Quantum Physics: Black Body Radiation, Photoelectric & Compton Effects, and Wave-Particle Duality: 25 flashcards

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1. What is black body radiation?

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The spectrum of electromagnetic radiation emitted by a perfect absorber and emitter (a black body), which depends only on its temperature.

2. What was the ultraviolet catastrophe?

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The classical Rayleigh–Jeans law predicted infinite energy emission at short wavelengths, which contradicted experiments.

3. State Planck's quantum hypothesis.

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Energy is emitted or absorbed in discrete packets called quanta, with energy $E = h\nu$.

4. What is the value of Planck's constant $h$?

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$h = 6.626 \times 10^{-34}$ J·s

5. Define the photoelectric effect.

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The emission of electrons from a metal surface when light of frequency above a threshold falls on it.

6. What is threshold frequency in the photoelectric effect?

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The minimum frequency $\nu_0 = \phi/h$ below which no electrons are emitted, regardless of light intensity.

7. Write Einstein's photoelectric equation.

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$K_{max} = h\nu - \phi$, where $\phi$ is the work function.

8. What is the work function $\phi$?

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The minimum energy required to remove an electron from the surface of a metal.

9. What is the Compton effect?

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The increase in wavelength of X-rays when scattered by free electrons.

10. Write the Compton shift formula.

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$\Delta\lambda = \frac{h}{m_e c}(1 - \cos\theta)$

11. What is the Compton wavelength of the electron?

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$h/m_e c = 2.426$ pm

12. At what angle is the Compton shift maximum, and what is its value?

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At $\theta = 180^\circ$, the shift is maximum and equals $2h/m_e c = 4.852$ pm.

13. What did the Davisson–Germer experiment demonstrate?

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Electrons diffract like waves, confirming de Broglie's matter wave hypothesis.

14. State Heisenberg's uncertainty principle for position and momentum.

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$\Delta x \cdot \Delta p \geq \frac{h}{4\pi}$

15. What is the physical meaning of the wave function $\psi$?

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$|\psi|^2$ gives the probability density of finding the particle at a given position and time.

16. List the conditions a valid wave function must satisfy.

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It must be single-valued, continuous, finite, and normalizable.

17. Write the normalization condition for a wave function.

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$\int_{-\infty}^{\infty} |\psi|^2 dx = 1$

18. Calculate the energy of a photon with frequency $5 \times 10^{14}$ Hz.

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$E = h\nu = (6.626 \times 10^{-34})(5 \times 10^{14}) = 3.313 \times 10^{-19}$ J

19. If work function is 2.0 eV and photon energy is 3.5 eV, find $K_{max}$.

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$K_{max} = 3.5 - 2.0 = 1.5$ eV

20. Find the Compton shift for scattering at $90^\circ$.

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$\Delta\lambda = 2.426$ pm $\times (1 - \cos 90^\circ) = 2.426$ pm

21. Find the minimum uncertainty in momentum if an electron is confined to $1 \times 10^{-10}$ m.

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$\Delta p \geq \frac{h}{4\pi \Delta x} = 5.27 \times 10^{-25}$ kg m/s

22. What is the momentum of a photon?

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$p = h/\lambda$

23. What is the de Broglie wavelength of a particle?

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$\lambda = h/p$

24. Why does classical wave theory fail to explain the photoelectric effect?

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It predicts that brighter light gives more energetic electrons and any frequency works, but experiments show a threshold frequency and intensity-independent kinetic energy.

25. What is the energy–time uncertainty relation?

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$\Delta E \cdot \Delta t \geq \frac{h}{4\pi}$

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