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Quantum Phenomena Calculator

Quantum phenomena calculations. Tunneling, photoelectric effect, Compton scattering, blackbody radiation, and quantum entanglement.

About this calculator

This calculator bundles five independent quantum-mechanics formulas behind a single Phenomenon selector, and only the inputs relevant to whichever mode you pick are shown -- the other modes' fields never affect the result you're looking at. In the default Quantum Tunneling mode, a particle with less energy than a barrier's height still has some probability of appearing on the far side; the Transmission Coefficient responds to both Barrier Height and Barrier Width, since together they set how far the particle's energy falls short of clearing the barrier and how much material the wavefunction has to tunnel through, and both feed the same exponential suppression term. Photoelectric Effect mode applies Einstein's equation (kinetic energy equals photon energy minus the material's work function) to find the maximum kinetic energy of an electron knocked loose by light. Compton Scattering computes the wavelength shift of an X-ray photon after it bounces off an electron, using the Compton wavelength of the electron as the scale factor.

Blackbody Radiation applies the Stefan-Boltzmann and Wien's displacement laws to find the total radiated power and peak emission wavelength of an object at a given temperature. Quantum Entanglement mode is descriptive rather than computed from a physical measurement: it reports the standard properties (correlation type, entropy, CHSH bound) of whichever Bell state you select, rather than deriving them from other numeric inputs. What none of these five modes model: real-world imperfections such as detector efficiency, thermal noise, or decoherence -- each is the textbook, idealized version of its formula.

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How to Use This Calculator
  1. In the Tunneling section, enter Particle Energy (eV), Barrier Height (eV), and Barrier Width (nm) to compute transmission probability.
  2. Switch to Photoelectric Effect and enter Photon Wavelength (nm) and Work Function (eV) to see maximum kinetic energy of ejected electrons.
  3. Use the Compton Scattering section: enter Incident Wavelength (nm/Å) and Scattering Angle (°) to compute wavelength shift Δλ.
  4. In Blackbody Radiation, enter Temperature (K) to get peak wavelength from Wien's law and compare to visible spectrum.
  5. In Quantum Entanglement mode, pick a Bell State, Number of Qubits, and Measurement Basis to see that state's correlation type, entanglement entropy, and CHSH bound -- these are textbook properties of the selected state, not derived from a physical measurement.
  6. Check the Tunneling chart showing Transmission vs. Barrier Width to visualize exponential suppression.

What each input means

Phenomenon
Calculation mode to use.
Particle Mass (kg)
Electron: 9.109e-31 kg
Work Function (eV)
Cu: 4.7, Na: 2.3, Cs: 2.1
Incident Wavelength (nm)
X-ray region
Temperature (K)
Sun: 5778K
Measurement Basis
Quantum measurement basis.

How this is calculated

Formula

T ≈ e^(-2κa) | KE = hf - φ | Δλ = λ_c(1-cos θ) | λ_peak = b/T

Worked example, using the default values

  1. Identify Input Parameters
    4 parameters
    Phenomenon = 0, Barrier Height (eV) = 1, Barrier Width (nm) = 1, Particle Energy (eV) = 0.5 = 4 input(s) provided
  2. Calculate Transmission Coefficient
    0.0028505810396497484 = 0.0028505810396497484
  3. Calculate Penetration Depth
    Penetration Depth
    0.27604864066523277 = 0.27604864066523277
  4. Calculate Tunneling Type
    Quantum tunneling = Quantum tunneling

Engine last updated . Checked against 7 independently-derived tests — how we verify calculators. Built by Paul Gunder, a software engineer, not a licensed financial, medical, or legal professional.

Frequently Asked Questions

Why doesn't changing the photon wavelength affect my tunneling result?

Because Photon Wavelength belongs to the Photoelectric Effect mode, not Quantum Tunneling -- the calculator only feeds the four tunneling inputs (Barrier Height, Barrier Width, Particle Energy, and Particle Mass) into the Transmission Coefficient formula. Switch the Phenomenon selector to "Photoelectric Effect" to see photon wavelength drive a result, specifically the ejected electron's maximum kinetic energy.

Which inputs matter most for the tunneling transmission coefficient?

Barrier Height and Barrier Width, not Particle Mass or Particle Energy alone. Barrier Height sets V₀ in the exponential suppression term that governs how much of the particle's wavefunction survives crossing the barrier, and Barrier Width sets how much material that wavefunction has to tunnel through -- both appear directly inside the same exponential, which is why the transmission coefficient falls off so sharply as either one increases.

Why does the Compton wavelength shift only depend on the scattering angle?

The Compton shift formula, Δλ = λc(1 − cos θ), factors out the electron's Compton wavelength (a fixed physical constant, about 2.43 picometers) from the angle-dependent term entirely -- the incident photon's own wavelength does not appear in the shift itself, only in the final wavelength (incident wavelength plus the shift). That is why the shift maxes out at exactly twice the Compton wavelength, at a 180° backscatter.

Does raising the temperature always shift blackbody radiation toward blue?

Yes, within the visible-light classification this calculator uses. Wien's displacement law puts the peak emission wavelength inversely proportional to temperature, so hotter objects peak at shorter (bluer) wavelengths -- the Sun's surface at 5,778 K peaks in visible green-yellow light, while a much hotter blue star's peak shifts into the ultraviolet, and a cooler object like a candle flame peaks in the infrared, below what the eye perceives as color at all.

Why do the entanglement entropy and CHSH values not depend on my inputs?

The Quantum Entanglement mode largely reports the textbook properties of whichever Bell state and qubit count you select rather than computing them from a measured quantity -- the CHSH quantum bound (2√2, the Tsirelson bound) is a fixed mathematical result for any maximally entangled two-qubit state, and the maximum entanglement entropy depends only on how many qubits you split into two halves, not on a continuous input you can dial up or down.

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