Chapter 2 Flashcards
- State the major evidence for classifying light as a wave phenomenon. Use the de Broglie equation to show that matter has wavelike properties.
Lambda = h/mass*velocity
- Young’s double slit experiment
- Describe the electromagnetic spectrum and calculate wavelength from frequency or frequency from wavelength. Also be able to calculate the energy of a photon from its frequency or wavelength.
- Left to Right. Gamma rays, X - Rays, UV Light, Visible Light ( Blue - red) , Infrared, Microwave, Radio Waves
- Gamma Rays are smallest wavelength, Radio waves are the largest wavelength
- Gamma Rays are the highest frequency, Radio waves are the lowest frequency (Wavelength and frequency are inversely related)
- Wavelength*Frequency = Speed of light Change in Energy = h*frequency => h*c/wavelength
- Given the energies of a set of energy levels, predict the wavelengths or frequencies of the lines in a line spectrum. Alternatively, calculate the energy level separations from the wavelength or frequency of the lines in a line spectrum.
Practice Problems
- State the major evidence for classifying light as a particle.
- Photoelectric effect
- Explain the term “quantized” as it is applied to energy in this chapter.
- Energy can be gained or lost only in integer multiples of h*frequency.
- Each of these small “packets” of energy is called a quantum. A system can transfer energy only in whole quanta.
- = atoms and molecules can’t accept just any amount of energy, but instead only the amount of energy that exactly matches the size of these quanta.
- Describe the photoelectric effect and discuss what was learned from a study of this effect.
Refers to the phenomenon in which electrons are emitted from the surface of a metal when light strikes it.
(a) Light with frequency less than the threshold frequency produces no electrons.
(b) Light with frequency higher than the threshold frequency causes electrons to be emitted from the metal.
Summarize the series of electromagnetic radiation for the names
- Lyman: Emit to n = 1, Large transitions, Uv light
- Balmer: Emit to n= 2, Medium transitions, Visible light
- Paschen: Emit to n= 3, small transitions, Infrared “
- Explain what an atomic (line) spectrum is and describe the kind of information that it gives about the energy levels in an atom.
- A spectrum in which spectral line can be distinguished.
- Because each spectral line can be clearly distinguished, match each line to the transition between energy levels responsible for it.
- Changes in energy between discrete energy levels in hydrogen will produce only certain wavelengths of emitted light,
- Distinguish between a continuous spectrum and a line spectrum.
- Continuous spectrum results when white light is passed through a prism. This spectrum contains all the wavelengths of visible light.
- Line spectrum: emission spectrum, only shows wavelengths for which the photons were emitted
- Distinguish between an emission and an absorption spectrum.
- Absorption lines are where light has been absorbed by the atom thus you see a dip in the spectrum
- Emission spectra have spikes in the spectra due to atoms releasing photons at those wavelengths.
- EX: Hydrogen for example, indicates that only certain energies are allowed for the electron in the hydrogen atom.
- Explain how emission spectra and absorption spectra of the same element are related.
the lines in the emission spectrum of a substance are at the exact same wavelengths as the lines in the absorption spectrum of the same substance.
- State the Rydberg formula and explain its relationship to the spectrum of hydrogen atoms.
- Use Rydberg equation to calculate the wavelength of light emitted when energy is emitted from n final to n initial
- Look up formula - use exmple
- State the Bohr model of the hydrogen atom and explain its significance (work on this answer).
Key things to remember:
- Energy levels are stationary states
- Change in energy casues by electrons between stationary states
- When electron move, absorbing electron (increase in energy), or emitting energy (decreasing energy)
- Explain the relationship of a line in a spectrum to the atom’s energy levels and photons emitted by that atom.
The lines on the atomic spectrum relate to electron transitions between energy levels, if the electron drops an energy level a photon is released resulting in an emission line and if the electron absorbs a photon and rises an energy level an absorption line is observed on the spectrum.
- State the Heisenberg Uncertainty Principle and explain its meaning.
- The exact position of the electron is never known, which is consistent with the Heisenberg uncertainty principle:
- it is impossible to know accurately both the position and the momentum of a particle simultaneously.
- Think about how small the mass of an electron is - this helps to explain it’s uncertainty