closely related result. In [3] they prove an LPPL-bound as in (2), but with subexponential decay, assuming LTQO for a unique frustration-free gapped ground state of the unperturbed Hamiltonian which has no long-range entanglement.

Our result is a corollary of a result by Yarotsky [22] (see Theorem 7 below), which provides a bound on the difference of so-called finite volume ground states in quantum spin systems described by Hamiltonians of the form (1). His aim and main result in that work was to show the uniqueness of the ground state of such systems in the thermodynamic limit. In a different work Yarotsky [21] has shown that Hamiltonians of the form (1) with \(\left\Vert {\varPhi } \right\Vert <c\) indeed have a unique ground state separated by a gap \({\tilde{g}} > 0\) from the rest of the spectrum, with \({\tilde{g}}\) independent of \(\varLambda \) (see [7, 9, 10] for similar results). Closely related to the stability of the gap is the stability of phase diagrams at low temperatures, see [4,5,6].

2 Main results

Consider the lattice \({\mathbb {Z}}^\nu \) for fixed \(\nu \in {\mathbb {N}}\) equipped with the \(\ell ^1\)-metric \(d \, \mathpunct {:} {\mathbb {Z}} ^\nu \times {\mathbb {Z}} ^\nu \rightarrow {\mathbb {N}}_0\) and define \({\mathcal {P}}_0({\mathbb {Z}} ^\nu ) \mathrel = \{\varLambda \,{\subset }\, {\mathbb {Z}} ^\nu : \left|{\varLambda } \right| \,{<}\, \infty \)}, where \(\left|{\varLambda } \right|\) denotes the cardinality of \(\varLambda \). With each site \(x \in {\mathbb {Z}} ^\nu \) one associates a (possibly infinite dimensional) Hilbert space \({\mathcal {H}}_x\). For \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) set \({\mathcal {H}}_{\varLambda }=\bigotimes _{x \in \varLambda } {\mathcal {H}}_x\) and denote the algebra of bounded linear operators on \({\mathcal {H}}_{\varLambda }\) by \({\mathcal {A}}_{\varLambda }={\mathcal {B}}({\mathcal {H}}_{\varLambda })\). Due to the tensor product structure, we have \({\mathcal {A}}_{\varLambda }=\bigotimes _{x \in \varLambda } {\mathcal {B}}({\mathcal {H}}_x)\). Hence, for \(\varLambda '\subset \varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\), any \(A \in {\mathcal {A}}_{\varLambda '}\) can be viewed as an element of \({\mathcal {A}}_{\varLambda }\) by identifying \(A\) with \(A\otimes {\mathbf {1}}_{\varLambda \setminus \varLambda '} \in {\mathcal {A}}_{\varLambda }\), where \({\mathbf {1}}_{\varLambda \setminus \varLambda '}\) denotes the identity in \({\mathcal {A}}_{\varLambda \setminus \varLambda '}\). Note that

$$\begin{aligned}{}[{A,B}] = 0 \quad \text {for all} \quad A \in {\mathcal {A}}_\varLambda \,, \ B \in {\mathcal {A}}_{\varLambda '} \quad \text {with} \quad \varLambda \cap \varLambda ' = \emptyset \,. \end{aligned}$$

Similarly, we will also denote by \(K\) the closure of \({\mathbf {1}}_{\varLambda \setminus \varLambda '} \otimes K\) on \({\mathcal {H}}_{\varLambda \setminus \varLambda '} \otimes D(K)\) for any self-adjoint operator \(K\) on \({\mathcal {H}}_{\varLambda '}\). Here and in the following, \(D(K)\) denotes the domain of the operator \(K\).

Our main result will be formulated for a Hamiltonian

$$\begin{aligned} H = H_0 + H_{\mathrm{int}} \in {\mathcal {A}}_{\varLambda } \end{aligned}$$

that is composed of a non-interacting part \(H_0\) and an interacting part \(H_{\mathrm{int}}\). The non-interacting part \(H_0\) is assumed to be of the form

$$\begin{aligned} H_0 = \sum _{x \in \varLambda } h_x\,, \end{aligned}$$

where each \(h_x\) is a non-negative self-adjoint (possibly unbounded) operator on \({\mathcal {H}}_x\) with a unique gapped ground state \(\psi _x \in D(h_x)\) satisfying

$$\begin{aligned} h_x \psi _x = 0 \quad \text {and} \quad h_x\big \vert _{D(h_x) \ominus \psi _x} \ge g\,, \end{aligned}$$
(3)

for some fixed \(g>0\). The latter means that \(\langle {\varphi _x,(h_x-g{\mathbf {1}}_x)\varphi _x}\rangle \ge 0\) for all \(\varphi _x \in D(h_x)\) with \(\langle {\psi _x,\varphi _x}\rangle =0\). In other words, all Hamiltonians \(h_x\) have a spectral gap of size at least \(g\) above the bottom of their spectrum. The interacting part is of the form

$$\begin{aligned} H_{\mathrm{int}} = \sum _{x \in \varLambda } \varPhi _x\,, \end{aligned}$$

with \(\varPhi _x\in {\mathcal {A}}_{b_x(R)}\) self-adjoint for each \(x \in \varLambda \) and some fixed \(R\in {\mathbb {N}} \). Here \(b_x(R) \,{:=}\, \{{y \in \varLambda : d(x,y) \le R}\}\) denotes the \(\ell ^1\)-ball with radius \(R\) centered at \(x \in \varLambda \). We set

$$\begin{aligned} \left\Vert {\varPhi } \right\Vert \,{:=}\, \sup _{x \in \varLambda } \, \left\Vert {\varPhi _x} \right\Vert \,. \end{aligned}$$

Definition 1

Weakly interacting spin system

For any \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu ) \) we call a Hamiltonian \(H = H_0 + H_{\mathrm{int}}\) on \({\mathcal {H}}_\varLambda \) with \(H_0\) and \(H_{\mathrm{int}}\) satisfying the above conditions a weakly interacting spin system on \(\varLambda \) with on-site gap \(g\), interaction range \(R\) and interaction strength \(\left\Vert {\varPhi } \right\Vert \).

We use the following definition for ground states and briefly explain how it is connected to the standard definition in the Appendix.

Definition 2

Let \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) and \(K\) be a self-adjoint and bounded below operator on \({\mathcal {H}}_\varLambda \). We say that \([{K,A}]\) is a bounded operator \(B\in {\mathcal {A}}_\varLambda \), whenever \(A\) leaves \(D(K)\) invariant and \([{K,A}]=B\) on \(D(K)\).

A state \(\rho \in {\mathcal {A}}_{\varLambda }\), i.e. a positive semi-definite bounded operator with trace equal to one, is called a ground state of \(K\), if

$$\begin{aligned}{\mathrm{tr}}\big ( A^* [{K,A}] \,\rho \big ) \,\ge \, 0 \quad \text {for all } A \in {\mathcal {A}}_{\varLambda } \text { such that } [{K,A}] \text { is bounded} . \end{aligned}$$

Our first main result is the following.

Theorem 3

The strong LPPL-principle

Let \(R\in {\mathbb {N}} \) and \(g>0\). There exist constants \(c, c_1, c_2>0\), such that for any \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) and any weakly interacting spin system \(H = H_0 + H_{\mathrm{int}}\) on \(\varLambda \) with on-site gap at least \(g\), interaction range \(R\), and interaction strength \(\left\Vert {\varPhi } \right\Vert \le c\) the following holds:

Let \(X\subset \varLambda \) be non-empty and \(P\) be a symmetric operator on \({\mathcal {H}}_X\) such that \(P\) is relatively bounded with respect to \(H\) with \(H\)-bound less than one. Set \(H_P = H + P\). Then for any ground state \(\rho \) of \(H\), any ground state \(\rho _P\) of \(H_P\), and all \(A \in {\mathcal {A}}_Y\) with \(Y \subset \varLambda \) it holds that

$$\begin{aligned} \left|{{\mathrm{tr}} \big ( \left( \rho _P -\rho \right) A\big )} \right| \,\le \, {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2 {{\,\mathrm{dist}\,}}(Y,X)} \,. \end{aligned}$$
(4)

Under the assumptions of the theorem, Yarotsky has proven in [21] that \(H\) has a unique ground state \(\rho \), whenever \(c>0\) is small enough.Footnote 1 In the following we will assume that this is the case.

For \(X\) at the edge of \(\varLambda \), the perturbation \(P\) can be employed to realize all kinds of boundary conditions, e.g. if \(\varLambda = \{ -M,\dotsc ,M \}^\nu \) is a box, periodic boundary conditions can be modeled by some \(P\) connecting opposite sites in \(\varLambda \). Therefore, if \(X\) is at the edge, one can take the thermodynamic limit \({\varLambda \nearrow {\mathbb {Z}} ^\nu }\) in (4) and conclude that there exists a unique ground state \(\rho \), i.e. a normalized positive functional, on the \(C^*\)-algebra of quasi-local observables \({\mathcal {A}} = {\overline{{{\mathcal {A}}_{\mathrm{loc}}}}}^{\Vert {\cdot }\Vert }\), independent of the imposed boundary conditions for the finite systems. This uniqueness of ground states for the infinite system was the main result of [22] and has been shown by Yarotsky based on Theorem 7, which we quote below.

As mentioned in the introduction, we expect a similar strong LPPL-principle to hold also for fermionic lattice systems with weak finite range interactions. As discussed in [12, 13], this would have important consequences for linear response and adiabatic theorems for systems with a gap only in the bulk.

Our second main result is a local version of Theorem 3, where we assume the on-site gap and the weak interaction only locally.

Definition 4

Locally weakly interacting spin system

For any \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) and \(\varLambda '\subset \varLambda \) we say that a self-adjoint operator \(H\) on \({\mathcal {H}}_\varLambda \) is weakly interacting in the region \(\varLambda '\) with on-site gap \(g\), range \(R\) and strength \(s\), if and only if there exists a weakly interacting spin system \({\tilde{H}} = {\tilde{H}}_0 + {\tilde{H}}_{\mathrm{int}}\) on \(\varLambda \) with on-site gap \(g\), range \(R\) and strength \(\left\Vert {\varPhi } \right\Vert =s\) such that \( H - {\tilde{H}} = {\mathbf {1}}_{{\mathcal {H}}_{\varLambda '}} \otimes \, Q\) with \(Q\) a possibly unbounded symmetric operator on \({\mathcal {H}}_{\varLambda \setminus \varLambda '}\) such that \(Q\) is infinitesimally \({\tilde{H}}\)-bounded.

Corollary 5

The strong LPPL-principle for local gaps

Let \(R \in {\mathbb {N}} \), \(g>0\), and \(c, c_1, c_2>0\) be the constants from Theorem 3. Then for any \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\), \(\varLambda '\subset \varLambda \), and any self-adjoint operator \(H\) on \({\mathcal {H}}_\varLambda \) which is weakly interacting in the region \(\varLambda '\) with on-site gap at least \(g\), range \(R\) and strength \(s \le c\) the following holds:

Let \(X\subset \varLambda \) be non-empty and \(P\) be a symmetric operator on \({\mathcal {H}}_X\) such that \(P\) is relatively bounded with respect to \(H\) with \(H\)-bound less than one. Set \(H_P = H + P\) (see Fig. 1). Then for any ground state \(\rho \) of \(H \), any ground state \(\rho _{P}\) of \(H_{P}\), and all \(A \in {\mathcal {A}}_Y\) with \(Y \subset \varLambda '\) it holds that

$$\begin{aligned} \left|{{\mathrm{tr}}\big (({\rho _{P} -\rho }) A\big )} \right| \,\le \, 2 \, {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2 \min \{ {{\,\mathrm{dist}\,}}(Y,X), {{\,\mathrm{dist}\,}}(Y,\varLambda \setminus \varLambda ')\}} \,. \end{aligned}$$
Fig. 1
figure 1

Depicted is the setting from Corollary 5. The system \(H\) defined on \(\varLambda \) is assumed to be weakly interacting and to have an on-site gap in \(\varLambda '\subset \varLambda \). For any perturbation \(P\) acting on \(X\subset \varLambda \), ground states of \(H\) and \(H+P\) agree in regions \(Y\) away from \(X\) and \(\varLambda \setminus \varLambda '\)

Proof

Let \(\tilde{H}\) and \(Q\) be as in Definition 4. Then \({\tilde{H}}\), \({\tilde{H}} + Q\) and \({\tilde{H}} + Q + P\) are self-adjoint. For the latter this follows, because also \(Q+P\) is relatively bounded with respect to \({\tilde{H}}\) with \({\tilde{H}}\)-bound less than one. This is not obvious, but the proof is a straightforward calculation that we skip.

Let \({\tilde{\rho }}\) be a ground state of \(\tilde{H}\), see the comment after Theorem 3 for existence. Then the triangle inequality and two applications of Theorem 3 yield

$$\begin{aligned} \left|{{\mathrm{tr}}\big (({\rho _{P} -\rho }) A\big )} \right| \,&\le \, \left|{{\mathrm{tr}}\big (({\rho _{P} -\tilde{\rho })} A\big )} \right| + \left|{{\mathrm{tr}}\big (({\rho -\tilde{\rho }}) A\big )} \right|\\&\le \, {\mathrm {e}}^{ c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, \big ({ {\mathrm {e}}^{-c_{2}{{\,\mathrm{dist}\,}}(Y,X \cup (\varLambda \setminus \varLambda ')) } + {\mathrm {e}}^{-c_{2}{{\,\mathrm{dist}\,}}(Y,\varLambda \setminus \varLambda ') }}\big ). \end{aligned}$$

\(\square \)

3 Proof

The proof of Theorem 3 is essentially a reinterpretation of a result by Yarotsky [22]. Since we only deal with finite volumes, we modify Yarotsky’s notion of finite volume ground states to ground states in the bulk. To make the arguments as transparent as possible, we will add superscripts to Hamiltonians and states indicating on which subset of \({\mathbb {Z}} ^\nu \) they are defined. These superscripts are also used to distinguish different operators and states. From now on let

$$\begin{aligned} {\mathcal {D}}_\varLambda := \{\,A\in {\mathcal {A}}_\varLambda : [{H_0^\varLambda ,A}] \text { is bounded}\,\} \end{aligned}$$

and note, that also \(\{\,A\in {\mathcal {A}}_\varLambda : [{H_0^\varLambda +K,A}] \text { is bounded}\,\} = {\mathcal {D}}_\varLambda \) for all bounded operators \(K\in {\mathcal {A}}_\varLambda \).

Definition 6

Ground states in the bulk

Let \(R \in {\mathbb {N}}\), \(\varLambda _* \subset \varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) and \(H^{\varLambda _*} = H_0^{\varLambda _*} + H_{\mathrm{int}}^{\varLambda _*} \in {\mathcal {A}}_{\varLambda _*}\) be a weakly interacting spin system on \(\varLambda _*\) with range \(R\). Then we call

$$\begin{aligned} \varLambda _*^\circ \mathrel := \,\{x \in \varLambda _* : {{\,\mathrm{dist}\,}}(x,{\mathbb {Z}} ^\nu \setminus \varLambda _*) > 2R\} \end{aligned}$$

the bulk of the Hamiltonian \(H^{\varLambda _*}\) and any state \(\rho ^\varLambda \in {\mathcal {A}}_{\varLambda }\) satisfying

$$\begin{aligned} {\mathrm{tr}}\left( {\rho ^\varLambda \, A^* \big [{H^{\varLambda _*},A}\big ]}\right) \ge 0 \quad \text {for all} \quad A \in {\mathcal {D}}_{\varLambda _*^\circ } \end{aligned}$$

a ground state in the bulk of \(H^{\varLambda _*}\).

Our proof is based on the following theorem due to Yarotsky [22].

Theorem 7

([22, Theorem 2]) Let \(R\in {\mathbb {N}} \) and \(g>0\). There exist constants \(c, c_1, c_2>0\) such that for any \(\varLambda _* \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\), and any weakly interacting spin system \(H^{\varLambda _*} = H_0^{\varLambda _*} + H_{\mathrm{int}}^{\varLambda _*}\) on \(\varLambda _*\) with on-site gap at least \(g\), range \(R\) and interaction strength \(\left\Vert {\varPhi } \right\Vert \le c\) the following holds:

Let \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) be such that \(\varLambda _* \subset \varLambda \). Then for any two ground states \(\rho ^\varLambda _1\) and \(\rho ^\varLambda _2 \in {\mathcal {A}}_\varLambda \) in the bulk of \(H^{\varLambda _*}\) in the sense of Definition 6, \(Y \subset \varLambda _*\), and \(A \in {\mathcal {A}}_Y\) it holds that

$$\begin{aligned} \left|{ {\mathrm{tr}}\big (({ \rho ^\varLambda _1 - \rho ^\varLambda _2 ) A}\big )} \right| \, \le \, {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2\, {{\,\mathrm{dist}\,}}(Y, {\mathbb {Z}} ^\nu \setminus \varLambda _*^\circ )} \,. \end{aligned}$$

Note that the set denoted by \(\varLambda \) in [22, Theorem 2] corresponds to our set \(\varLambda _*\). Note, moreover, that any ground state \(\rho ^\varLambda \) in the bulk of \(H^{\varLambda _*}\) trivially defines a finite-volume ground state \(A \mapsto {\mathrm{tr}}{\rho ^\varLambda \, (A\otimes {\mathbf {1}}_{\varLambda \setminus \varLambda _*})}\) of \(H^{\varLambda _*}\) in the sense of [22, Definition 2]. Allowing an arbitrary on-site gap \(g>0\) instead of \(g=1\), as in [22], is achieved by simple scaling.

Lemma 8

Let \(R \in {\mathbb {N}}\), \(\varLambda _*\subset \varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) and \(H^{\varLambda } = H_0^{\varLambda } + H_{\mathrm{int}}^{\varLambda } \in {\mathcal {A}}_{\varLambda }\) be a weakly interacting spin system. Then the canonical restriction of \(H^\varLambda \) to \(\varLambda _*\) defined by

$$\begin{aligned} H^{\varLambda }|_{\varLambda _*} = H_0^{\varLambda }|_{\varLambda _*} + H_{\mathrm{int}}^{\varLambda }|_{\varLambda _*} {:=} \sum _{x \in \varLambda _*} h_x + \sum _{\begin{array}{c} x \in \varLambda _*:\\ {{\,\mathrm{dist}\,}}(x,\varLambda \setminus \varLambda _*)>R \end{array}}\varPhi _x \end{aligned}$$

is a weakly interacting spin system on \(\varLambda _*\) with the same on-site gap, range and strength and has the following property: For any symmetric operator \(Q\) on \({\mathcal {H}}_{\varLambda \setminus \varLambda ^\circ _*}\) such that \(Q\) is relatively bounded with respect to \(H^\varLambda \) with \(H^\varLambda \)-bound less than one, any ground state of \(H^\varLambda + Q\) is also a ground state in the bulk of \(H^{\varLambda }|_{\varLambda _*}\).

Proof

It is clear that \(H^{\varLambda }|_{\varLambda _*}\) is a weakly interacting spin system on \(\varLambda _*\). A simple calculation shows, that \(Q\) is also relatively bounded with respect to \(H_0^{\varLambda \setminus \varLambda ^\circ _*}=\sum _{x \in \varLambda \setminus \varLambda ^\circ _*} h_x\) with \(H_0^{\varLambda \setminus \varLambda ^\circ _*}\)-bound less than one. Hence, \(K\,{:=}\, (H^\varLambda - H^{\varLambda }|_{\varLambda _*} + Q)\) is a self-adjoint operator on \({\mathcal {H}}_{\varLambda \setminus \varLambda ^\circ _*}\). Moreover, any \(A\in {\mathcal {A}}_{\varLambda _*^\circ }\) leaves invariant the domain of \({\mathbf {1}}_{\varLambda _*^\circ } \otimes K\) and satisfies

$$\begin{aligned} \left[ { {\mathbf {1}}_{\varLambda _*^\circ } \otimes K, A \otimes {\mathbf {1}}_{\varLambda \setminus \varLambda _*^\circ }}\right] = 0. \end{aligned}$$

Similarly, for all \(A\in {\mathcal {D}}_{\varLambda _*^\circ }\), \([{H^\varLambda + Q, A}]\) is bounded and satisfies

$$\begin{aligned}{}[{H^\varLambda + Q, A}] = [{H^{\varLambda }|_{\varLambda _*}, A}]. \end{aligned}$$

Therefore, any ground state of \(H^\varLambda +Q\) is also a ground state in the bulk of \(H^{\varLambda }|_{\varLambda _*}\). \(\square \)

Fig. 2
figure 2

Depicted is the setting from the proof of Proposition 9. The subset \(X\subset \varLambda \) is the region where the perturbation \(P\) acts, and we choose \({\varLambda _*=\varLambda \setminus X}\). The shaded region \(\varLambda _*^\circ \) is the bulk of \(H^{\varLambda _*}\). \({Y\subset \varLambda _*^\circ }\) is the support of the observable \(A\). This indicates why (5) holds

Before we prove Theorem 3, let us give an intermediate result, which follows rather directly from Theorem 7 and Lemma 8.

Proposition 9

Let \(R\in {\mathbb {N}} \) and \(g>0\). There exist constants \(c, c_1, c_2>0\) such that for any \(\varLambda \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) and any weakly interacting spin system \(H^\varLambda = H^\varLambda _0 + H^\varLambda _{\mathrm{int}}\) on \(\varLambda \) with on-site gap at least \(g\), interaction range \(R\), and interaction strength \(\left\Vert {\varPhi } \right\Vert \le c\) the following holds:

Let \(X\subset \varLambda \) be non-empty and \(P\) be a symmetric operator on \({\mathcal {H}}_X\) such that \(P\) is relatively bounded with respect to \(H^\varLambda \) with \(H^\varLambda \)-bound less than one. Set \(H^\varLambda _P = H^\varLambda + P\). Then for any ground state \(\rho ^\varLambda \) of \(H^\varLambda \), any ground state \(\rho ^\varLambda _P\) of \(H^\varLambda _P\), and all \(A \in {\mathcal {A}}_Y\) with \(Y \subset \varLambda \) it holds that

$$\begin{aligned} \left|{{\mathrm{tr}}\left( { ({\rho ^\varLambda _P - \rho ^\varLambda }) A}\right) } \right| \, \le \, {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2 \min \{ {{\,\mathrm{dist}\,}}(Y, {\mathbb {Z}} ^\nu \setminus \varLambda ^\circ ), \, {{\,\mathrm{dist}\,}}(Y,X) - 2R\}} \,. \end{aligned}$$

Proof

Assume w.l.o.g. that \(Y \subset \varLambda ^\circ \). Otherwise, the statement in Proposition 9 is trivially satisfied after a possible adjustment of \(c_1\).

Let \(\varLambda _* = \varLambda \setminus X\), and let \(H^{\varLambda }|_{\varLambda _*} \) be the canonical restriction of \(H^\varLambda \) to \(\varLambda _*\) as defined in Lemma 8. Then \(\varLambda _*^\circ \cap X = \emptyset \). We can assume w.l.o.g. that \({{\,\mathrm{dist}\,}}(X,Y) > 2R\) since otherwise the statement in Proposition 9 is trivially satisfied after a possible adjustment of \(c_1\). Then also \(Y \subset \varLambda _*^\circ \) (compare Fig. 2). By application of Lemma 8 with \(Q = P\) and \(Q = 0\) we find that both, \(\rho _P^\varLambda \) and \(\rho ^\varLambda \), are ground states in the bulk of \(H^{\varLambda }|_{\varLambda _*}\). Hence, Theorem 7 implies that

$$\begin{aligned} \left|{ {\mathrm{tr}}\big (({\rho ^\varLambda _P - \rho ^\varLambda }) A\big )} \right| \, \le \, {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2 {{\,\mathrm{dist}\,}}(Y, {\mathbb {Z}} ^\nu \setminus \varLambda _*^\circ )} \,. \end{aligned}$$

From

$$\begin{aligned} {\mathbb {Z}} ^\nu \setminus \varLambda _*^\circ = ({\mathbb {Z}} ^\nu \setminus \varLambda ^\circ ) \cup \{\, x \in {\mathbb {Z}} ^\nu : {{\,\mathrm{dist}\,}}(x,X) \le 2R \,\} \end{aligned}$$

we immediately conclude that

$$\begin{aligned} {{\,\mathrm{dist}\,}}(Y, {\mathbb {Z}} ^\nu \setminus \varLambda _*^\circ ) = \min \{ {{\,\mathrm{dist}\,}}(Y, {\mathbb {Z}} ^\nu \setminus \varLambda ^\circ ), \, {{\,\mathrm{dist}\,}}(Y, X) - 2R \}\,, \end{aligned}$$
(5)

which yields the claim. \(\square \)

We now extend this result to obtain Theorem 3.

Proof of Theorem 3

In the following, we add superscripts \(\varLambda \) to the Hamiltonians and states from the statement of Theorem 3.

Let \(\varOmega \in {\mathcal {P}}_0({\mathbb {Z}} ^\nu )\) be such that \(\varLambda \subset \varOmega \). For each \(x \in \varOmega \setminus \varLambda \) let \(h_x \in {\mathcal {A}}_{\{x\}}\) be a self-adjoint operator with gap at least \(g\) and non-degenerate ground state \(\psi _x\) satisfying (3). Then \(\rho ^{\varOmega \setminus \varLambda } = \bigotimes _{x\in \varOmega \setminus \varLambda } |{\psi _x}\rangle \langle {\psi _x}|\) is the ground state of

$$\begin{aligned} H_0^{\varOmega \setminus \varLambda } {:=} \sum _{\begin{array}{c} x\in \varOmega \setminus \varLambda \end{array}} h_x\,. \end{aligned}$$

Moreover, \(\rho ^{\varOmega }\,{:=}\,\rho ^{\varLambda } \otimes \rho ^{\varOmega \setminus \varLambda }\) is a ground state of \(H^\varOmega \,{:=}\, H^\varLambda + H_0^{\varOmega \setminus \varLambda }\) which is a weakly interacting spin system on \(\varOmega \) with on-site gap at least \(g\), range \(R\), and interaction strength \(\left\Vert {\varPhi } \right\Vert \). And also \(\rho _P^{\varOmega }\,{:=}\,\rho _P^{\varLambda } \otimes \rho ^{\varOmega \setminus \varLambda }\) is a ground state of \(H_P^\varOmega \,{:=}\, H_P^\varLambda + H_0^{\varOmega \setminus \varLambda } = H^\varOmega + P\).

According to Proposition 9 we have

$$\begin{aligned} \left|{{\mathrm{tr}}\big ({ ({\rho ^\varOmega _P - \rho ^\varOmega }) A}\big )} \right| \, \le \, {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2 \min \{ {{\,\mathrm{dist}\,}}(Y, {\mathbb {Z}} ^\nu \setminus \varOmega ^\circ ), \, {{\,\mathrm{dist}\,}}(Y,X) - 2R\}} \end{aligned}$$

for all \(A\in {\mathcal {A}}_Y\) and \(Y\subset \varOmega \). By requiring \(Y\subset \varLambda \) we obtain

$$\begin{aligned} \left|{{\mathrm{tr}}\big ({ ({\rho ^\varLambda _P - \rho ^\varLambda }) A}\big )} \right|&= \left|{{\mathrm{tr}}\big ({ ({\rho ^\varOmega _P - \rho ^\varOmega }) A}\big )} \right|\\&\le {\mathrm {e}}^{c_1 \left|{Y} \right|} \, \left\Vert {A} \right\Vert \, {\mathrm {e}}^{-c_2 \min \{ {{\,\mathrm{dist}\,}}(\varLambda , {\mathbb {Z}} ^\nu \setminus \varOmega ^\circ ), \, {{\,\mathrm{dist}\,}}(Y,X) - 2R\}}. \end{aligned}$$

Since this bound is independent of \(\varOmega \), we can choose \(\varOmega \) sufficiently large such that \( {{\,\mathrm{dist}\,}}(\varLambda , {\mathbb {Z}} ^\nu \setminus \varOmega ^\circ ) > {{\,\mathrm{dist}\,}}(Y,X) - 2R\). Absorbing \({\mathrm {e}}^{2c_2R}\) in \(c_1\) yields the claim. \(\square \)