REVIEW
Becoming classical: A possible influence on the quantum-to-classical transition
General Physics · Submitted 23 Feb 2006 · 1 reference
Pith's verdict: A clean dimensional analysis built on a category error: Hubble-flow velocity spread is not a quantum uncertainty, so the 0.1 mm threshold has no physical basis.
T0 · AI review
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Referee report
The paper
The paper claims
The paper claims that cosmic expansion sets a fundamental quantum-classical boundary at about 0.1 millimeter (roughly a microgram of mass), above which whole objects must behave classically.
The reading
What carries the argument
The load-bearing device is the substitution of the Hubble-flow velocity spread for a quantum velocity uncertainty. The identity $\Delta v \approx H_0 L$, where $H_0$ is the Hubble constant and $L$ the object's size, is combined with the Heisenberg inequality through $\Delta p = m\Delta v$; imposing $\Delta x \approx L$ then produces the threshold formula $L_{\rm cr} \approx [h/(4\pi\rho H_0)]^{1/5}$. This one formula turns a very small classical expansion rate into a macroscopic cutoff near 0.1 millimeter.
Extended reading notes
Core claim
The central claim is that cosmic expansion itself supplies the dividing line between quantum and classical behavior. For an object of size $L$ and density $\rho$, the spread of recessional velocities across the object is $\Delta v \approx H_0 L$; multiplying by the mass turns this into a momentum uncertainty $\Delta p \approx m H_0 L$. The Heisenberg relation then implies a position uncertainty $\Delta x \approx h/(4\pi m H_0 L)$, and setting $\Delta x = L$ gives a critical size $L_{\rm cr} \approx [h/(4\pi\rho H_0)]^{1/5}$. With $\rho \approx 1\,\mathrm{g/cm^3}$ and $H_0 \approx 2.3\times 10^{-18}\,\mathrm{s^{-1}}$, this is about 0.1 millimeter, so objects larger than that (or more massive than about a microgram) are predicted to behave classically as whole objects.
Load-bearing premise
The whole derivation rests on treating the Hubble-flow spread across a bound object as a genuine quantum uncertainty in velocity, when cosmic expansion is a coherent classical motion and bound objects do not actually recede from themselves.
Editorial extensions
If this is right
- If the claim is correct, objects larger than roughly 0.1 millimeter (or heavier than about a microgram) at ordinary density should show classical center-of-mass behavior even in the absence of environmental decoherence.
- The mechanism depends only on density and the Hubble constant, so it would apply universally to any extended body regardless of composition.
- Below the threshold, quantum behavior of an entire object is not excluded by this effect, so the proposal is a size-and-mass cutoff rather than a sharp universal law.
- The threshold does not conflict with observed quantum behavior of molecules, which are far smaller than 0.1 millimeter.
- For objects above the threshold, quantum effects would be expected only among internal constituents, not for the object's motion as a whole.
Reading between the lines
- If the argument were correct, a concrete testable consequence is that center-of-mass interference experiments on objects approaching the microgram scale should encounter a fundamental classical floor; current levitated-interference experiments are moving toward that scale.
- A natural extension the paper does not develop is the density scaling: because the threshold scales as $\rho^{-1/5}$, changing the density by a factor of 1000 shifts the cutoff by only a factor of about 4, which could serve as a distinctive signature across materials.
- The same Hubble-flow logic, applied to internal coordinates, would suggest a universal coherence length in matter that is independent of temperature, an effect distinct from ordinary thermal decoherence.
Original abstract
Although cosmic expansion at very small distances is usually dismissed as entirely inconsequential, it appears that these extraordinarily small effects may in fact have a real and significant influence on our world. Calculations suggest that the minute recessional velocities associated with regions encompassed by extended bodies may have a role in creating the distinction between quantum and classical behavior. Using an uncertainty in position estimated from the spread in velocities associated with its size, the criterion that the uncertainty in position should be smaller than the extension of the object leads to a threshold size that could provide a fundamental limit distinguishing the realm of objects governed by classical laws from those governed by quantum mechanics.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
Although cosmic expansion at very small distances is usually dismissed as entirely inconsequential, it appears that these extraordinarily small effects may in fact have a real and significant influence on our world. Calculations suggest that the minute recessional velocities associated with regions encompassed by extended bodies may have a role in creating the distinction between quantum and classical behavior. Using an uncertainty in position estimated from the spread in velocities associated with its size, the criterion that the uncertainty in position should be smaller than the extension of the object leads to a threshold size that could provide a fundamental limit distinguishing the realm of objects governed by classical laws from those governed by quantum mechanics.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Although cosmic expansion at very small distances is usually dismissed as entirely inconsequential, it appears that these extraordinarily small effects may in fact have a real and significant influence on our world. | background 0.88 | 0.11 | 0.18 | hedged possibility 1.00 |
| s1 | Calculations suggest that the minute recessional velocities associated with regions encompassed by extended bodies may have a role in creating the distinction between quantum and classical behavior. | result 0.40 | 0.50 | 0.60 | hedged possibility 1.00 |
| s2 | Using an uncertainty in position estimated from the spread in velocities associated with its size, the criterion that the uncertainty in position should be smaller than the extension of the object leads to a threshold size that could provide a fundamental limit distinguishing the realm of objects governed by classical laws from those governed by quantum mechanics. | result 0.51 | 0.77 | 0.68 | hedged possibility 0.99 |
What was examined, and what was not
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References
How the literature uses it
Papers whose main result relates to this one's
States the same result 1 paper
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A calculation suggests that the minute recessional velocities associated with regions encompassed by extended bodies may have a role in creating the distinction between quantum and classical behavior.
A possible cosmological effect on the quantum-to-classical transition · 1.00
Discussion
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