Tuesday, 10 May 2016

Did Bergson Influence Einstein’s Nobel Prize?

 In a recent book, The Physicist & the Philosopher (Princeton University Press, 2015), and in a Nautilus post a few weeks ago, historian Jimena Canales claims that the philosopher Henri Bergson’s criticisms of relativity theory influenced the Nobel Prize committee in its deliberations regarding a prize for Einstein, and helped ensure that there would be no Nobel Prize for relativity.

Interesting, if true.  Moreover, if true, this is something that has evaded Einstein’s biographers, and so would be a major contribution to Einstein scholarship.  But I’m not convinced.

Why not? Canales’ claim is based, not on new documentary evidence previously unavailable to historians, but on a novel and idiosyncratic reinterpretation of something that has long been in the public record, the presentation speech by Svante Arrhenius, Chair of the Nobel Prize Committee.  I don’t think that the text of the speech bears out Canales’ interpretation.  Moreover, Canales’ claim is at odds with the conclusion drawn by Abraham Pais, who was permitted to examine the documents considered by the Nobel Prize committee and devoted a section of his biography of Einstein to what he found.  I will quote Pais’ conclusion below.

Background: in 1905, his “annus mirabilis,” Einstein published a number of seminal papers.  This included the classic papers on special relativity, one on Brownian motion, and one in which he introduced the hypothesis of light quanta.  From this hypothesis Einstein derived a prediction about the photoelectric effect: that there would be a linear relation between the energy of electrons released by light impinging on a metal and the frequency of the light.  This relation was confirmed in 1916 by the careful experiments of Robert Millikan.  In 1915 Einstein added the general theory of relativity to his list of accomplishments, and it was Eddington's eclipse observations of 1919, verifying a prediction of general relativity, that brought him widespread fame outside the physics community.  By 1921 it was clear that he deserved a Nobel prize, and there was an embarrassment of riches as to what to base the award on.

Honestly, I would have regarded it as a tough call. The 1905 paper on special relativity is terrific, but it's largely a (much-needed) clarification of the foundations of electrodynamics, and much of its content is foreshadowed in the work of others, notably Lorentz and Poincaré. I've recently had occasion to read through much of Einstein's work on the light quantum hypothesis (in conjunction with supervising a dissertation by Molly Kao), and I've come to appreciate how instrumental Einstein was in the development of the quantum theory.  General relativity is certainly worth a Nobel Prize, but nonetheless, I’m not sure that the Nobel Prize committee’s decision to single out the light quantum work was not the right decision.

At any rate, in 1922 Einstein was awarded the Nobel Prize for 1921 (deferred one year).  The citation said that the Prize was “for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect.”  Here's what Arrhenius says in the opening of his presentation speech.

Your Majesty, Your Royal Highnesses, Ladies and Gentlemen.

There is probably no physicist living today whose name has become so widely known as that of Albert Einstein. Most discussion centres on his theory of relativity. This pertains essentially to epistemology and has therefore been the subject of lively debate in philosophical circles. It will be no secret that the famous philosopher Bergson in Paris has challenged this theory, while other philosophers have acclaimed it wholeheartedly. The theory in question also has astrophysical implications which are being rigorously examined at the present time.

Throughout the first decade of this century the so-called Brownian movement stimulated the keenest interest. In 1905 Einstein founded a kinetic theory to account for this movement by means of which he derived the chief properties of suspensions, i.e. liquids with solid particles suspended in them. This theory, based on classical mechanics, helps to explain the behaviour of what are known as colloidal solutions, a behaviour which has been studied by Svedberg, Perrin, Zsigmondy and countless other scientists within the context of what has grown into a large branch of science, colloid chemistry.

A third group of studies, for which in particular Einstein has received the Nobel Prize, falls within the domain of the quantum theory founded by Planck in 1900. This theory asserts that radiant energy consists of individual particles, termed “quanta”, approximately in the same way as matter is made up of particles, i.e. atoms. This remarkable theory, for which Planck received the Nobel Prize for Physics in 1918, suffered from a variety of drawbacks and about the middle of the first decade of this century it reached a kind of impasse. Then Einstein came forward with his work on specific heat and the photoelectric effect ...

Compare this with Canales’ account of the presentation speech (quoting from the Nautilus post, which reproduces, close to word-for-word, the opening pages of the book):

The chairman for the Nobel Committee for Physics explained that although “most discussion centers on his theory of relativity,” it did not merit the prize. Why not? The reasons were surely varied and complex, but the culprit mentioned that evening was clear: “It will be no secret that the famous philosopher Bergson in Paris has challenged this theory.” Bergson had shown that relativity “pertains to epistemology” rather than to physics—and so it “has therefore been the subject of lively debate in philosophical circles.”

One thing leaps out: Canales attributes a role to Bergson that  Arrhenius does not. Arrhenius does not say that Bergson had shown that relativity pertains to epistemology; he says that relativity “pertains especially to epistemology” and for this reason has been a topic of discussions, pro and con, by philosophers, and he says this before mentioning Bergson. He then says that the theory has been challenged by one philosopher, Bergson, and acclaimed wholeheartedly by others.

Crucially, he does not say that Bergson’s criticisms played any role in the Prize Committee’s deliberations. Canales says that it would have been clear to the audience that Bergson was being mentioned as an explanation for why it was the photoelectric effect, rather than relativity, that was singled out for specific recognition among Einstein’s contributions to theoretical physics, but this is her interpretation, and she offers no evidence that anyone in the audience took it that way.   Canales’ claim that Bergson’s criticisms influenced the Committee’s decision is based solely on this reading of what Arrhenius said that day; this seems to me a very thin thread on which to hang such a claim.

Some light on what did influence the decision is shed in the section entitled “How Einstein got the Nobel Prize” of Pais’ biography, ‘Subtle is the Lord...’. Pais was given access to Committee Reports and letters of proposal concerning Einstein's Nobel Prize, and he reports on these documents in that section.  Pais does not report any mention of  Bergson’s critiques during the Committee’s deliberations. What do seem to have played a crucial role are reports prepared in 1921 and 1922 by Committee member Allvar Gullstrand on the status of the theory of relativity, written at the request of the Committee.  These reports, says Pais, are “highly critical of relativity.”  (Canales omits mention of these reports, though, in the book, she cites this section of Pais’ book, and quotes from his conclusion.)

Pais sums up his conclusions about why Einstein was not awarded the Nobel Prize for relativity in the final paragraphs of that section, which I quote in full.

Why did Einstein not get the Nobel prize for relativity? Largely, I believe, because the Academy was under so much pressure to award him.  The many letters sent in his behalf were never the result of any campaign. Leading physicists had recognized him for what he was. It is understandable that the Academy was in no hurry to award relativity before experimental issues were clarified, first in special relativity, later in general relativity.  It was the Academy’s bad fortune not to have anyone among its members who could competently evaluate the content of relativity theory in early years.  Oseen’s proposal to give the award for the photoeffect must have come as a relief  of conflicting pressures.

Was the photoeffect worth a Nobel prize? Without a doubt. Einstein’s paper on that subject was the first application of quantum theory to systems other than pure radiation. That paper showed true genius. The order of awards for quantum physics was perfect: first Planck, then Einstein, then Bohr. It is a touching twist of history that the Committee, conservative by inclination, would honor Einstein for the most revolutionary contribution he ever made to physics.

Saturday, 12 December 2015

Decision problems in continuous spaces: a follow-up

Follow-up to Thursday's post, clarifying what the issue is, as I now have a better understanding of what Cubitt et al. achieved.

Here's the tl;dr version:   The question addressed is by Cubitt et al is, in their words, "Given a quantum many-body Hamiltonian, is the system to be described gapped or gapless?"  They show that, in a very strong sense, the problem is undecidable.  My claim is that this is much more than is needed to demonstrate undecidability in the sense relevant to decision problems in physics, and that, in the sense relevant to  physics, undecidability is generic. [Edited 12-13-15]



Question: what should be meant by a decision problem of this sort?

When it comes to decision problems regarding sets of integers, there's no issue.  Thanks to Church, Turing, and Post, we have a well-agreed upon definition of computable function on the natural numbers, and of decidable subset of the natural numbers: a  subset A of the natural numbers is decidable if and only if it is recursive, that is, if and only if there is a computable function f such that f(n) is equal to 1 if nA, and 0 otherwise.

But the question posed isn't one of classifying integers, it's one of classifying Hamiltonians.  Given a Hilbert space, there are uncountably many Hermitian operators on the space, and so we can't code up the full decision problem in natural numbers that we can feed into a Turing machine.

What Cubitt at al. do is to construct a family of Hamiltonians that depend on a real parameter φ, such that the system is gapped for some values of  φ, and gapless for others.  Clearly, if this restricted problem is undecidable, then the general problem is.

So, let's think about decision problems on the reals.  How should we think of the question of whether a given subset A of the reals is algorithmically decidable?

I can think of a few ways to do this.

  1. There is a widely accepted notion of a computable function on the reals.  We could adopt that, and ask whether there is a computable function f such that f(x) is equal to 1 if x is in A, and 0 if not.
  2. Alternatively, one could restrict the problem to the computable reals.  There are only countably many of those, and they can be indexed by the code-numbers of the Turing machines that compute them.  We could ask whether there is a computable function f such that f(n) is equal to 1 if n is the index of a Turing machine that computes a real number x that is in A, and equal to 0 if n is the index of a Turing machine that computes a real number x that is not in A.  We don't care what it does when n is not the index of a machine that computes a number; it can fail to halt, for all we care.
  3. One could restrict the problem to rationals.  We can index the rationals by natural numbers, and we can ask whether there is a computable function  f such that f(n) is equal to 1 if n is the index of a rational number in A, and equal to 0 if it's not.
 In effect, Cubitt et al. showed that the problem they posed is undecidable in sense 3.  And that's by far the hardest question of the three, and doing so took a lot of work.

Clearly, if a problem is undecidable in sense 3, it's undecidable.  But I want to claim that sense 1, which is far weaker, is really the relevant sense.  This is, perhaps, disappointing, because it makes the question of decision problems on the reals into a boring one.

First: what is a computable function on the reals? The standard answer, known as Grzegorczyk computability, is reminiscent of floating point computation.  A program that computes a real function works with rationals as approximations to inputs and outputs.  Suppose you want the program to compute the value of f(x) within a certain rational degree of precision ε. You provide the program with ε, and with rational approximations to the input x.  The program is allowed to request closer and closer approximations to the input, which you are obliged to provide, but it has to halt and yield an approximation, within ε, to f(x), after finitely many steps.

This is, I think, the notion of computable function relevant to decision problems in physics.    If you are asked to decide whether a given physical system, characterized by certain parameters, is in one class or another, you can ask the experimentalists to provide you with values of the parameters, but they will only be able to yield approximations within experimental error.  You might ask them for better and better information about the relevant parameters, but, if you are to render a decision, you have to do so with only an approximation to the input parameter.

It's easy to see that, on this notion of a computable function on the reals, all computable functions are continuous.   Which means that, in sense 1, there are no non-boring decision problems.

This strikes some people as counter-intuitive.  But it is, I claim, the right answer.

Here's why.  Recall that a sequence {xn} of real numbers is a computable sequence if and only if there is a computable function that yields rational approximations, within 2-m, to xn, as a function of n and m.  I claim that
  • a necessary condition for a function f on the reals to be a computable function is that it map computable sequences onto computable sequences, and 
  •  a necessary condition for a set A of reals to be decidable is that, for every computable sequence {xn}, the sequence {χA(xn)}is a computable sequence of 1s and 0s, where χA is the characteristic function of A.
Before reading on, taking a moment to ask yourself whether you agree.


If you do agree that these are necessary conditions on the relevant notions, they have far-reaching consequences.  Mazur (1963, Th. 4.28) proved the following (see also Weihrauch 2000, Th. 9.1.2).
  • If is a real-valued  function on the reals that maps computable sequences to computable sequences, then, if {ak}is a computable sequence that converges to a computable limit a, the sequence {f(ak)} converges to f(a).
Suppose, now, that you accept what I suggested, above, should be taken to be a necessary condition for a subset of the reals to be decidable.  Then this means that equality is undecidable.  Deciding whether a real number is in the singleton set {0} is an undecidable problem.  Similarly for simple subsets of the reals; the interval [0, 1] is undecidable.

  What people who work in computable analysis do, in light of this, is to replace questions of deciding membership in a set of reals with other questions.  We can, for example, ask whether, for a given set A, there is a computable function is equal to 1 in the interior of A, equal to 0 in the exterior, and is undefined on its boundary.  Or we can ask whether the distance function dA(x), defined as the greatest lower bound of |xy| for yA, is a a computable function.  See Weihrauch 2000, Chs 4 & 5 for more on this sort of thing.

It seems to me that, given a fixed Hilbert space, one ought to be able to extend notions like these to subsets of the set of all Hermitian operators on the space.  It would be interesting to see how the spectral gap problem looks from that point of view.


 References

Cubitt, Toby S., David Perez-Garcia, & Michael M. Wolf, “Undecidability of the spectral gap” Nature 528 (10 December 2015), 207–211.

Mazur, S. (1963). Computable Analysis. Rozprawy Matematyczne 33, 1-111.

Weihrauch, Klaus (2000). Computable Analysis. Springer.

Thursday, 10 December 2015

Generic Undecidability of Decision Problems in a Continuous Space: Is undecidability of the spectral gap surprising?

An article by Toby S. Cubitt, David Perez-Garcia, and Michael M. Wolf, “Undecidability of the Spectral Gap,” published today in Nature, has been receiving some attention (at least as judged by the number of my facebook friends who have shared or commented on it!)  It’s been called “genuinely shocking, and probably a big surprise for almost everybody working on condensed-matter theory” (Christian Gogolin, quoted by Castelvecchi).


I don’t mean to rain on anyone’s parade, but I wonder whether it should be regarded as surprising.  It seems to me that the result follows from something that is well-known in the field of computable analysis: undecidability of equality of real numbers.

Turing machines operate on integer inputs; to deal with real numbers, we use rational approximations.  Since there are countably many rationals, we can index them by natural numbers; pick your favourite enumeration, and let qk be the rational number indexed by k.  A real number x is computable if and only if there is an algorithm that delivers rational approximations to x, as a function of desired degree of accuracy; that is, if there is an algorithm that delivers k(m) as a function of m, such that the distance between x and qk(m) is always less than 2m.   A sequence of numbers {xn}  is a computable sequence if and only if there is an algorithm that delivers a rational number that is within a distance 2m of xn, as a function of n and m.

Now, if I hand you an algorithm for computing a number x (or an oracle that delivers rational approximations to any desired degree of precision), can you decide whether or not the number is equal to 0?

If the number is not equal to 0, then knowing a sufficiently precise rational approximation to the number will tell you that.  But if you keep computing closer and closer rational approximations and don’t find the number bounded away from zero, then you don’t know whether the number is zero, or whether a closer rational approximation will bound it away from zero.  You don’t know when to stop.

This should sound familiar, as it is reminiscent of the Halting Problem.  And, in fact, it is easy to show that the undecidability of equality is equivalent to the Halting Problem.

Given a Universal Turing machine T,  it is easy to construct a computable sequence {xn} such that xn is greater than zero if T halts on input n and is equal to zero if it doesn’t  (see my 1995 and 1997).  So, if we could effectively decide which members of the computable sequence {xn} are equal to zero, we could solve the halting problem.

This means that, if we have any decision problem that asks whether a given quantity that is a calculable function of real-valued input parameters is equal to zero or not, it’s an undecidable problem.  All computable functions on the reals are continuous!  (Weihrauch 2000, Th. 4.3.1)

This is why I’m not surprised by the Cubitt et al. result.

The result concerns 2-dimensional L×L  lattices of spins, with nearest-neighbour interactions.  The system is gapped if there is a number γ such that, for sufficiently large L, the difference between the energy of the ground state and the energies of all excited states is at least γ.  The system is gapless if, in the thermodynamic limit, it has continuous spectrum above the ground state.  The authors construct a family of interaction Hamiltonians h(φ), depending on an input parameter φ, such that whether or not the spectrum is gapped depends on the value of φ, and they rig things so that there is a computable sequence of numbers {φ(n)} such that whether or not the system with interaction Hamiltonian h(φ(n)) is gapped or gapless depends on whether or not a Universal Turing machine halts on input n.

If all that is needed to show that the problem is undecidable is to construct a family of Hamiltonians, depending on input parameter φ , such that there is a computable sequence {φn } of input parameters such that the system is gapped if a Universal Turing Machine halts on input n and gapless if it doesn’t, then I can’t help but wonder whether it could be done more simply.
Suppose we construct interactions h(λ) such that whether the system is gapped or gapless depends on whether the input parameter λ is greater than zero. Then, without further ado, there is, as mentioned above, a computable sequence {λn} of input parameters such that the system is gapped if a Universal Turing Machine halts on input n and gapless if it doesn’t, and we can conclude that the problem is not effectively decidable as a function of the input parameter.


References


Castevecchi, Davide (2015), “Paradox at the heart of mathematics makes physics problem unanswerable.”  Nature News, 9 December 2015, http://www.nature.com/news/paradox-at-the-heart-of-mathematics-makes-physics-problem-unanswerable-1.18983.

Cubitt,  Toby S., David Perez-Garcia, & Michael M. Wolf, “Undecidability of the spectral gap” Nature 528 (10 December 2015), 207–211.

Myrvold, Wayne C. (1995). “Computability in Quantum Mechanics,” in Werner DePauli-Schimanovich, Eckehart Köhler, and Friedrich Stadler, eds., The Foundational Debate: Complexity and Constructivity in Mathematics and Physics (Kluwer Academic Publishers, 1995), pp. 33–46.   Available at http://philpapers.org/rec/MYRCIQ

——— (1997). “The Decision Problem for Entanglement.”  In Robert S. Cohen, Michael Horne & John Stachel (eds.), Potentiality, Entanglement, and Passion-at-a-Distance: Quantum Mechanical Studies for Abner Shimony. (Kluwer Academic Publishers), pp. 177–190.  Available at http://philpapers.org/rec/MYRTDP

Weihrauch, Klaus (2000).  Computable Analysis: An Introduction. Springer.

Tuesday, 27 October 2015

Public Library Talk: Einstein and the Atom

I'm giving a talk tomorrow (Wednesday, October 28), at the Central Branch of the London Public Library, (251 Dundas Street), 7 PM, Stevenson & Hunt Room.   The talk will be non-technical, and accessible to all.  Please join me, if you can!



Einstein and the Atom.
 Abstract:
Einstein’s name is widely associated with the “atom bomb,” via the formula E = mc2. Less widely known is that he played a key role in providing evidence that atoms exist at all. One of Einstein’s early papers was an analysis of Brownian motion, the ceaseless dance of tiny particles, such as pollen grains, suspended in a fluid. The dance of pollen grains, Einstein realized, was evidence that they are being buffeted by smaller particles, beyond microscopic resolution. This talk will be about the ingenuity required to turn the visible into evidence about the invisible.




Friday, 23 October 2015

Was Einstein Wrong?

Some headlines from the past day or so:
This sort of thing is nothing new, of course.  Many  discussions of Einstein's attitude towards quantum mechanics suggest that Einstein simply refused to accept a straightforward consequence of quantum mechanics: non-locality.

Now, if you have no reason to believe something, and you don’t believe it, but it happens to be true, then, in one sense, you’re wrong in your belief But you can’t be accused of being unreasonable or irrational.  So, in an uninteresting sense, Einstein was wrong, in not having beliefs that scientists would later provide good evidence for.  But the same could be said of everybody, ever.

Einstein didn’t believe that nonlocality was a feature of the world. But should he have? Was he wrong not to believe in nonlocality?  What reason did anyone have, in 1935, or in the late ‘40s, when he wrote his fullest discussions of his attitude towards quantum mechanics, for thinking that nonlocality was a feature of physical reality?

We can’t fault Einstein for not having read Bell’s 1964 paper, or for not having read the December 20, 1982 issue of Physical Review Letters—after all, he was no longer alive by the time Doc Brown and Marty McFly arrived in 1955, and, besides, as far as we know, they didn’t bring literature of that sort with them. We can't fault him, either, for not having read this week's issue of Nature.  Hindsight is 20-20, and we now know two things that, as far as I know, nobody really knew during Einstein’s lifetime.
  1. Some quantum correlations are not locally explicable.
  2. Quantum correlations persist when the systems are separated by a large distance.
The first, of course, is Bell's theorem, and the second we know through a series of increasingly impressive experimental demonstrations of violations of Bell inequalities.  Re 1:  As Bell himself emphasized, the mere fact that outcomes of spatially separated experiments are correlated is no indication of any sort of nonlocality.  As you're reading this, someone else on the other side of the world might be reading the same words.  No spooky action-at-a-distance is needed to explain this; nor is there any need for direct influence between the two of you, as there's a common source for what's displayed on your computer screen, and what is being displayed on the other side of the world.
 
As I’ve emphasized in earlier blog posts (here and here),  Einstein was not nearly as dogmatic about locality as he is sometimes painted to be.  He did not regard the assumptions of locality and separability as non-negotiable; his attitude was that one could, indeed, drop them as requirements on a physical theory, given good reason.  But he saw no reason to do so.  He wrote, in 1948,

if I consider the physical phenomena with which I am acquainted, and especially those which are so successfully comprehended by means of quantum-mechanics, then, nevertheless, I nowhere find a fact which makes it appear to me probable that one has to give up requirement II [of locality and separability]. For that reason I am inclined to believe that the description afforded by quantum-mechanics is to be viewed … as an incomplete and indirect description of reality, that will again be replaced later by a complete and direct description (Einstein 1948; translation in Howard 1985).

Systems that are interacting or have interacted, and whose quantum-mechanical state is entangled, have probabilistically correlated behaviour.  That by itself isn’t enough to answer Einstein’s challenge to point to a phenomenon that would count as evidence for a breakdown of locality. Correlations are already familiar in classical probability theory: for example, if two classical  systems interact, a probability distribution that represents thermal equilibrium will involve correlations between the two.  An answer to Einstein’s challenge would have to give us some reason to think that quantum correlations aren’t like that.

My question for historians: did anyone even attempt to provide an argument of that kind, during Einstein’s lifetime?


References


Aspect, A., J. Dalibard, and G. Roger (1982). Experimental test of Bell’s inequalities using time-varying analyzers. Physical Review Letters 49, 1804-1807.

Bell, John S.,  (1964). On the Einstein-Podolsky-Rosen Paradox. Physics 1, 195-200.

Einstein, Albert (1948). Quanten-mechanik und wirklichkeit. Dialectica 2, 320–324.

Hensen, B. et al. (2015).  Loophole-free Bell inequality violation using electron spinsseparated by 1.3 kilometres. Nature, online 21 October 2015.

Howard, Don (1985). “Einstein on Locality and Separability.” Studies in History and Philosophy of Science 16, 171-201.

Friday, 16 October 2015

Bohr's reply to EPR (Part III)



Did Bohr find a flaw in the EPR argument?

He says he did.  In a brief note (Bohr 1935a) published soon after the publication of the EPR paper, in his fuller reply to EPR (1935b), and in his later (1949) recap of his discussions with Einstein about QM, Bohr claims to have discovered an ambiguity in the EPR reality criterion.

The EPR reality criterion reads:

If, without in any way disturbing a system, we can predict with certainty (i.e. with probability equal to unity) the value of a physical quantity, then there exists an element of physical reality corresponding to this physical quantity (EPR 1935, p. 777).

Here’s what Bohr says about the alleged ambiguity:

the wording of the above-mentioned criterion of physical reality proposed by Einstein, Podolsky and Rosen contains an ambiguity as regards the expression “without in any way disturbing a system.” Of course there is in a case like that just considered no question of a mechanical disturbance of the system under investigation during the last critical stage of the measuring procedure. But even at this stage there is essentially the question of an influence on the very conditions which define the possible types of predictions regarding the future behavior of the system.  Since these conditions constitute an inherent element of the description of any phenomenon to which the term “physical reality” can be properly attached, we see that the argumentation of the mentioned authors does not justify their conclusion that quantum-mechanical description is essentially incomplete (Bohr 1935b, p. 700; 1949, p. 324).

EPR consider two systems that interact for a while, and then, after a certain time, no longer interact.  On the basis of this absence of interaction, they conclude that what is done to the first system produces no change in the state of the second system.  According to Bohr, this is ambiguous between two readings.


  1. They could mean that an experiment performed on the first system produces no mechanical disturbance of the other.
  2. On the other hand, they could mean that an experiment performed on the first system has no effect on the types of predictions that can be made about the other.

I submit that there is no ambiguity, because (2) is not a possible reading of what EPR meant.  Of course the choice of experiment done on one particle has an effect on the sorts of predictions that can be made about the other; that’s the whole point of the argument!  And EPR do note that, since the choices are mutually exclusive, to make a choice means losing the opportunity to make the other sort of prediction about the other particle:

one would not arrive at our conclusion if one insisted that two or more physical quantities can be regarded as simultaneous elements of reality only when they can be simultaneously measured or predicted. On this point of' view, since either one or the other, but not both simultaneously, of the quantities P and Q can be predicted, they are not simultaneously real (p. 780).

Bohr says that that the conditions that define the possible types of prediction that can be made about a system constitute an inherent element of the description of any phenomenon to which the term “physical reality” can be properly attached.  This sounds to me as if he saying that being able to predict the outcome of a position “measurement” is a condition for applying the concept of position, and being able to predict the outcome a momentum “measurement” is a condition for applying the concept of momentum. But, if that’s what he’s saying, he’s simply taking the out that EPR offer at the end of their paper.  They note that this way out has the consequence that the reality of properties of one system depends on what is done to the other.  If that is, indeed, what Bohr is saying, then one wishes he had said so straightforwardly!


References

Bohr, Niels (1935a).  Quantum Mechanics and Physical Reality. Nature 136, 65.

——— (1935b). Can Quantum-Mechanical Description of Physical Reality Be Considered Complete? Physical Review 48, 696-702.

——— (1949).  Discussions with Einstein on Epistemological Problems in Atomic Physics, in P.A. Schilpp, ed., Albert Einstein: Philosopher-Scientist (Chicago: Open Court Press), 199–241.

Einstein, Albert, Boris Podolsky, and Nathan Rosen (1935), Can Quantum-Mechanical Description of Physical Reality Be Considered Complete? Physical Review 47, 777-780.