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De Broglie Wavelength Equation Calculator

De Broglie Wavelength Equation:

\[ \lambda = \frac{h}{m v} \]

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1. What is the De Broglie Wavelength Equation?

The De Broglie wavelength equation describes the wave nature of matter, showing that particles like electrons exhibit wave-like properties. It was proposed by Louis de Broglie in 1924 and is fundamental to quantum mechanics.

2. How Does the Calculator Work?

The calculator uses the De Broglie wavelength equation:

\[ \lambda = \frac{h}{m v} \]

Where:

Explanation: The equation shows that the wavelength of a particle is inversely proportional to its momentum (mass × velocity).

3. Importance of Wavelength Calculation

Details: Calculating De Broglie wavelength is crucial for understanding quantum behavior, electron microscopy, and wave-particle duality experiments. It helps predict when quantum effects become significant.

4. Using the Calculator

Tips: Enter mass in kilograms and velocity in meters per second. For subatomic particles, use very small mass values (e.g., electron mass = 9.109 × 10⁻³¹ kg).

5. Frequently Asked Questions (FAQ)

Q1: Why is Planck's constant in the equation?
A: Planck's constant relates the energy of a photon to its frequency, and in this context, it connects the particle properties (mass, velocity) with wave properties (wavelength).

Q2: What's a typical wavelength for an electron?
A: For an electron with 1 eV energy (velocity ~593 km/s), λ ≈ 1.23 nm - comparable to atomic spacing in crystals, explaining electron diffraction patterns.

Q3: Does this apply to macroscopic objects?
A: Yes, but wavelengths are extremely small. A 1 kg object moving at 1 m/s has λ ≈ 6.6 × 10⁻³⁴ m - far too small to observe wave effects.

Q4: How was this equation verified experimentally?
A: Davisson-Germer experiment (1927) showed electron diffraction from nickel crystals, confirming wave nature with wavelengths matching de Broglie's prediction.

Q5: What about relativistic particles?
A: For particles approaching light speed, use relativistic momentum \( p = \gamma m v \) where \( \gamma \) is the Lorentz factor.

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