Testing Time-Adjacency as a Basis for Entanglement Correlations
Posted: Thu Aug 21, 2025 7:40 pm
I recall an ISUS Journal issue suggesting that time-adjacent-unit coupling might provide an alternative explanation for quantum entanglement. That got me wondering: could the consequences of that idea actually be tested in the lab?
I’m not a quantum optics specialist, but I’ve drafted a short paper describing how such a test might be carried out with fairly standard tools — an SPDC source, a variable optical delay line, and coincidence counting. The key idea is to look for a finite “Frame Width of Coupling” (FWC) in the coincidence histogram, which would show up as sharp correlation boundaries, rather than assuming the correlations are strictly unbounded.
To my knowledge, no published experiments have explicitly searched for such a finite coupling width beyond detector resolution effects — but if I’ve overlooked one, I’d be glad to know. I’d also greatly appreciate feedback from those with experience in experimental quantum optics, particularly on feasibility, possible refinements, or related prior work.
For those familiar with the Reciprocal System of theory (RST), this proposal can be interpreted as a direct test of whether “entanglement” is simply the observational signature of time-adjacent motion. In RST, photons are scalar units of motion with vibration in one sector (space or time) and rotation in the reciprocal sector. Normally, correlations between photons are understood spatially, but RST extends this to the temporal domain: two photons may be “adjacent” in three-dimensional time, even while spatially separated. Such adjacency in time imposes a coupling condition, because their scalar motions share a contiguous orientation at the temporal zero point. When projected into our spatial reference system, this coupling manifests as entanglement-like correlations.
The key point is that time adjacency is not “clock time” but the structural ordering of unit scalar motions in the temporal sector. This adjacency has a finite width, arising from the quantized nature of scalar displacements. Thus, while quantum mechanics assumes that entanglement correlations are unbounded, RST predicts that correlations should fall within a measurable “Frame Width of Coupling” (FWC). This FWC reflects the interval over which coupled temporal displacements remain contiguous, after which correlations degrade. In practice, the experiment would not attempt to alter this coupling — which is a fixed property of scalar motion — but would measure its projection into spatial coincidence timing. A finite boundary in the coincidence histogram would therefore be evidence of time-adjacent coupling as the underlying mechanism, providing a physically constructive explanation for entanglement that avoids the invocation of nonlocal causation.
Link: Experimental Proposal: Testing Frame Width of Coupling in Entangled Photon Correlations (This work is shared anonymously to allow community replication and evaluation without reputational or institutional bias. It introduces no new physical postulates and relies solely on established quantum-optical formalism.)
Follow-up Idea: What Sets the Width of the Coupling Window?
If the first Hong–Ou–Mandel (HOM) experiment shows a finite temporal window in the dip (a flat region instead of a perfectly smooth curve), the natural next step is to ask:
What actually determines the size of that window?
There are two simple, general directions to explore.
1) Does the width depend on how the source is built?
The first question is whether the coupling window is just a detail of the specific SPDC setup, or something more robust.
In a follow-up, you could repeat the same HOM measurement while changing basic source parameters, for example:
If the width stays roughly the same under those changes, it starts to look like a more intrinsic feature of the biphoton state, not just a quirk of one particular crystal+filter combination.
In short, this step asks:
“Is the finite window tied to this specific setup, or is it geometry-independent?”
2) Does the width depend on photon energy?
The next high-level question is whether the window size changes with photon frequency.
The idea here is to repeat the HOM measurement at different wavelengths (for example infrared, visible, and near-UV), using comparable conditions in each case, and then compare the extracted coupling widths.
Possible outcomes include:
“Does the width scale with photon energy, or does it look like a fixed timescale?”
Overall goal
These two follow-up directions—changing the source geometry and changing the photon wavelength—are enough to give a general answer to:
I’m not a quantum optics specialist, but I’ve drafted a short paper describing how such a test might be carried out with fairly standard tools — an SPDC source, a variable optical delay line, and coincidence counting. The key idea is to look for a finite “Frame Width of Coupling” (FWC) in the coincidence histogram, which would show up as sharp correlation boundaries, rather than assuming the correlations are strictly unbounded.
To my knowledge, no published experiments have explicitly searched for such a finite coupling width beyond detector resolution effects — but if I’ve overlooked one, I’d be glad to know. I’d also greatly appreciate feedback from those with experience in experimental quantum optics, particularly on feasibility, possible refinements, or related prior work.
For those familiar with the Reciprocal System of theory (RST), this proposal can be interpreted as a direct test of whether “entanglement” is simply the observational signature of time-adjacent motion. In RST, photons are scalar units of motion with vibration in one sector (space or time) and rotation in the reciprocal sector. Normally, correlations between photons are understood spatially, but RST extends this to the temporal domain: two photons may be “adjacent” in three-dimensional time, even while spatially separated. Such adjacency in time imposes a coupling condition, because their scalar motions share a contiguous orientation at the temporal zero point. When projected into our spatial reference system, this coupling manifests as entanglement-like correlations.
The key point is that time adjacency is not “clock time” but the structural ordering of unit scalar motions in the temporal sector. This adjacency has a finite width, arising from the quantized nature of scalar displacements. Thus, while quantum mechanics assumes that entanglement correlations are unbounded, RST predicts that correlations should fall within a measurable “Frame Width of Coupling” (FWC). This FWC reflects the interval over which coupled temporal displacements remain contiguous, after which correlations degrade. In practice, the experiment would not attempt to alter this coupling — which is a fixed property of scalar motion — but would measure its projection into spatial coincidence timing. A finite boundary in the coincidence histogram would therefore be evidence of time-adjacent coupling as the underlying mechanism, providing a physically constructive explanation for entanglement that avoids the invocation of nonlocal causation.
Link: Experimental Proposal: Testing Frame Width of Coupling in Entangled Photon Correlations (This work is shared anonymously to allow community replication and evaluation without reputational or institutional bias. It introduces no new physical postulates and relies solely on established quantum-optical formalism.)
Follow-up Idea: What Sets the Width of the Coupling Window?
If the first Hong–Ou–Mandel (HOM) experiment shows a finite temporal window in the dip (a flat region instead of a perfectly smooth curve), the natural next step is to ask:
What actually determines the size of that window?
There are two simple, general directions to explore.
1) Does the width depend on how the source is built?
The first question is whether the coupling window is just a detail of the specific SPDC setup, or something more robust.
In a follow-up, you could repeat the same HOM measurement while changing basic source parameters, for example:
- type-I vs type-II phase matching
- crystal length
- pump bandwidth or chirp
- filter bandwidth
If the width stays roughly the same under those changes, it starts to look like a more intrinsic feature of the biphoton state, not just a quirk of one particular crystal+filter combination.
In short, this step asks:
“Is the finite window tied to this specific setup, or is it geometry-independent?”
2) Does the width depend on photon energy?
The next high-level question is whether the window size changes with photon frequency.
The idea here is to repeat the HOM measurement at different wavelengths (for example infrared, visible, and near-UV), using comparable conditions in each case, and then compare the extracted coupling widths.
Possible outcomes include:
- the window gets smaller at higher photon frequencies
- the window stays about the same at all wavelengths
- the window mainly changes when filtering or dispersion changes
“Does the width scale with photon energy, or does it look like a fixed timescale?”
Overall goal
These two follow-up directions—changing the source geometry and changing the photon wavelength—are enough to give a general answer to:
- whether the finite temporal window is just another optical coherence effect,
- or whether it behaves like a more stable, geometry-invariant feature,
- and whether it shows any simple scaling with photon energy.