Rydberg Equation:
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The Rydberg equation predicts the wavelength of light resulting from an electron moving between energy levels in a hydrogen atom. It was formulated by the Swedish physicist Johannes Rydberg in 1888.
The calculator uses the Rydberg equation:
Where:
Explanation: The equation calculates the inverse wavelength of the photon emitted when an electron transitions from a higher energy level (n₂) to a lower one (n₁).
Details: The Rydberg equation accurately predicts the wavelengths of the hydrogen spectral lines (Lyman, Balmer, Paschen series) and was crucial in the development of quantum mechanics.
Tips: Enter the initial (n₁) and final (n₂) energy levels as positive integers with n₂ > n₁. The Rydberg constant is pre-filled but can be adjusted for different hydrogen-like atoms.
Q1: What are typical values for n₁ and n₂?
A: For visible spectrum (Balmer series), n₁=2 and n₂=3,4,5... For UV (Lyman series), n₁=1. For IR (Paschen series), n₁=3.
Q2: Why does the equation use 1/λ instead of λ?
A: The equation was originally formulated in terms of wavenumber (1/λ), which is proportional to energy.
Q3: Can this be used for other elements?
A: The equation works best for hydrogen and hydrogen-like ions (He⁺, Li²⁺). For other elements, modified versions are needed.
Q4: What are the limitations of the Rydberg equation?
A: It doesn't account for fine structure, hyperfine structure, or other quantum effects that cause small shifts in spectral lines.
Q5: How accurate is the Rydberg constant?
A: The current accepted value is 1.0973731568160(21)×10⁷ m⁻¹, one of the most precisely determined physical constants.