At a glance
This sim zooms from the size of the Earth down to below a quark and shows, at each size d, the smallest probe energy Emin it assigns to that size. Every instrument, from the eye to the Large Hadron Collider, is chosen by how small a detail it must resolve.
What you'll learn
- How the probe wave in the stage relates to the size d you want to resolve.
- How a probe's momentum and energy depend on its wavelength.
- How Emin changes as d runs through 27 decades of size.
- Which kinds of instrument the sim assigns to which sizes.
What's on screen
- Probe wave (coloured wave): five periods across the view. Its colour follows the probe type.
- Target (centre): an object of size d, one fifth of the stage wide, with its name and size on a pill beneath.
- Pills (top): d on the left, and "min. probe: …" with a colour dot on the right.
- Ruler band (bottom): the size ruler with its coloured technology strip, and the probe-energy ruler.
- Cursor (accent diamond): the current d, drawn on both rulers at once.
The controls
Press ⌖ on a row to see where that control sits in the sim.
| Control | What it changes | Range | |
|---|---|---|---|
| Size to resolve, d | The size of the detail you want to see. The stage re-zooms so the target stays one fifth of its width. The slider is logarithmic. | 10⁻¹⁹ m–10⁸ m opens at 1.7 m | |
| Min. probe energy, Emin | A second handle on the same cursor: moving it also moves d. Logarithmic. | feV–TeV opens at 116 neV | |
| ◀ bigger · smaller ▶ | Jump to the next labelled object on the size ruler, so the steps are uneven. | buttons | |
| Ruler band | Drag along the ruler band under the stage to set d directly. | drag | |
| At this scale | The imaging technology the sim assigns to the current d, with the colour key of the ruler strip. It opens when you click its header, and appears once the guided inquiry is finished. | panel | |
| ▶ Play / ⏸ Pause | Runs or freezes the moving wave. In Free exploration the sim first sweeps once from the smallest size to the largest, and any move of yours ends the sweep. | top bar | |
| Speed | How fast the wave moves and how fast the zoom travels when the sim moves the cursor for you. The numbers do not change. | 0.25×–4× opens at 0.25× | |
| ↻ Reset | Restarts the scene and puts d back at the starting size of the active step: 1.7 m on the first two inquiry cards. | top bar |
Fixed: the probe is treated as massless, like a photon, and energies are quoted in the target's rest frame. The sim's technology bands are its own markers, not a model of forces.
Detail finer than the wave is lost
A wave can only report features about as big as its own wavelength or bigger. The sim turns this into a rule of thumb: the wave must wiggle at least once across the target.
- The probe wave in the stage is drawn with period ƛ = λ/2π, the reduced wavelength. The true wavelength λ is 2π ≈ 6.3 times longer.
- The sim's rule is ƛ ≲ d. It is an order-of-magnitude criterion, not a sharp cut-off.
- When ƛ is far larger than d, the wave is nearly uniform across the target and cannot tell it from a point.
- A better lens does not change this. A lens focuses and magnifies the wave, but it cannot bring back detail the wave never carried.
A shorter wave carries more momentum
The reduced wavelength is tied to momentum by ƛ = λ/2π = ħ/p. Putting this into the rule ƛ ≲ d gives a floor on the probe's momentum:
A massless probe, like a photon, has E = pc. The floor on momentum becomes a floor on energy:
- The constant is ħc = 0.19733 GeV·fm, which is also 197.33 eV·nm.
- Worked example, d = 1 nm: Emin = 197.33 eV·nm ÷ 1 nm = 197 eV. In the sim this is an X-ray.
- This Emin is a minimum. Any probe with this momentum or more can resolve d.
Size and energy move decade for decade
Because Emin = ħc/d, the product of the two is a constant. Divide d by any factor and Emin is multiplied by that same factor:
- On the rulers, one decade of size lines up with one decade of energy. The 27 decades of d on the size ruler cover 27 decades of Emin, about 2 feV to 2 TeV.
- From the opening size, d = 1.7 m gives 116 neV. A target 1000 times smaller, 1.7 mm, needs 1000 times more: 116 µeV.
These sliders move the sim too.
The minimum energy is a floor, not a beam energy
Emin is the momentum the probe must deliver, written as an energy through E = pc. The sim quotes it as a momentum transfer in the target's rest frame, not as the energy of a beam.
- A probe with mass m and the same p has kinetic energy K = √((pc)² + (mc²)²) − mc², which is (pc)²/2mc² when pc ≪ mc².
- At d = 1 nm, pc = 197.3 eV. A photon needs 197 eV. An electron with the same momentum has K = 38 meV, about 5000 times less.
- It is also a floor in another sense. Real lenses resolve about λ/2 = πƛ, roughly 3ƛ, so a working instrument needs more than the sim's minimum.
Where each technology takes over
The coloured strip on the size ruler marks which family of instruments the sim assigns to each size. Each edge is the sim's own marker.
- Naked eye to about 70 µm, a hair's width. Visible light is not the limit here; the eye's own optics are.
- Light microscope to about 105 nm, where Emin = 1.88 eV lies inside the visible range, 1.65–3.27 eV. Real optical microscopes reach about 200 nm.
- Electron microscope to about 40 pm, where Emin = 4.9 keV, a floor that an electron meets with far less energy.
- Accelerator · collider below that. At 10⁻¹⁸ m, Emin = 197 GeV. Colliders do not form an image; they reconstruct the debris of collisions.
Where it matters
- Electron microscopes. A 100 keV electron has a wavelength of about 3.7 pm. Conventional instruments resolve about 0.1 nm, limited by lens aberrations rather than by the wave.
- Sizes of nuclei and the proton. In the 1950s Robert Hofstadter scattered electrons of a few hundred MeV at Stanford and measured the sizes of nuclei and of the proton (Nobel Prize 1961). The sim puts the proton at 1.7 fm, where Emin = 116 MeV.
- Quarks inside the proton. Electrons of 7–20 GeV scattered at SLAC in the late 1960s revealed point-like constituents. Hard collisions at the LHC exchange momenta of a TeV, about 2 × 10⁻¹⁹ m in the sim's relation.
Go deeper: beating the limit without a shorter wave
- Super-resolution fluorescence microscopy (Nobel Prize in Chemistry, 2014) images detail well below λ/2 with visible light. It gains extra information by controlling which molecules emit, not by shortening the wave.
- The sim's rule is about what a plain, one-shot wave can resolve. It does not cover tricks that add information.
Summary
Key points
- The sim's rule is ƛ ≲ d, an order-of-magnitude criterion.
- With ƛ = ħ/p and E = pc, it gives Emin = ħc/d.
- Each decade of size costs one decade of energy.
- Emin is a floor, not a beam energy.
Common mix-ups
- "A better lens or a brighter beam lets you see smaller." The wavelength sets the limit. Brightness only adds signal.
- "Emin = 197 GeV means a 197 GeV machine." Emin is a momentum, written as an energy. A massive probe with that momentum carries less kinetic energy.
- "The wave drawn in the stage has wavelength d." It is drawn with period ƛ = d. The true wavelength is λ = 2πƛ, about 6.3 times longer.
Things to try on your own
- Set d to 10 nm and then to 100 pm. Predict Emin from ħc = 197.3 eV·nm, then check the readout.
- Drag along the ruler band to the green-to-cyan edge and read Emin.
- Move the Emin slider to about 100 MeV and read which object d now matches.