What is the Interferometer multi-solver?

Interferometer is a guided workflow that chains 3 individual PolySim solvers into one end-to-end analysis, piping each result into the next step.

Yes. Every step runs entirely in your browser using real numerics — no install, no account, no cloud cost. Custom or private solver packs are available as a paid service.

Physics & Quantum Pack · Multi-Solver

Interferometer

Fringes & coherence. This multi-solver chains 3 solvers into a single guided workflow — run each step in order and carry the result forward.

Workflow steps

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Wave Interference

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Wave Interference StudioLive

two-source interference · ripple tank

Controls

Speed1×

Two point sources emit circular waves — where they meet, you see constructive and destructive interference fringes. Drag either source on the canvas to reposition it and watch the pattern update live.

Presets

Frequency

Source separation

▶ Run in Python

Data Inspector

Sources2

Grid220×220

Wavelength15.7 px

Separation100 px

Patterninterference fringes

Governing equation

y = A_{1} sin (k r_{1} - ω t) + A_{2} sin (k r_{2} - ω t), Δ r = mλ, λ \approx 15.7 px, Δ s = 100 px

Reading this result: Wavelength is about 15.7 px and the two sources sit 100 px apart. Bright fringes appear where the path difference to the two sources equals a whole number of wavelengths (constructive interference); dark fringes fall halfway between, where the difference is a half-wavelength (destructive interference). Shrinking the wavelength or widening the separation would pack more fringes into the same space.

Runs locally in your browser — free forever. Scale to the cloud when reality gets heavy.

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Double Slit

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Double-Slit ExperimentLive

wave interference + diffraction

Controls

The iconic experiment: two slits create interference fringes, modulated by each slit's diffraction envelope.

Presets

Slit separation d

Slit width a

Wavelength λ

▶ Run in Python

Data Inspector

Fringe spacing∝ λ/d

Envelope∝ λ/a

Regimeinterference-dominated

Governing equation

I = I_{0} cos^{2} \frac{π d sin θ}{λ} sinc^{2} \frac{π a sin θ}{λ}, Δ y = \frac{λ L}{d} = \frac{20 \cdot 800}{40} = 400

Reading this result: Two-slit interference sets the fine fringe spacing (∝ λ/d) while single-slit diffraction sets the envelope (∝ λ/a); here about 10 bright fringes fit under the central peak.

Runs locally in your browser — free forever. Scale to the cloud when reality gets heavy.

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Single Slit

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Single-Slit DiffractionLive

light bending around edges

Controls

Presets

Slit width (µm)

Wavelength (nm)

Send light through a narrow slit and it fans out into a bright central band flanked by dimmer fringes — diffraction. The pattern follows a sinc-squared curve, with the first dark fringe where the path difference across the slit equals one wavelength. Narrower slits spread the light more, the diffraction limit that caps every lens and telescope's sharpness.

▶ Run in Python

Data Inspector

First minimum1.6°

Central width3.2°

Slit/λ36.4

Governing equation

I = I_{0} sinc^{2} β, β = \frac{π a sin θ}{λ}, a = 20 μ m, λ = 550 nm

Reading this result: Wide slit relative to the wavelength: the central peak is tight and the beam stays nearly collimated, with only faint fringes.

Runs locally in your browser — free forever. Scale to the cloud when reality gets heavy.

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Frequently asked questions

What is the Interferometer multi-solver?: Interferometer is a guided workflow that chains 3 individual PolySim solvers into one end-to-end analysis, piping each result into the next step.
Is it free to use?: Yes. Every step runs entirely in your browser using real numerics — no install, no account, no cloud cost. Custom or private solver packs are available as a paid service.