Bohr Energy Levels Equation:
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The Bohr equation calculates the energy levels of electrons in hydrogen-like atoms. It's based on Niels Bohr's model of the atom and provides the energy of an electron in the nth quantum state.
The calculator uses the Bohr equation:
Where:
Explanation: The equation shows that electron energy levels are quantized and depend on the atomic number and quantum number.
Details: Calculating energy levels helps predict atomic spectra, understand chemical bonding, and explain electron transitions that produce spectral lines.
Tips: Enter atomic number (Z) as a positive integer (1 for hydrogen, 2 for helium, etc.) and quantum number (n) as a positive integer (1 for ground state).
Q1: Why is the energy negative?
A: Negative energy indicates the electron is bound to the nucleus. Zero energy would mean the electron is free.
Q2: Does this work for all atoms?
A: The equation works best for hydrogen-like atoms (single electron systems like H, He+, Li2+, etc.).
Q3: What are typical energy values?
A: For hydrogen (Z=1), ground state (n=1) is -13.6 eV, first excited state (n=2) is -3.4 eV.
Q4: What are the limitations of Bohr's model?
A: It doesn't explain fine structure, Zeeman effect, or multi-electron atoms well. Quantum mechanics provides more complete solutions.
Q5: How does this relate to atomic spectra?
A: Energy differences between levels correspond to photon energies emitted/absorbed in spectral lines.