The Bohr Condition: For an atom to absorb or emit radiation, the energy of the photon must exactly match the difference between two energy levels. This is expressed as .
Conservation of Energy: During absorption, the energy of the incoming photon is completely transferred to the electron, moving it to a higher state. During emission, the potential energy lost by the electron as it drops to a lower state is converted into the energy of a departing photon.
Frequency-Wavelength Relationship: Since the speed of light is constant (), the energy can also be expressed in terms of wavelength: . This implies that larger energy gaps result in shorter wavelengths (bluer light).
Calculating Transition Energy: To determine the frequency of light emitted, first identify the initial and final energy states of the electron. Subtract the lower energy value from the higher energy value to find the energy of the emitted photon.
Predicting Absorption Spectra: When white light passes through a cool gas, specific frequencies are removed. By identifying these 'missing' frequencies, one can determine the specific energy level structure of the atoms in the gas.
Unit Conversion: Energy levels are often given in electron-volts (eV). To use the standard Planck's constant ( J·s), you must convert eV to Joules using the conversion factor .
Check the Energy Match: Always remember that an atom will only absorb a photon if its energy matches the gap exactly. If a photon has slightly more or slightly less energy than the gap, it will pass through the atom without being absorbed.
Inverse Relationship: Be careful with the relationship between energy and wavelength. A common mistake is assuming a 'higher' energy transition produces a 'longer' wavelength; in fact, higher energy means a shorter wavelength.
State Identification: Ensure you distinguish between the 'ground state' () and the 'first excited state' (). Miscounting the levels is a frequent source of calculation errors in multi-step problems.
The 'In-Between' Fallacy: Students often mistakenly believe an electron can absorb half a photon's energy or stop between levels. In reality, the transition is 'all or nothing' and instantaneous.
Kinetic vs. Potential Energy: Do not confuse the electron's orbital speed with the photon's energy. The photon's energy relates to the change in the atom's total internal energy (potential + kinetic), not just the speed of the electron.
Ignoring the Work Function: In the context of the photoelectric effect (a related topic), remember that absorption can sometimes lead to ionization if the photon energy exceeds the binding energy of the electron.