Atomic and Nuclear Physics — Practice Quiz
A Physics cheat sheet for Atomic and Nuclear Physics — every key formula with its symbols defined — plus a medium-level practice quiz to test recall.
Formulas & key concepts
Bohr Model Radius: The radius \(r_n\) of the \(n\)-th orbit in a hydrogen-like atom with atomic number \(Z\).
Where: \(n\) = principal quantum number
Bohr Model Energy: The energy \(E_n\) of the \(n\)-th orbit in a hydrogen-like atom.
Rydberg Equation: Calculates the wavelength \(\lambda\) of a photon emitted/absorbed during a transition between levels \(n_i\) and \(n_f\).
Where: \(R\) = Rydberg constant \((1.097 \times 10^7 m^{-1})\)
X-ray Cutoff Wavelength: The minimum wavelength \(\lambda_{min}\) of X-rays produced by electrons accelerated through voltage \(V\).
Mass-Energy Equivalence: Energy \(E\) is equivalent to mass \(m\) multiplied by the speed of light squared \(c^2\). (Used for nuclear binding energy).
Where: \(c\) = speed of light
Binding Energy per Nucleon: The total binding energy \(BE\) divided by the mass number \(A\).
Radioactive Decay Law: The number of remaining radioactive nuclei \(N(t)\) after time \(t\).
Where: \(\lambda\) = decay constant
Half-Life: The time \(T_{1/2}\) required for half of the radioactive nuclei to decay.
Activity: The rate of decay \(A\) (decays per second) is proportional to the number of nuclei \(N\).
Where: Unit: Becquerel (Bq)
Practice quiz
What is the ratio of the radius of the $n=2$ orbit in a hydrogen atom ($Z=1$) to the radius of the $n=1$ orbit in a singly ionized helium atom ($Z=2$)?
- A) $2$
- B) $4$
- C) $8$
- D) $16$
Answer: C) $8$
Calculate the energy (in $eV$) required to ionize a hydrogen atom from its ground state ($n=1$).
- A) $3.4 \text{ eV}$
- B) $6.8 \text{ eV}$
- C) $13.6 \text{ eV}$
- D) $27.2 \text{ eV}$
Answer: C) $13.6 \text{ eV}$
A hydrogen atom undergoes a transition from the $n_i=3$ state to the $n_f=2$ state. What is the wavelength of the emitted photon? (Use $R = 1.097 \times 10^7 \text{ m}^{-1}$)
- A) $486 \text{ nm}$
- B) $656 \text{ nm}$
- C) $121 \text{ nm}$
- D) $1875 \text{ nm}$
Answer: B) $656 \text{ nm}$
What is the minimum wavelength of X-rays produced when electrons are accelerated through a potential difference of $50 \text{ kV}$? (Use $h = 6.626 \times 10^{-34} \text{ J} \cdot \text{s}$, $c = 3.00 \times 10^8 \text{ m/s}$, $e = 1.602 \times 10^{-19} \text{ C}$)
- A) $0.0124 \text{ nm}$
- B) $0.0248 \text{ nm}$
- C) $0.0496 \text{ nm}$
- D) $0.0620 \text{ nm}$
Answer: B) $0.0248 \text{ nm}$
If $1 \text{ kg}$ of mass were completely converted into energy, how much energy would be released? (Use $c = 3.00 \times 10^8 \text{ m/s}$)
- A) $3.00 \times 10^8 \text{ J}$
- B) $9.00 \times 10^{16} \text{ J}$
- C) $1.00 \text{ J}$
- D) $9.00 \times 10^{13} \text{ J}$
Answer: B) $9.00 \times 10^{16} \text{ J}$
A nucleus has a total binding energy ($BE$) of $28.3 \text{ MeV}$ and a mass number ($A$) of $4$. What is its binding energy per nucleon ($BEN$)?
- A) $4 \text{ MeV/nucleon}$
- B) $7.075 \text{ MeV/nucleon}$
- C) $14.15 \text{ MeV/nucleon}$
- D) $28.3 \text{ MeV/nucleon}$
Answer: B) $7.075 \text{ MeV/nucleon}$
A radioactive sample initially contains $N_0$ nuclei. After $3$ half-lives, how many nuclei remain?
- A) $N_0/2$
- B) $N_0/4$
- C) $N_0/8$
- D) $N_0/16$
Answer: C) $N_0/8$
A radioactive isotope has a decay constant ($\lambda$) of $0.0231 \text{ s}^{-1}$. What is its half-life ($T_{1/2}$)?
- A) $15 \text{ s}$
- B) $30 \text{ s}$
- C) $45 \text{ s}$
- D) $60 \text{ s}$
Answer: B) $30 \text{ s}$
A sample contains $1.0 \times 10^{10}$ radioactive nuclei and has a decay constant ($\lambda$) of $5.0 \times 10^{-3} \text{ s}^{-1}$. What is the activity ($A$) of the sample?
- A) $5.0 \times 10^6 \text{ Bq}$
- B) $5.0 \times 10^7 \text{ Bq}$
- C) $2.0 \times 10^{12} \text{ Bq}$
- D) $2.0 \times 10^{13} \text{ Bq}$
Answer: B) $5.0 \times 10^7 \text{ Bq}$
Which of the following statements correctly describes the relationship between the energy levels of a hydrogen atom and the wavelength of emitted photons during electron transitions?
- A) Larger energy differences between states result in longer emitted wavelengths.
- B) The energy of an emitted photon is inversely proportional to the difference in energy levels.
- C) Transitions to lower principal quantum numbers ($n_f$) generally result in the emission of higher energy photons.
- D) The Rydberg equation is only applicable for absorption spectra, not emission spectra.
Answer: C) Transitions to lower principal quantum numbers ($n_f$) generally result in the emission of higher energy photons.
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