# Theoretical Background

December 14, 2016 12:13 pmHeisenberg’s uncertainty principle is probably the most famous statement of modern physics and familiar to most in the formulation of *standard deviations*, such as for *position* and *momentum* , or as , for *arbitrary non-commuting observables* and . However, a naive *Heisenberg-type error-disturbance relation (EDR)*, for non-commuting observables, denoted as is *not* valid in general. In addition, if one looks closely at the way the uncertainty principle is used by Heisenberg and Bohr in their analysis of though experiments, it emerges that their arguments cannot be – and in fact are not – based on a relation in terms of *standard deviations*. The uncertainty principle turns out to be a much more *intricate* statement.

*Contents:*

Heisenberg’s Uncertainty Principle

Ozawa’s generalized Uncertainty Relation

””””Tighter uncertainty relations

””””Mixed state uncertainty relations

Busch/Werner/Lahti’s Proof of Heisenberg’s original Error-Disturbance Relation

Information-theoretic (e*ntropic*) Uncertainty Relations

””””Entropic uncertainty relations for projective qubit measurements

””””Information-theoretic uncertainty relations for general qubit measurements

## **Heisenberg’s Uncertainty Principle**

**Heisenberg’s Uncertainty Principle**

The * uncertainty principle* represents, without any doubt, one of the most important cornerstones of the Copenhagen interpretation of quantum theory. In his celebrated paper from 1927

^{1}Werner Heisenberg gives at least

*three*distinct statements about the limitations on preparation and measurement of physical systems: (i) It is impossible to

**a system such that a pair of**

*prepare***(**

*noncommuting**incompatible*) observables are arbitrarily well defined. In the original paper the observables are represented by position and momentum. In every state the

*probability distributions*of the observables will have

*widths*that obey a (

*preparation*)

*uncertainty relation*. (ii) Incompatible observables cannot be

**– or more precisely**

*jointly measured***, with arbitrary accuracy. What can be done is to perform**

*simultaneously**approximate joint measurements*with inaccuracies that satisfy an

*uncertainty relation*or

*inaccuracy relations “Ungenauigkeitsrelationen“,*which was Heisenberg’s favorite terminology. (iii) it is not possible to measure an observable without

*a subsequent measurement of an (incompatible) observable and*

**disturbing***vice versa*. The inaccuracy (

*error*) of the measurement of the first and the

*disturbance*of the measurement of the second observable obey an

*error-disturbance uncertainty relation*. Heisenberg illustrates this in his paper by proposing a reciprocal relation for

*mean**error**“mittlere Fehler“*and

**of a measurement using the famous –**

*disturbance**ray microscope*thought experiment: “

*At the instant when the position is determined—therefore, at the moment when the photon is scattered by the electron—the electron undergoes a discontinuous change in momentum. is change is the greater the smaller the wavelength*of

*the light employed— that is, the more exact the determination of the position*. . .”

^{1}. Heisenberg follows Einstein’s realistic view, that is, to base a new physical theory only on observable quantities (

*elements of reality*), arguing that terms like velocity or position make no sense without defining an appropriate apparatus for a measurement. By solely considering the Compton effect, named after the American physicist Arthur Holly Compton

**Heisenberg gives a rather**

*heuristic*estimate for the product of the

*of a position measurement and the*

**inaccuracy (error)***induced on the particles momentum, denoted by . This equation can be referred to as a*

**disturbance***measurement uncertainty*(i)

*or as an e*

*rror-disturbance uncertainty relation (EDR)*. Heisenberg’s original formulation can be read in modern treatment as for error of a measurement of the position observable and disturbance of the momentum observable induced by the position measurement. Just as a side node: Heisenberg himself never used the term “

*principle*” for his relations, as already stated above he referred to them as

*inaccuracy relations “Ungenauigkeitsrelationen”*or

*indeterminacy relations “Unbestimmtheitsrelationen“.*

However, most modern textbooks introduce the uncertainty relation in terms of a* preparation uncertainty (ii)* relation denoted by , originally proved by Earle Hesse Kennard ^{2} for the * standard deviations* and and of the position observable and the momentum observable in an arbitrary state , where the standard deviation is defined by . This formulation of the

*uncertainty principle*is

*uncontroversial*and has been tested with several quantum systems including neutrons. However it does not capture Heisenberg’s initial intensions: Kennard’s formulation is an inequality for statistical distributions of

**a**

*not**joint*but rather single measurements of either or . It is an

*intrinsic*uncertainty inherent to any quantum system independent whether it is measured or not. The unavoidable recoil caused by the measuring device is ignored here. The reciprocal behavior of the distributions of and is illustrated on the right side. Heisenberg actually derived Kennard’s relation, from above, for Gaussian wave functions , applied this relation to the state just after the measurement with error and disturbance , and concluded his relation from the additional, implicit assumptions and . However, his assumption holds only for a restricted class of measurements and holds if the initial state is the momentum eigenstate state, but it does

*hold generally. In 1929, Howard Percy “Bob” Robertson*

**not**^{3}extended Kennard’s relation () to an arbitrary pair of observables and as , with the

*commutator*. The corresponding generalized form of Heisenberg’s original e

*rror-disturbance uncertainty relation*would read . But the validity of this relation is known to be limited to specific circumstances.

## **Ozawa’s generalized Uncertainty Relation**

**Ozawa’s generalized Uncertainty Relation**

In the year 2003 Japanese theoretical physicist Masanao Ozawa proposed a new *error- disturbance uncertainty relation * ^{4}, and proved its universal validity in the general theory of quantum measurements (see here for details of the derivation). Here denotes the * root-mean-square* (

*r.m.s.*) error of anarbitrary measurement for an observable , is the r.m.s. disturbance on another observable induced by the measurement, and and are the standard deviations of and in the state before the measurement. Here error and disturbance are defined via an

*indirect measurement model*for an apparatus

**A**measuring an observable of an object system

**S**as and . Here is the initial state of system

**S**, which is associated with Hilbert space . is the state of the probe system

**P**before the measurement, defined on Hilbert space , and an observable , referred to as

*meter observable*of

**P**. The time evolution of the composite system

**P+S**during the measurement interaction is described by a unitary operator on . The Hilbert–Schmidt norm is used where the norm of a state vector in Hilbert space is given by the square root of its inner product: . A schematic illustration of a measurement apparatus

**A**is given aside. See here for our

*experimental*test of Ozawa’s generalized error-disturbance uncertainty relation.

### ** Tighter uncertainty relations**

**Tighter uncertainty relations**

Though *universally valid* Ozawa’s relation from above is not optimal. The reason for this is that three terms in Ozawa’s relation come from three independent uses of Robertson’s relation (see here for details) to different pairs of observables. Although this indeed leads to a valid relation, this is not optimal because the three Robertson’s relations – and consequently Ozawa’s relation – generally cannot be saturated simultaneously. Thus, Cyril Branciard ^{6 }showed that one can improve on the *sub-optimality* of Ozawa’s proof and derived the following trade-off relation between error and disturbance by applying two geometric lemmas: , where we have again . For the *special case* , which implies , and replacing and by and , respectively, the above equation can be strengthened yielding the * tight relation , *as illustrated aside in comparison with

*Heisenberg’s*and

*Ozawa’s*

*error-disturbance uncertainty relations*. Click here for our

*experimental*test of a tight error-disturbance uncertainty relation.

### ** Mixed state uncertainty relations **

**Mixed state uncertainty relations**

Aiming in of an improvement of **e**rror-**d**isturbance **u**ncertainty **r**elations (*EDUR*) a stronger inequality was proposed. Later, it was pointed out that the relation above is not stringent for mixed states in general, when the Robertson bound is simply extended to , which decreases for mixed states and vanishes for *totally mixed states*. Further improvement of the bound was put forward by Masanao Ozawa who could show that the constant can be replaced by a stronger constant defined by . This new parameter coincides with the Robertson bound when is a pure state, but makes the EDUR stronger for a mixed ensemble. Our *experimental* test for mixed state uncertainty relations is reported here.

## **Busch/Werner/Lahti’s Proof of Heisenberg’s original Error-Disturbance Relation**

**Busch/Werner/Lahti’s Proof of Heisenberg’s original Error-Disturbance Relation**

In 2013, as a result of various attempts of rigorous *reformulations* of Heisenberg’s original Error-Disturbance Relation, Paul Busch, and Pekka Lahti, and Reinhard F. Werner (BLW) provided a general, quantitative quantum version of Heisenberg’s original semiclassical uncertainty, by applying appropriate definitions of our and disturbance ^{7 }. Unlike in Ozawa’s approach, where the measurement process is described by the interaction of a quantum object with a probe, in BLW’s scheme error and disturbance are evaluated from the *difference* between *output probability distributions*, as illustrated schematically below. This is achieved by performing highly accurate single measurements, so-called *reference* or *control measurements* of the (general) target observables and in the input state , yielding probability distributions and . In a next step, using a successive measurement scheme, the observable is approximated by an observable , thereby inducing a change of the input state and thus a modification of the subsequent -measurement to be effectively a measurement of an observable on . The marginal distributions and of the *joint probability distribution* obtained from the successive measurement are then compared with the output statistics of the reference (single) measurements. Hence, the difference between and then account for the *state dependent error*, denoted as . Likewise the difference between and is the *state dependent disturbance,* which is expressed as . Both quantities are evaluated using the Wasserstein-2-distance resulting in for *error* and for *disturbance*. For the special case of position and momentum Heisenberg’s original error-disturbance relation is maintained in terms of , where and are the marginal observables of some joint measurement device. However for *qubit observables* the respective inequality is given by , where the bound accounts for the incompatibility of and ^{8 }. See here for our experimental comparison between the theoretical approaches of BWL with Ozawa’s.

## *Information-theoretic (e***ntropic) Uncertainty Relations**

**ntropic) Uncertainty Relations**

The uncertainty relation, as formulated by Robertson Relation in terms of standard deviations has two flaws, which was first recognized by Israeli-born British physicist David Deutsch in 1983 ^{9 }: i) standard deviation not optimal *measure* for all states, there exist certain states, for which the standard deviation diverges (see here for an example). ii) the boundary (right hand side of any uncertainty relation) can become zero for non-commuting observables (this is also the case for our neutron spins for a combination of and ). So Deutsch suggested to seek a theorem of linear algebra in the form . Heisenberg’s (Kaennard) inequality has that form but its generalization does not. In order to represent a quantitative physical notion of “*uncertainty*, must at least possess the following elementary property: If and only if is a simultaneous eigenstate of and may become zero. From this we can infer a property of , namely that it must vanish if and only if and have an eigenstate in common. “*The most natural measure of the uncertainty in the result of a measurement or preparation of a single discrete observable is the (Shannon) entropy* ^{9 }” (see here for a short introduction to probability theory). According to Claude Shannon entropy is the expected (*average*) information received, which consists of the so called self-*information *a.k.a.* surprisal *and its probability to occur defined as

which can be expressed in the language of quantum mechanics as

### ** Information-theoretic uncertainty relations for projective qubit measurements (dichotomic case)**

**Information-theoretic uncertainty relations for projective qubit measurements (dichotomic case)**

A *tight* ** noise-disturbance** uncertainty relation for

*projective*qubit measurements, with two possible outcames, i.e., dichotomic, including appropriate

*information-theoretic*definitions for noise and disturbance in quantum measurements were proposed in

^{10}. The procedure is the following: Randomly selected eigenstates of and , with and , are sent into a measurement apparatus , followed by a correction operation . The experimental procedure is schematically illustrated below:

From the obtained data a state independent noise-disturbance trade-off relation in terms of , with , is inferred. The predicted values are given by the blue line in the plot above (right). For maximally incompatible qubit observables, represented by the Pauli matrices and we have been able to significantly strengthen this relation to the tight relation , where denotes the inverse of the function given by . Experimentally this is achieved by applying a *correction operation* after the measurement yielding the green curve in the above diagram. See here for our *experimental* test of a tight entropic noise-disturbance uncertainty relations for *projective* qubit measurements.

### ** Information-theoretic uncertainty relations for general qubit measurements (POVM case)**

**Information-theoretic uncertainty relations for general qubit measurements (POVM case)**

A *tight information-theoretic (or entropic) uncertainty relation* for *general* qubit measurements, that is a *positive-operator valued measure (POVM),* was proposed recently by Alastair A. Abbott and Cyril Branciard in ^{11}, discussing both, entropic *noise-noise* and entropic *noise-disturbance* uncertainty relations (see here for details on POVMs). Let’s take a look at the * noise-noise *scenario first: The qubit preparation uncertainty region , for two observables and (), can be completely characterized by the

*tight*p

*reparation uncertainty relation*in terms of

*standard deviations*as . An equivalent formulation in terms of

*entropies*reads . Interestingly, the region is

*for and*

**nonconvex****for . Hence, for the above relation expresses the**

*convex**tight uncertainty relation*. For no analytic form for the convex hull of exists in general. However, for , i.e., for orthogonal Pauli measurements for instance as and , the relation can be given explicitly and we have the simple tight relation . Then an apparatus implementing the POVM , which performs a combination of these two projective measurements with probabilities and , respectively, allows for may reach any point in the region and is therefore able to saturate the boundary, which is illustrated aside for the noise of an qubit observable .

Hence, projective measurements are able to saturate the tradeoff when is ** convex**, but are suboptimal when it is not, i.e.,

*. Above on the left you can see the expected results for a*

**non-convex***noise-noise*Plot for and meaning and on the right side.

1. W. Heisenberg, *Z. Phys.* **43**, 172 (1927). ↩

2. E. H. Kennard, *Z. Phys.* **44**, 326 (1927). ↩

3. H. P. Robertson, *Phys. Rev.* **34**, 163 (1929). ↩

4. M. Ozawa, *Phys. Rev. A* **67**, 042105 (2003). ↩

6. C. Branciard, *Proc. Natl. Acad. Sci. USA* **17**, 6742-6747 (2013). ↩

7. P. Busch, P. Lahti, and R. F. Werner *Phys. Rev. Lett.* **17**, 6742-6747 (2013). ↩

8. P. Busch, P. Lahti, and R. F. Werner *Phys. Rev. A* **89**, 012129 (2014). ↩

9. D. Deutsch, *Phys. Rev. Lett.* **50**, 631 (1983). ↩

10. F. Buscemi, M. J. W. Hall, M. Ozawa, and M. M. Wilde, *Phys. Rev. A* **112**, 050401 (2014). ↩

11. A. A. Abbott and C. Branciard, *Phys. Rev. Lett.* **94**, 062110 (2016). ↩