Control-driven critical fluctuations across quantum trajectories
Abstract
Monitored quantum circuits in which entangling unitary dynamics compete with projective local measurements can host measurement-induced phase transitions witnessed by entanglement measures at late times. Adding feedback conditioned on the measurement outcomes gives rise to another type of phase transition witnessed by local order parameters and correlation functions. These transitions, known as control or absorbing-state transitions, generically occur within the area-law entanglement phase and are thought to be governed by classical physics in that their critical exponents match those of the classical limit of the model. In this work, we examine quantum features of these transitions, focusing on a Bernoulli circuit model with a well-defined classical limit. First we demonstrate that, in the local basis defined by the absorbing state, the steady-state quantum coherence undergoes a phase transition at the control transition, where its logarithm changes discontinuously from volume- to area-law scaling. Second, we analyze the control transition from the perspective of fluctuations in observables, which carry two contributions: classical fluctuations over circuit realizations (present in the classical limit), and quantum fluctuations over trajectories and states (both absent in the classical limit). Both contributions can be estimated in experiments without post-selection. The circuit-to-circuit fluctuations, the dominant contribution, carry the critical behavior of the classical limit. However, the subleading quantum fluctuations that represent fluctuations between different quantum “worlds” also go critical at the control transition. These critical quantum fluctuations at the control transition also occur in other models, and we discuss how they can be measured experimentally without post-selection.
I Introduction
The non-equilibrium dynamics of strongly interacting quantum systems is a fundamental and timely topic at the intersection of quantum information science and many-body physics. In addition to entangling unitary dynamics, tasks like quantum error correction and state preparation require the ability to perform mid-circuit measurements (i.e., to measure local parts of the system in real time). This capability, which is becoming available on a variety of noisy intermediate-scale quantum (NISQ) hardware platforms, will be an important driver of the transition to the early fault-tolerant era of quantum computing.
The competition between projective local measurements and entangling unitary dynamics drives a measurement-induced phase transition (MIPT) between dynamical phases with extensive volume-law and subextensive area-law entanglement at late times [1, 2, 3, 4, 5]. This phenomenon is inherently quantum mechanical as it can only be witnessed in quantities (e.g. any entanglement diagnostic) that are non-linear in the reduced density matrix. This is a consequence of the fact that the reduced density matrix becomes featureless upon averaging over the outcomes of the projective measurements at any measurement rate. To circumvent this, entanglement measures must be computed in a manner that resolves the quantum trajectories associated with different measurement histories. While this can be achieved experimentally for small systems [6, 7], the number of measurement histories scales exponentially in the number of measurements, which makes scaling up prohibitive. Despite this challenge, known as the post-selection problem, experiments have now observed signatures of the MIPT on trapped ion and superconducting qubit NISQ devices. This defines a new notion of dynamical phases of quantum matter and non-equilibrium phase transitions with universality classes that share close connections to percolation physics.
A natural generalization of measurement-enriched quantum dynamics is adaptive quantum dynamics, where the measurement outcomes are used to control the subsequent dynamics. In particular, we will consider models where they are used to steer the dynamics towards a pre-determined state. For this target state to be stable, generic unitary dynamics cannot be used; instead, a dark or control state is embedded into the unitary dynamics that can allow the feedback from the measurement outcomes to overcome the quantum chaotic evolution. As a result, a control-induced phase transition (CIPT) has been uncovered in several contexts [8, 9, 10, 11, 12, 13, 14, 15]. This is a transition between an active phase, where the system’s steady state is by some measures far from the control state; and a control phase, where the system’s steady state is either a dark state with no fluctuations or is near the control state with very limited fluctuations.
Importantly, unlike feedback-free MIPTs, CIPTs are naturally witnessed by local order parameters or correlation functions that are linear in the density matrix, so they can be studied without postselection. However, a CIPT may or may not coincide with a transition out of the volume-law phase (i.e., a MIPT) depending on whether the feedback acts locally or globally on the quantum state; generically, the MIPT occurs within the active phase, preceding the CIPT, but global feedback can drive them together [10, 11, 13, 12]. At the classical level, these systems realize dynamical phase transitions that result from either the stochastic or deterministic control of chaotic evolution. Embedding such classical critical dynamics into a quantum system is a systematic protocol that can induce a CIPT in a monitored quantum many-body system with feedback. In this paper, we only consider dynamics that take pure states to pure states, so there is no unmonitored coupling of the system to its environment that would produce a mixed state of the system.
As a result, a central question in the field, which is also a main focus of the present manuscript, is if this dynamical transition remains purely classical or if there are any inherently universal, quantum critical degrees of freedom present due to the interplay of measurements, feedback, and chaotic unitary dynamics.
To make this question precise, it is helpful to first identify what kinds of quantum fluctuations are possible in adaptive quantum circuits. The first, which is shared by unitary quantum many-body systems, are the quantum uncertainties that are present whenever there is quantum entanglement in the state of the system. The second, which is due to measurements and possible feedback, involves the differences between quantum states that are produced by different quantum trajectories (different measurement outcomes). In other words, the latter involves fluctuations across the many possible “worlds” of quantum mechanics, corresponding to different measurement and feedback histories. In monitored quantum circuits without feedback the trajectory-averaged density matrix, which includes both types of fluctuations, goes to a long-time steady state that maximizes the entropy, and thus the MIPT is not detectable in quantities that are linear in the density matrix. However, introducing feedback may drive the system to critical behavior (such as the CIPT) that is detectable in the trajectory-averaged density matrix, and thus without postselection.
In this work, we provide precise definitions of classical and quantum fluctuations, including both coherent (within trajectory) and incoherent (across quantum trajectories or “worlds”) quantum contributions, which we use to investigate the quantum properties of CIPTs. The critical universality classes uncovered in quantum CIPTs have so far been governed by classical stochastic processes: a random walk in Ref. [8], directed percolation in Refs. [11, 12, 13], a classical branching-annihilating random walk in Ref. [14], and a probabilistic cellular automaton with long-range correlations in Ref. [16]. We stress that while in each of these cases, the entanglement does display a transition (either volume-to-area or area-to-zero) at the CIPT, it does so with the critical exponents of the classical model. As a result, the universal properties of the entanglement do not simply unveil the distinction between classical and quantum contributions to the critical properties of the CIPT and new insight is required. In the following, we provide a framework to quantitatively describe the universal quantum fluctuations at CIPTs, transitions that arise from embedding a classical dynamical transition into a quantum system, which is applicable to a broad class of adaptive random quantum circuits.
To unveil the quantum features of the CIPT we focus on a model that embeds the classical Bernoulli map under stochastic control [17, 18, 19] into a qubit chain with Haar random unitary gates and conditional reset operations. To show that the framework we present within applies to other models undergoing CIPTs we also analyze a quantum model with an absorbing state transition that has an exact dark state in the dynamics in Appendix F.
This “Bernoulli circuit” model [8, 9, 20, 10] is ideal for our purposes for several reasons. First, it has been studied in both classical and quantum circuits in Refs. [8, 10] and the phase diagram is well understood. Second, the classical model has a control transition that can be derived analytically and whose universal properties are described by a simple random walk. Third, the model’s dynamics are naturally described in terms of an emergent quasiparticle, the first domain wall (defined in Sec. II), that is a sharp point-like object in the classical model but becomes a wave packet in the quantum model; it is this object that undergoes an unbiased random walk at the CIPT. Last, by focusing on local feedback, we can split the CIPT and MIPT so that the control transition takes place entirely within the area-law phase. This enables an efficient simulation using matrix product states (MPS), allowing us to study the critical behavior of the CIPT in systems of up to sites with periodic boundary conditions (see Appendix E for a better estimate of critical exponents).
To set the stage, we begin by considering the probability density of the quantum state averaged over samples (including random initial states, circuit realizations, and measurement outcomes), finding that this “average wave function” inherits the behavior of the classical model. We, therefore, turn to study the fluctuations of the wave function, which are comprised of both classical and quantum fluctuations. If we do not distinguish between these contributions, the classical behavior dominates the signal. However, if we carefully separate out the quantum fluctuations arising from random measurement outcomes and quantum state superpositions and analyze them in their own right, we find that they become critical with universal scaling properties captured by a “quantum” scaling dimension (i.e., a scaling dimension that is zero classically but nonzero in the quantum limit). To show these quantum fluctuations are phase coherent we compute the ensemble-averaged -coherence [21] of the quantum state (defined below), which is quite challenging to compute using MPS. Nonetheless, we are able to compute the -coherence accurately by utilizing the tensor cross interpolation approach [22, 23, 24, 25], which allows us to learn the mapping from an individual bit string to the norm of the corresponding wave function amplitude in the computational basis. The complexity of the method is , where is the maximal bond dimension of the MPS. This allows us to definitively show that the CIPT in the Bernoulli circuit model is, in fact, a transition from quantum coherent to classical dynamics.
The rest of the paper is organized as follows. In Sec. II, we present the model, define the classical and quantum fluctuations, and outline the main results of this work. In Sec. III, we present numerical evidence that the quantum CIPT inherits the features of the classical one at the level of the average wave function. We also probe the -coherence across the CIPT, unveiling the transition’s quantum nature. In Sec. IV, we show that the quantum nature of the control transition manifests in the fluctuations of the wave function. In particular, while the circuit-to-circuit fluctuations for the classical and quantum models are both governed by the random walk universality class, the trajectory-to-trajectory fluctuations develop a non-zero scaling dimension that is universal and only non-zero in the quantum model. We conclude and offer an outlook in Sec. V. In Appendix A, we provide additional details on statistical properties of the wave function. In Appendix B, we derive an expression for the coherence of a Haar random state. In Appendix C, we provide technical details on estimating the coherence in the MPS simulations using tensor cross interpolation. In Appendix D, we study the three kinds of fluctuations examined in this paper for another metric, the magnetization density, to demonstrate the scaling dimension we have estimated is universal. In Appendix E, we use our MPS numerics to obtain a better estimate of the critical point and correlation length exponent of the CIPT studied for smaller system sizes in Ref. [10]. Similarly, we present the trajectory fluctuation in the magnetization in the absorbing-state transition of Ref. [13] in Appendix F.
II Background and Overview of Results
In this section, we first introduce the Bernoulli circuit model used in this paper to demonstrate the concept of isolating the classical and quantum fluctuations in Sec. II.1, and then define each type of fluctuations in detail in Sec. II.2. Finally, we outline the main results of this work in Sec. II.3.
II.1 Bernoulli circuit model

We begin by defining the Bernoulli circuit model as shown in Fig. 1 and reviewing its phase diagram [8, 10]. We first describe the classical version of the model before discussing what changes when quantum superpositions are introduced.
II.1.1 Classical Model
The chaotic dynamics in the Bernoulli circuit model are derived from the classical Bernoulli map defined as [26]
(1) |
where is a real number between 0 and 1. For any rational number , the Bernoulli map generates a finite-length periodic orbit. However, the orbit of any rational is unstable under infinitesimally small deviations as the irrationals are dense on the number line, leading to chaotic dynamics. Thus, we introduce a control map that aims to push the dynamics towards the rational numbers on the orbit of . For any , the control map acts as
(2) |
where is the point on the orbit closest to . In the following, we restrict our attention to the orbit of , which corresponds to a single fixed point such that . At each time step, the control map is stochastically applied to the system with probability to counteract the chaotic dynamics generated by the Bernoulli map, which is applied with probability , as shown in Fig. 1(a) [17].
In order to move towards a quantum analog of this model, we encode the real number in a binary representation truncated to bits,
(3) |
where . Here, we use the bra-ket notation, which applies to both classical and quantum models, with the only difference being that the classical model is restricted to a single element of the computational basis at any given time , while the quantum model allows for superpositions of these states. Under this mapping, the fixed point becomes the polarized state , which is the “control state”.
With the discretization into bit strings, the multiplication by 2 in the Bernoulli map can be realized by a leftward shift of the entire bit string, i.e.,
(4) |
where the first bit is cycled to the leftmost bit to ensure unitarity (or equivalently, we impose the periodic boundary condition). However, this discretization does not yet accommodate chaotic dynamics since the -bit binary representation at finite can only represent a rational number and therefore must return to its initial value after at most applications of the left-shift . Therefore, to restore the chaotic dynamics, we introduce a scrambler acting on the last three bits. We choose the scrambler as a random element , the permutation group of the computational basis spanned by the last three bits. Thus, the discretized Bernoulli map or Bernoulli circuit is realized by the composition of the left-shift and the scrambler, i.e.,
(5) |
as shown in Fig. 1(b). We note that this formulation of the Bernoulli map captures the action of the original map on the normal numbers [27], which are a dense subset of the irrational numbers whose binary expansion is uniformly random. This is sufficient to reproduce the fundamental aspects of the chaotic dynamics in the limit of large , including the model’s Kolmogorov-Sinai entropy of [26, 9].
The control map is naturally realizable in the discretized setting. When the control targets the fixed point , reduces to division by [see Eq. (2)]. This can be accomplished by resetting the last bit to , followed by a rightward cyclical shift of the entire bit string as shown in Fig. 1(d), i.e.,
(6) |
where is the Pauli that flips the value of the bit at the last site. Note that the last bit is flipped only if it was initially set to , guaranteeing that the first bit in the string will be zero after the rightward cyclic bit shift. This ensures that the new bit string will correspond to a number less than . This process erases the initial value of , so the control map in this formulation is intrinsically nonunitary (i.e., irreversible).
II.1.2 Quantum model
The quantum model differs from the classical model in two important ways. First, the scrambler in the Bernoulli map changes from a 3-bit permutation to a 2-qubit Haar random unitary acting on the last two qubits, as shown in Fig. 1(c). That is, the Bernoulli map in the quantum model is given by
(7) |
which, unlike Eq. (5), generates superpositions when acting on a computational basis state. Second, the reset operation entering the control map [Eq. (6)] is implemented using a quantum measurement. A quantum measurement of the th qubit changes a generic quantum state according to the nonlinear operation
(8) |
where is the outcome of the measurement and
(9) |
is the projection operator onto outcome at site . The action of the reset operation in Eq. (6) on a single computational basis state can then be expressed as
(10) |
Note that, for a single computational basis state, is the only possible measurement outcome and the above is equivalent to the reset performed in Eq. (6). However, for a superposition of quantum states the measurement outcomes are no longer deterministic; rather, they are distributed according to the Born rule, i.e., is drawn at random with probability each time a measurement is performed.
II.1.3 First domain wall
A major benefit of working with the present model is that its dynamics can be captured by an object called the first domain wall (FDW). The FDW in an individual computational basis state is defined with respect to the target state as the location of the first “1” in the bit string; e.g., for the state the location of the FDW is labeled by the underline. The FDW can be viewed as the boundary between controlled and uncontrolled regions in the bit string. Its position, measured from the right edge of the bit string, quantifies the distance between that bit string and the fixed point . In particular, when the FDW is at position , ; the extreme limits and correspond to fully uncontrolled and fully controlled, respectively. The FDW also acts like an effective “quasiparticle” that we can track as the system evolves. In particular, we can consider the evolution of an initial (product) state with the FDW at position : with arbitrary . In the classical model, the control map translates the FDW to the right, while the chaotic map translates it to the left, leaving behind scrambled bits in its wake. In the quantum model, the FDW’s location can be promoted to a quantum operator . Under dynamics starting from a computational basis state with the FDW at , the quantum mechanical average FDW position constitutes an “entanglement front” separating a disentangled region to its left from an entangled region to its right (where the Haar scrambler acts), see e.g. Fig. 1 in Ref. [8]. Moreover, the FDW is no longer a perfectly sharp quasiparticle; rather, it is a wave packet with mean position and spread . Thus, the FDW is a convenient object that we can use to separate out classical and quantum aspects of the dynamics.
II.1.4 Phase diagram
The phase diagram of the quantum Bernoulli circuit model involves both a CIPT, where the system transitions from an uncontrolled to a controlled phase, and an MIPT, where the system transitions from a volume-law to an area-law phase [8, 9, 20, 10]. The controlled and uncontrolled phases can be characterized by a local order parameter, the magnetization density
(11) |
where is a Pauli operator whose eigenstates are the local computational basis states. In the “chaotic” or uncontrolled phase, the system stays away from the control state and at late times and , while in the controlled phase, the system always is driven near the control state, and the magnetization density is nonzero at late times. The volume- and area-law phases are characterized by the system-size scaling of entanglement measures as discussed in Sec. I.
In principle, the CIPT and MIPT can occur simultaneously or separately as a function of the control rate , depending on the locality of the control map [10]. When the control map targets the fixed point (i.e., the polarized state ), they occur separately, and three phases emerge: a volume-law chaotic phase, an area-law chaotic phase, and a disentangled controlled phase [see Fig. 1(e)]. The MIPT between volume-law and area-law chaotic phases occurs at and its nature is inherently quantum. The CIPT between area-law chaotic and controlled phases occurs at in both the classical and quantum models defined by Eqs. (5) and (7), respectively. For more details on the phase diagram, we refer to Refs. [8, 10].
In this paper, we are primarily interested in the features of the CIPT around , which occurs within the area-law phase of the model. Thus, in addition to the usual exact state vector evolution [8, 10], we can take advantage of matrix product states (MPS) to efficiently study the critical behavior (note that the entanglement remains area-law even at the CIPT). We adopt a technique called tensor cross interpolation to compute the quantum coherence in polynomial complexity, which would otherwise be exponentially hard to compute in the MPS formalism.
II.2 Separating classical and quantum fluctuations

We now introduce the main concept of isolating different types of fluctuations to reveal the quantum nature of seemingly-classical transitions in the adaptive monitored circuit. This idea is broadly applicable to various models with a dark or control state, e.g., the CIPT in the competition between chaotic and controlled dynamics [8], and absorbing-state transitions in adaptive monitored circuits [13]. In the following results, we will use the CIPT as a paradigmatic example to illustrate the concept. The application of this idea to another model with an absorbing state transition is discussed in Appendix F.
The aim is to determine the variance of a generic quantum operator . To begin, we define all quantities being averaged. Starting from an initial pure state , we have a sequence of stochastic events that either apply a unitary or a measurement with feedback. The combination of the initial state and the sequence of unitaries and measurements defines one circuit realization labeled by . Each time step (e.g., in Fig. 1(a)) that the circuit performs a measurement, the outcome is randomly sampled from the Born probability distribution with outcome . We denote the full measurement history of a trajectory for circuit realization by the vector ; we seek to parse the fluctuations into those due to variations between circuits and those due to variations within a fixed circuit .
We are now in a position to specify an average over “samples”, where each “sample” is a single trajectory of a single circuit, indexed by . The average over samples is then
(12) |
Note that since this is a simple average (no post-selection), it can be experimentally estimated by gathering many samples. We further stress the nested form of the averages (also denoted through the conditional probability ) that allows us to take the classical limit, which has deterministic measurement outcomes, so for fixed circuit , all classical trajectories are identical.
If we make projective measurements of operator , giving results for , the variance of these single-shot experimental observations across can be estimated without post-selection by
(13) |
It is now straightforward, using Eq. (12), to see that this will involve a combination of fluctuations over quantum trajectories (i.e., measurement outcomes for a fixed circuit realization) and circuit-to-circuit fluctuations that also exist in the classical limit of the model. Therefore, we can now decompose this variance over samples into classical circuit fluctuations and quantum fluctuations:
(14) |
where and denote averages over circuits , and different trajectories given a circuit , respectively. In going from the first to the second line in Eq. (14), we have added and subtracted the quantity , where is for a single shot measurement of the measurement history given a circuit . The first term, circuit fluctuations, pertains to the classical limit of choosing different circuits to evolve. The second term, quantum fluctuations, is the variance of the outcome of measuring over many trials with the same circuit . For the classical model, only the circuit fluctuations are nonzero because the measurement outcome is deterministic, while for the quantum model, both circuit and quantum fluctuations can be nonzero.
Theoretically and, if we allow postselection, experimentally, the quantum fluctuations in Eq. (14) can be further decomposed into two parts:
(15) |
where denotes the quantum state expectation over the wave function of the system immediately before any measurement of is made. (Note that with 1 and 2.) The first term, trajectory fluctuations , characterizes the uncertainty of different quantum trajectories , coming from the randomness in the outcomes of the measurements that are made earlier than the measurement of . The second term, state fluctuations , characterizes the quantum nature (superposition) of the pure state immediately before the measurement of is made. These two terms capture different aspects of the quantum fluctuations. In the MIPT without feedback, the transition is seen only in properties of the state , although this is in entanglement properties rather than simple observables.
For our model with feedback, we will show that the trajectory fluctuations and state fluctuations both become critical at the CIPT, i.e., they obey single-parameter scaling. Whereas both parts of the quantum fluctuations are large for , they become small for , where only small fluctuations around a classical trajectory remain. One open question about more general CIPT models is whether there exist models where the critical behavior differs between the trajectory fluctuations and the state fluctuations.
II.2.1 Experimental tractability
The separation of the observable fluctuations in Eq. (14) not only serves for a conceptual understanding of the quantum nature of the CIPT, but also provides a practical way to experimentally measure the quantum fluctuations, as this separation does not require post-selection. The first term in Eq. (14), the circuit fluctuations [see Fig. 2(a)], can be experimentally sampled without post-selection. This is because the first contribution is obtainable by first fixing a specific circuit , and then randomly sampling the different measurement outcomes and the random shots at the final time following the Born rule given that and . The second contribution involves a simple average over all measurement outcomes and shots.
The second term in Eq. (14), the quantum fluctuations can also be estimated without post-selection in experiments. We can fix a specific circuit , randomly sample the trajectories , and collapse the entire wave function at the final time to collect a single shot of the observables and . Repeating this process for each sampled trajectory, we can compute the variance given a specific circuit to obtain the quantum fluctuations in Eq. (14).
However, separating the quantum fluctuations into the trajectory fluctuations [the first term in Eq. (15) and also illustrated in Fig. 2(b)], and the state fluctuations [the second term in Eq. (15) and also illustrated in Fig. 2(c)]– in experiments seems to require postselection. This is due to the measurement of the quantum average , which involves repeated realization of the same pure state by post-selection Fortunately, in the Bernoulli map model with as the control state, as we will show later, these two fluctuations share the same scaling dimension at the CIPT, and therefore, their combination shows the same critical behavior. This also verified in Appendix D.4, where we present a direct numerical simulation of the shot-to-shot fluctuation finding results consistent with those in Sec. IV.2 for the trajectory and state fluctuations, respectively.

II.3 Summary of main results
Having addressed these preliminaries, we now briefly summarize our main results regarding the quantum nature of the CIPT.
-
1.
At the level of ensemble-averaged wave function properties (e.g. the ensemble-averaged distribution of the wave function over computational basis states), the quantum model looks similar to the classical model near the CIPT.
-
2.
The CIPT nevertheless manifests a phase transition in a quantum information-theoretic quantity: the ensemble-averaged -coherence changes from an exponential growth as a function of system size in the chaotic phase to a saturating -independent value in the controlled phase. At the critical point, the coherence growth remains exponential, indicating the critical wave function is quantum coherent.
-
3.
At the level of fluctuations in observables, the circuit-to-circuit fluctuations present in both the classical and quantum limits provide the dominant contribution and manifest the critical properties of the classical model.
-
4.
Although the trajectory-to-trajectory fluctuations, which appear only in the quantum limit, are subdominant, their contribution can be separated from the circuit-to-circuit fluctuations and measured experimentally. These intrinsic quantum fluctuations also become critical at the CIPT, and develop a non-zero scaling dimension that governs the algebraic decay of these fluctuations at the critical point.
These results provide a precise framework to demonstrate that the CIPT, which naively appears fully classical in nature, in fact, manifests inherent quantum critical properties that were previously “washed out” (or hidden) by equally averaging over circuits and measurement outcomes. We defer discussion of this point and further consequences to Sec. V.
III Ensemble-Averaged wave function Properties
Before discussing the different types of fluctuations, we first consider ensemble-averaged properties of the wave function, as it provides a direct connection to the classical limit. We analyze the probability distribution of the bit-string-resolved wave function, ensemble averaged over different circuits and trajectories, without separating the quantum and classical contributions, and find that the quantum and classical results are essentially indistinguishable. However, a distinction appears when we compute the ensemble-averaged -coherence of the wave function to demonstrate that the system is quantum coherent at the CIPT. In the regime governed by quantum dynamics, the coherence is exponentially large (in the number of qubits ), and in the controlled phase, it saturates to an -independent value. At the CIPT critical point, it retains an exponential growth, indicating the average wave function is quantum coherent in the classical computational basis. This implies that the CIPT in the quantum model has become more than the classical transition from which originates, and we therefore need to look at its quantum effects in a precise manner, which is the focus of the section following this one.
III.1 Ensemble-averaged bit string distribution
To explicitly visualize how the control map is imprinted upon the quantum state, we plot the ensemble-averaged probability distribution over bit strings as a function of the control rate for both the classical [Fig. 3(a)] and quantum [Fig. 3(b)] Bernoulli circuit models for system size . Here, the probability of finding the state in a specific bit string is defined as
(16) |
where is the steady state of the system for a specific sample including a fixed circuit realization and measurement history . In the classical model, the system is in a simple product state at all times.
In Fig. 3(a,b), we notice a striking visual resemblance between the classical and quantum models—as the control rate increases from 0, the distribution of the bit string changes from a uniform distribution over all bit strings (corresponding to an ergodic chaotic phase) to a distribution localized at the fixed point of the polarized state .
To understand the structure in the computational basis in more detail we turn to Figs. 3(c-e), where we present bit string distributions for three typical values of corresponding to the chaotic phase at (orange), the critical point at (red), and the controlled phase at (green), respectively. We see for that is almost uniformly distributed across all the basis states, namely , where is the measure coming from the discretization of the interval . For , we find up to a tail that goes to zero in the thermodynamic limit (see Appendix A for more details on the scaling of the distribution with system size ), demonstrating that the wave function “sticks” to the fixed point in the controlled phase. At the CIPT , the bit string distribution takes the power law form .
An interesting feature is the staircase pattern in the distribution of bit strings, , at a given , where abrupt changes all happen at bit strings that are inverse of the power of 2, and probability density within each interval remains almost uniform. The positions of abrupt changes motivate us to define the position of FDW measured as the first (leftmost) “1” from the right edge of the bit string . For example, and have , and the polarized state has . Formally, we can define the FDW position for as
(17) |
where is the floor function.
Therefore, the state of the system can be effectively described by the FDW location instead of tracking the entire wave function, hence providing an effective metric to monitor its dynamics. (see Appendix A for more quantitative analysis of the FDW distribution.)
III.2 Quantum coherence


In the previous section, we found that the ensemble-averaged FDW distribution is the same for both the classical and quantum models (see Appendix A for a quantitative analysis of the two distributions), which does not inform us about the quantum nature of the CIPT. However, we can probe quantum effects by directly looking at the essence of a quantum state, i.e., its coherence due to superposition.
The coherence measure we adopt here is the ensemble-averaged -quantum coherence [21]
(18) |
where is the density matrix for a specific sample , and is the off-diagonal element of the density matrix corresponding to . The summation runs over all the off-diagonal elements of the density matrix, which originate from multiple superposition components within the quantum state. Consequently, the -coherence is manifestly zero in the classical model. Note that we choose to focus on the average coherence of the state rather than the coherence of the average state as, in the latter case, the sample average washes out the off-diagonal density-matrix elements, leading to zero coherence. This is similar to the reason why ensemble-averaged entanglement measures are considered in studies of MIPTs.
In our numerical simulations of the coherence, we use both state-vector and MPS evolution algorithms. We use state-vector evolution to compute the coherence throughout the phase diagram (including the volume-law phase) up to . Within the area-law phase, which includes the CIPT, the object of our study, we use MPS to simulate system sizes beyond . Here, the nontrivial part is to compute the element-wise absolute value of the MPS wave function without fully contracting the internal legs of the MPS, which would lead to an exponential memory cost. We, therefore, use tensor cross interpolation [22, 23, 24, 25] (TCI) to learn the mapping from the physical index of an MPS to the norm of the corresponding wave function amplitude:
(19) |
where corresponds to the computational basis state with . With TCI, we can directly obtain each element in the density matrix—in complexity where is the maximal bond dimension of the MPS—without fully contracting the MPS. We choose a sufficiently large maximal bond dimension to capture the wave function within the area-law phase. More details on the TCI method are provided in Appendix C.
We start with an initial product state with FDW location and evolve the system to the steady state, which is reached after time steps. In Fig. 4, we plot the steady-state coherence as a function of system size for different using state-vector evolution for the chaotic phase in Fig. 4(a) and MPS for the critical and controlled phases in Fig. 4(b). In the chaotic phase [Fig. 4(a)], we find that the coherence grows exponentially with , namely . At , we analytically find as from the coherence of a Haar random state (see Appendix B), which is the maximal possible coherence. For a finite in the chaotic phase, the coherence continues to grow exponentially, however, with . Surprisingly, we find that at the critical point, the coherence remains exponential with . In contrast, for , we find that saturates to a system size independent value. This motivates the hypothesis that the coherence can be parameterized as , with becoming non-analytic at the control transition. To test this, we apply an empirical “proof by contradiction” by assuming is analytic in , so that an asymptotic expansion of the form
(20) |
holds. We will show that the coefficients of this expansion become singular near the critical point, demonstrating that becomes non-analytic at this dynamical quantum phase transition.
We analyze the fitted parameters , , and in Fig. 5 by gradually excluding smaller system sizes from the fitting. In Fig. 5(a), we find that , which parameterizes the exponential growth of the coherence, remains almost constant throughout the chaotic phase up to the CIPT, where it jumps to zero. As we continue to exclude smaller system sizes, the jump becomes more abrupt, as shown in the inset. In Fig. 5(b), we study , which parameterizes the system-size independent contribution. Starting with at zero control rate, we find that decreases monotonically with and reaches its minimum at the critical point, which is consistent with the decreasing growth exponent in Fig. 4(a). In the controlled phase at , we find that also decreases monotonically but from a large positive value. Here, corresponds to the saturation coherence at large , which is consistent with the decreasing saturation coherence for larger in Fig. 4(b). The growth from the minimum value to the large positive value between and is a finite-size effect: The data in the inset show that the peak of in the controlled phase near becomes sharper as we exclude smaller system sizes from the fitting as shown in the inset.
Finally, in Fig. 5(c), we show data for , which parameterizes the subleading correction of order . We notice that it remains zero in both the chaotic and controlled phases but diverges at the critical point, consistent with the function becoming non-analytic at the transition in the thermodynamic limit . It is striking that the coherence remains exponentially growing at the transition, demonstrating that the critical wave function is inherently quantum mechanical.
IV Classical vs. quantum fluctuations of observables
The critical behavior of the quantum coherence already demonstrates the quantum nature of the CIPT in the quantum model. However, quantum coherence is challenging to measure experimentally as, like the entanglement entropy, one must compute the coherence of each sample before averaging over samples. It is therefore preferable to try to access the quantum nature of the CIPT with quantities that do not require post-selection. In Sec. III, we showed that the ensemble-averaged bit string distribution is dominated by classical behavior. Nevertheless, as discussed in Sec. II.2, considering the sample-to-sample fluctuations of an observable allows us to separate out quantum and classical fluctuations. In the following results, we will demonstrate that the quantum nature of the CIPT can be observed in the quantum contribution to these fluctuations.

IV.1 Classical circuit-to-circuit fluctuations
We first consider the dominant contribution to the unresolved fluctuations in the quantum model, namely the classical circuit-to-circuit fluctuations
(21) |
where is the trajectory-averaged steady-state FDW expected value given a specific circuit .
To probe the classical fluctuations, we choose an initial state with the FDW at , and allow the circuit to reach the steady state (the dynamics will be discussed in a sequel [28]). The classical nature of the circuit-to-circuit fluctuation can be seen in the steady-state value as a function of for different system sizes , as shown in Fig. 6. Here, we find that the steady-state fluctuations peak at the critical point, with the peak value scaling as , consistent with the dynamical exponent of in the unbiased random walk. With the finite-size scaling ansatz
(22) |
we find data collapse as shown in the inset of Fig. 6 with the estimated critical exponents and consistent with the random walk universality reported in Ref. [8].


IV.2 Fluctuations across quantum trajectories
The steady-state trajectory fluctuation in Eq. (13), which measures fluctuations across different quantum trajectories for a fixed circuit realization, is unique to the quantum setting as it is only nonzero when the measurement outcomes are random:
(23) |
where is the steady state FDW expected value for a specific quantum trajectory given a specific circuit . It is subdominant [] compared to the classical circuit-to-circuit fluctuations [], so its contribution is not visible in the full average over samples. However, as discussed in Sec. II.2, it can be measured independently in experiments. We also examine the trajectory fluctuation using the magnetization density in Appendix D, finding results consistent with those for the FDW.
As an illustrative example, we first visualize the temporal spreading of the trajectories of the averaged FDW in Fig. 1(e) starting from for the three representative control rates , , and in the quantum model. Within each panel, we plot a collection of quantum trajectories given the same circuit realization (i.e., the same realization of the unitary scrambler in the Bernoulli map and the same sequence of chaotic and control time steps). The visible fluctuations come from the different measurement outcomes . In the chaotic phase (left panel), the trajectories start to diverge immediately from the initial state at and quickly saturate to the left end of the chain at . The large variance over different trajectories reflects the nature of the quantum dynamics due to the chaos in the Bernoulli map. However, in the controlled phase (right panel), the trajectories remain close to the fixed point, overlapping with each other, and the spreading of the trajectories only happens when the chaotic map is applied multiple times in a row (which is a rare event inside the controlled phase). This demonstrates the scenario where the quantum dynamics with a large spreading of trajectories is reduced to an effectively classical dynamics with a common trajectory. At the critical point in the middle panel, we see critical behavior where the FDW undergoes an unbiased random walk, and the spreading of the trajectories remains .
Figure 1(e) provides an intuitive picture of the trajectory fluctuations. To quantify these fluctuations, we plot in Figs. 7(a-c) the probability distribution of in the steady state for the three representative values , 0.5, and 0.6 over different circuit realizations . 111We evolve the circuit up to , and confirm that the dynamics reaches a steady state for . Therefore, all states within can be treated as separate samples for constructing the histogram in Fig. 7 to enhance the smoothness of the statistics with minimal additional computational cost. We also confirm the qualitatively same results using only the data at final time step . We find that in the chaotic phase [Fig. 7(a)], most of the trajectory fluctuations are finite (around ) and it is unlikely to have zero fluctuations in the thermodynamic limit—the probability of zero fluctuations is exponentially small in system size. At the critical point [Fig. 7(b)], the probability of zero fluctuations instead decays algebraically as a function of system size. In the controlled phase [Fig. 7(c)], most of the trajectory fluctuations are zero regardless of system size with an exponential tail of finite fluctuations, indicating classical dynamics that converge around a single trajectory with deterministic measurement outcomes.
This change in the distribution of the trajectory fluctuations as a function of motivates us to define an order parameter as the probability of zero fluctuations,
(24) |
where is a small numerical cutoff. This order parameter is shown in Fig. 8 as a function of for different system sizes . It vanishes in the chaotic phase, decays algebraically at the critical point, and saturates to a finite value in the controlled phase.
The algebraic decay of the order parameter at the critical point exposes another scaling dimension defined as
(25) |
in the and limit, characterizing the onset of classicality. Here, we denote the scaling dimension by to make an analogy to the order-parameter critical exponent in the conventional context of continuous phase transitions. In the classical model, does not exist since the trajectory fluctuations are manifestly zero, and therefore will be always 1. In the quantum model, to extract the scaling dimension , we perform finite-size scaling of the order parameter following the scaling form
(26) |
In the inset of Fig. 8, we estimate the new scaling dimension as , along with , consistent with the classical results. This unveils another inherently quantum aspect of the CIPT which was previously overlooked due to the subleading nature of the quantum contribution to the sample-to-sample fluctuations. These universal quantum fluctuations should be generic to other adaptive quantum dynamics as well. In Appendix F, we show that the absorbing-state transition studied in Ref. [13] exhibits a similar behavior where the quantum trajectory fluctuations become critical and are then suppressed once the system enters the absorbing phase (analogous to the controlled phase here). The only difference lies in the vanishing scaling dimension in the trajectory fluctuation.
IV.3 Fluctuations across quantum states

Having explored trajectory fluctuations in detail we now turn to a state fluctuation in Eq. (14). Similarly, we study the FDW location as
(27) |
where is the second moment of for a specific quantum trajectory and a fixed circuit . This quantity intuitively estimates the average spreading of the FDW wave packet within a single quantum trajectory. For the classical model, Eq. (27) is also by definition zero because the “wave function” is a product state with a sharp FDW location, as opposed to a quantum wave packet. For the quantum model, the Bernoulli map generates quantum coherence as it scrambles a product state into a superposition of product states.
Similar to the trajectory fluctuations in Eq. (24), the distribution of the state fluctuations at the steady state can also be used to unveil the quantum nature of the CIPT. Here, we can define the probability of zero fluctuations in for different circuits and trajectories as an order parameter similar to Eq. (24). The order parameter also changes from zero in the chaotic phase to a finite value in the controlled phase with an algebraic decay at the critical point, as shown in the lower inset in Fig. 9, similar to Eq. (24). To extract the corresponding scaling dimension , we plot in Fig. 9 the order parameter as a function of for to . The upper inset in Fig. 9 shows the finite-size scaling of the order parameter following the scaling form in Eq. (26) to find the scaling dimension , with critical exponent , and critical measurement rate , which is consistent with the critical exponents extracted from the trajectory fluctuation in Sec. IV.2.
Although both the trajectory and state fluctuations in the Bernoulli map model exhibit the same critical behavior at the CIPT, we notice that they are quantitatively different. In the controlled phase, the trajectory fluctuations (Fig. 8) have a larger order parameter than the state fluctuations in Fig. 9, indicating that the states with zero state fluctuations are a subset of those with zero trajectory fluctuations, given the ferromagnetic state as the dark state. This suggests that the state fluctuations being zero is a stronger condition than the trajectory fluctuations being zero. For example, when the states across all trajectories are reset to the fixed point (e.g., after many consecutive applications of the control map), a fixed Bernoulli map in the next time step drives all states to the same state , leading to a zero trajectory fluctuation, while finite state fluctuation due to the coherence.
The opposite scenario with finite trajectory fluctuations but zero state fluctuations can also exist. For example, in the conventional Haar-random MIPT bricklayer model without any feedback, the trajectory fluctuations are always finite regardless of the measurement rate, while the state fluctuations are zero beyond the connectivity transition. Adaptive circuits with other feedback operations targeting other dark states can lead to different qualitative behaviors for the two types of quantum fluctuations, which is an interesting direction for future research.
V Discussion
In this work, we have provided a framework to characterize the quantum nature of CIPTs. The classical contributions have been precisely identified and, in the case of the Bernoulli circuit model, have been shown to nicely capture the average long-time steady state properties, including the universal properties of the underlying classical absorbing state transition. By separating out the classical and quantum contributions to an average over measurement outcomes as in Eq. (12), we have been able to identify a critical mode associated with trajectory-to-trajectory fluctuations governed by a universal scaling dimension unique to the quantum limit. These critical fluctuations among the many “worlds” of quantum mechanics can be directly measured on NISQ hardware without the need for post-selection.
We also analyzed the quantum coherence across the CIPT using a combination of exact state-vector evolution and matrix product state simulations leveraging tensor cross interpolation. By uncovering the critical behavior of the coherence at the CIPT, we have shown that absorbing-state transitions embedded into quantum systems also entail a phase transition between quantum coherent and fully classical dynamics.
In the models we have investigated in this work, the phase transition in trajectory-to-trajectory fluctuations and quantum coherence coincide. However, this need not be the case in general. For example, if we were to instead consider controlling onto an area-law entangled state, such as the Greenberger-Horne-Zeilinger or cluster states as in Ref. [13], the two transitions may split apart. Understanding the structure of these critical properties in a precise manner is now possible utilizing the model-independent framework developed in this work. Opening this up to target states with various patterns of entanglement and correlations is a fascinating direction for future research.
Acknowledgments
We thank David A. Huse for his valuable feedback on the manuscript, as well as Kemal Aziz, Abhinav Deshpande, Sriram Ganeshan, Luke Govia, Barbara Jones, Bibek Pokharel, Oles Shtanko, Maika Takita, and Justin Wilson for many valuable discussions and for collaboration on related work. This work is partially supported by US-ONR grant No. N00014-23-1-2357 (H.P. and J.H.P.) and by the National Science Foundation under Grant No. DMR-2143635 (T.I.).
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- Note [1] We evolve the circuit up to , and confirm that the dynamics reaches a steady state for . Therefore, all states within can be treated as separate samples for constructing the histogram in Fig. 7 to enhance the smoothness of the statistics with minimal additional computational cost. We also confirm the qualitatively same results using only the data at final time step .
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Appendix A Distribution of the bit string and the first domain wall
In Sec. III.1, we introduce the distribution of the bit string . In this section, we show that it is directly related to the distribution of the first domain wall , which is exponential distribution with an exponent which can be numerically extracted in Fig. 10(b).
With the concept of FDW, it is convenient to rewrite the distribution of bit string in to a more compact form by grouping bit strings according to their FDW location and plot the cumulative distribution . In Fig. 10(a), we find that takes an exponential form for both the classical and quantum models. To analyze the behavior of as a function of , we define the ansatz
(28) |
where the exponent is a fitting parameter that characterizes the distribution. When (), the FDW is localized at (), reflecting that the system is in the controlled (chaotic) phase. As increases from zero, the exponent passes through zero at the CIPT, as shown in Fig. 10(b).

With the exponent known, we can further analytically derive the scaling behavior of the distribution of the bit string and the first domain wall .
At zero control rate , the distribution of the FDW is simply proportional to the number of bit strings within same FDW , i.e., . Therefore, should be 1 as also numerically verified in Fig. 10(a).
As increases, the linearity remains but with a smaller slope below 1 until approaches the critical rate , which gives a zero slope , indicating a uniform distribution as a function of the FDW , i.e., . The uniform distribution of at indicates that the bit strings start to localize at the fixed point as the distribution of the bit strings .
Beyond the critical point , the distribution of FDW is linear with a negative slope, implies a distribution of the FDW as with . This indicates an exponential localization of the fixed points with at compared to the algebraic decay at . At the limit of control , the slope indicates that the fixed points are the only possible states.
In summary, considering the normalization factor, the complete description of the distribution of the bit string in Eq. (16)
(29) |
where
(30) |
for being the position of FDW for the bit string . Here, the only unknown parameter is the slope where it changes from at to 0 at and to at , which can be fitted numerically in Fig. 10(b). We also note that the slope converges for both the classical and quantum models, which reiterates the fact that the quantum model inherits the classical critical point.

A.1 Scaling of the tail
With the analytic description of the distribution of the bit string, we can fully understand the drastic change in controllability before and after the critical point by studying the distribution of the tail (i.e., ) in Fig. 11. We show the distribution of the tail for different system sizes from the chaotic phase ( in Fig. 11(a)), to criticality ( in Fig. 11(b)), and finally to controlled phase ( in Fig. 11(c)).
In order to compare different system sizes on an equal footing, we define the probability density function over a continuous variable , which can be considered as an extrapolation to the thermodynamic limit. The probability density function is obtained by factoring the measure of a single bit string (i.e., ). Namely,
(31) |
In the chaotic phase as shown in Fig. 11(a), we find that the probability density function converges to an -independent distribution, which can be also understood from the analytic result Eq. (31) and Eq. (30) with
(32) |
Here, the last line is obtained because for in the thermodynamic limit, and by noting Eq. (17).
At the critical point as shown in Fig. 11(b), the probability density function decays algebraically as increases because,
(33) |
This can also be visually confirmed in Fig. 11(b) that is an exponential distribution independent of .
Finally, in the controlled phase as shown in Fig. 11(c), the probability density function decays exponentially as increases for the tail while diverges at the fixed points in the thermodynamic limit because
(34) |
where for . Therefore, in the thermodynamic limit, any non-fixed point bit string will be exponentially suppressed in the controlled phase, which indicates a Dirac -distribution for the fixed point, i.e., . This means that all the dynamics will be steered to the fixed point given a sufficient rate of control maps () in the thermodynamic limit. The -independent exponential decay of in Fig. 11(c) also confirms the analytic result Eq. (34).
Appendix B Quantum coherence for a Haar random state
In this section, we analytically derive the -coherence of a Haar random state, denoted as
(35) |
where is the total number of basis, and are uniformly distributed on the surface of a unit sphere, i.e., .
Following Eq. (18), the -coherence for averaged over the Haar random ensemble is
(36) |
where the new measure in is
(37) |
from the polar coordinate on a hypersurface defined as
(38) |
Here, each integrates from to except for the last one integrates from to . (Note that is not independent, so we only have to .) The third equal sign is due to the cyclic symmetry under the permutation of and .
The last line in Eq. (36) can be decomposed into the product of the following three integrals
(39) |
(40) |
and the normalization factor
(41) |
This leads to each off-diagonal element contributing on average
(42) |
and therefore, the -coherence averaged over the total number of basis is
(43) |
Since is exponentially large to system size , in the thermodynamic limit, the -coherence of a Haar random state per basis is .
Appendix C Tensor cross interpolation
In this section, we provide parameters on the tensor cross interpolation method used in the main text to compute the -coherence from the MPS. Since we always stay in the area-law phase, we can ensure that the bond dimension of the MPS will not grow exponentially with the system size . Therefore, for the circuit evolution, we only set the truncation error as without restricting the allowed maximal bond dimension.
Although the efficient simulation of the circuit using MPS is possible, the tensor cross interpolation of the final wave function to compute the -coherence, which requires resources, is not guaranteed for large system sizes a priori. Therefore, we first validate the tensor cross interpolation method using the package ‘TensorCrossInterpolation.jl’ [30] to estimate the -coherence in small systems sizes () by comparing the results with the exact state-vector evolution to find consistency.
For larger system sizes, we rely on the following error analysis. Since the TCI essentially is an interpolation method, meaning that for each bit string , we can evaluate its deviation from the exact value (e.g., the norm of the wave function amplitude) by contracting all internal indices. We randomly sample a few thousands different bit strings, and take the largest difference between the exact and interpolated values, which provides an estimate of upper bound of the error of the tensor cross interpolation, denoted as given a maximal bond dimension in TCI and a system size .
Finally, we can estimate the propagation of error from TCI to the -coherence of a specific pure state , given by
(44) |
where is the wave function amplitude of the pure state at a given basis (see Eq. 35). Here, to efficiently compute the summation in the last equation in Eq. (44) (i.e., ), we take the inner product of the interpolated MPS representing the vector with an all-one vector of the same dimension. With the upper bound of error in , we can estimate the final error of the -coherence by substitute , which gives the maximal error of the -coherence as . Therefore, we control the error of the -coherence to be (i.e., the relative error is bounded by ) by increasing the allowed maximal bond dimensions in the TCI, and finally, find the empirical the allowed maximal bond dimensions to be , and 4000 for , and 50, respectively.
Appendix D Fluctuations of the magnetization density

In this section, we additionally present the fluctuations of the magnetization density defined as
(45) |
serving as a ‘generic’ order parameter, to confirm the universality of the scaling dimension of these quantum fluctuations by demonstrating the same critical exponents as those in the main text.
D.1 Circuit-to-circuit fluctuations
D.2 Fluctuations across quantum trajectories


The fluctuations across quantum trajectories of the magnetization density are defined similarly to Eq. (23) as
(47) |
Here, we also find the same transition in the distribution of the fluctuations across quantum trajectories from the chaotic to controlled phase, as shown in Fig. 15, where the probability of zero fluctuations increases, and plot the probability of the zero fluctuations as shown in Fig. 14. We find a similar scaling dimension as in Fig. 8.
D.3 Fluctuations across quantum states

We also verify the fluctuations across quantum states
(48) |
and present similar results of finite-size scaling of the probability of zero fluctuations as shown in Fig. 15.
D.4 Fluctuations across different shots

Finally, we study the total quantum fluctuation of the magnetization density. We define the order parameter , the probability of zero quantum fluctuations, similarly, and find it exhibits the same critical behavior and exponents as in the trajectory fluctuation and state fluctuation, as shown in Fig. 16.
Appendix E Finite-size scaling of magnetization density using MPS

In this section, we present a better estimate of the critical exponents at the CIPT with larger system sizes up to . We focus on the steady-state ensemble-averaged magnetization density , and present the results in Fig. 17. The critical exponents at the transition can be better estimated under larger system sizes following
(49) |
where is a universal scaling function for the ensemble-averaged total magnetization density. We present the data collapse in the inset of Fig. 17, and extracted a critical exponent of and .
Appendix F Trajectory fluctuation in the absorbing-state transition


In this Appendix, we study trajectory fluctuations in the absorbing state transition of Ref. [13] and show that they become critical in a manner analogous to the discussion in Sec. IV.2.
We target a ferromagnetic absorbing state in an -site 1D qubit chain. The random unitary process is built from two-qubit gates of the form , where acts trivially on the basis state , preserving the absorbing state, and is a Haar-random unitary that scrambles the other three basis states , , and . The feedback consists of local reset operations in which a qubit is measured in the computational basis, and flipped only if the measurement outcome is (i.e., we choose to always correct with using the notation in Ref. [13]); otherwise, the qubit remains in . The circuit follows a bricklayer structure, with two-qubit random unitaries applied to even and odd pairs of qubits alternately, and interspersed with single-qubit measurements followed by feedback with probability of . The absorbing-state transition happens at with a dynamical exponent of and a temporal critical exponent of [13].
The order parameter to probe the absorbing-state transition can similarly be chosen as the defect density
(50) |
which is a shift to the magnetization density in Eq. (11), and the fluctuations across quantum trajectories are defined as
(51) |
similar to Eq. (47).
We simulate the absorbing-state transition model using state-vector evolution, and present the fluctuations across quantum trajectories for the steady state at for three different measurement rates in the non-absorbing phase [Fig. 18(a)], the critical point [Fig. 18(b)], and absorbing phase [Fig. 18(c)]. As the measurement rate increases, the probability of zero fluctuations also increases, indicating a transition from quantum to classical dynamics. This transition is also unique to the quantum model of the absorbing-state transition, since the classical stochastic process to mimic the dynamics of the diagonal elements of the density matrix does not manifest this transition.
We present the probability of zero fluctuations as a function of the measurement rate along with the finite-size scaling in Fig. 19, following the same definition in Eq. (24) as
(52) |
Here, unlike the order parameter in the control transition presented in the main text as shown in Figs. 8 and 14, the absorbing-state transition model manifests a universal crossing at the critical point for different system sizes. Therefore, we can perform the finite-size scaling according to
(53) |
and find a critical measurement rate and a spatial critical exponent , which is close to the derived as in Ref. [13].