AP Physics 2 · Unit 15 · Topic 15.5
Photon Thresholds in the Photoelectric Effect
Quantization, probability, nuclear processes, and relativity extend classical models at atomic scales.
1. Topic Lens
Photon Thresholds in the Photoelectric Effect is studied through modern physics. Connect the system boundary, interacting parts, and measurable evidence before applying a formula.
2. Why the Formula Works
The relationship is built from definitions and conservation reasoning:
- A photon carries discrete energy hf.
- The material requires work function φ to release an electron.
- Energy conservation leaves the remainder as the maximum electron kinetic energy.
3. Detailed Visual Model
4. Worked Example and Lab Link
A 5 eV photon strikes a surface with work function 2 eV. Find maximum electron kinetic energy.
Answer: Kmax=5-2=3 eV.
Investigation idea: Analyze original stopping-potential data versus frequency and infer threshold frequency and Planck-slope meaning.
Common trap: Light intensity changes photon count; below threshold frequency it does not release electrons in the ideal model.
Expanded Topic 15.5 Lesson
5. Learning Targets
- Use the photon model to explain immediate electron emission and the existence of a threshold frequency.
- Apply \(K_{\max}=hf-\phi\), \(eV_s=K_{\max}\), and the equivalent wavelength relationships.
- Predict separately how frequency, intensity, material, and applied voltage affect photoelectric data.
- Extract Planck's constant, work function, and threshold frequency from a linear graph.
- Distinguish maximum electron energy from photocurrent and identify limits of the ideal one-photon model.
6. The Effect and Its Boundary Condition
In the external photoelectric effect, incident light ejects electrons from a material surface. Emission occurs only when one photon supplies at least the material's work function \(\phi\):
The equality marks the ideal threshold. Above it, some photoelectrons leave with kinetic energy; below it, raising light intensity does not repair the energy shortage in the basic one-photon model.
7. Three Observations the Model Must Explain
A successful model must explain all three observations at once, not merely electron emission.
8. Original Photoelectric Apparatus Model
9. Einstein's One-Photon Energy Ledger
One photon transfers its energy to one electron. The minimum escape cost is the work function; any remaining energy can become electron kinetic energy:
The fastest emitted electrons require the least additional energy loss before leaving the surface, so
This maximum is an upper edge. Real photoelectrons can emerge with a distribution of smaller kinetic energies.
10. Work Function and Threshold Forms
At threshold, \(K_{\max}=0\). Therefore
The threshold wavelength is the longest wavelength that can eject an electron, not the shortest.
11. A Fast eV–nm Toolkit
If energies are in electron-volts, the numerical maximum kinetic energy in eV equals the stopping-potential magnitude in volts:
This shortcut follows from \(1\,\mathrm{eV}=e(1\,\mathrm V)\); it is a unit relationship, not the equation \(e=1\).
12. Worked Threshold Decision
A metal has \(\phi=2.30\,\mathrm{eV}\). Its threshold wavelength is
Light at 600 nm has lower photon energy and produces no photoelectrons in the ideal model. Light at 450 nm is shorter than the threshold wavelength and can eject electrons.
13. Worked Energy and Stopping-Potential Example
Light at 400 nm illuminates the same \(\phi=2.30\,\mathrm{eV}\) surface:
A retarding potential with magnitude 0.80 V stops even the fastest photoelectrons.
14. What Stopping Potential Actually Measures
When the collector repels electrons, each electron loses electric potential energy while crossing the tube. At the stopping condition for the fastest electrons,
Here \(V_s\) denotes the positive magnitude of the stopping potential. The actual applied collector voltage is retarding and may be plotted as \(-V_s\), so signs must be read from the circuit convention.
15. Original Linear Evidence Graph
16. Extract Physics from a Best-Fit Line
For a graph of \(K_{\max}\) versus \(f\), write \(y=mx+b\):
For a graph of \(V_s\) versus \(f\), the slope is \(h/e\) and the vertical intercept is \(-\phi/e\).
17. Example: Estimate \(h\) from Two Data Points
Suppose \(K_{\max}=0.50\,\mathrm{eV}\) at \(6.0\times10^{14}\,\mathrm{Hz}\) and \(1.33\,\mathrm{eV}\) at \(8.0\times10^{14}\,\mathrm{Hz}\). Then
Using either point gives \(\phi\approx2.0\,\mathrm{eV}\). A many-point best-fit line is more reliable than selecting two noisy measurements.
18. Frequency and Intensity Control Different Outcomes
| Change | \(K_{\max}\) | \(V_s\) | Photocurrent |
|---|---|---|---|
| Increase \(f\), fixed material and above threshold | increases | increases | not determined without photon-rate information |
| Increase monochromatic intensity at fixed \(f>f_0\) | unchanged | unchanged | generally increases |
| Increase intensity while \(f<f_0\) | no photoelectrons | not defined | remains zero in ideal one-photon model |
| Use a larger-\(\phi\) material at fixed \(f\) | decreases or emission stops | decreases or is absent | material-dependent |
For fixed frequency, higher intensity means a larger photon arrival rate. If emission probability and collection conditions are unchanged, more electrons per second give more current.
19. Photon Flux Is Not Photon Energy
For a monochromatic beam of incident power \(P_{\mathrm{light}}\), the photon arrival rate is
At fixed \(f\), doubling power doubles photon flux but leaves each photon's energy unchanged. At fixed power, raising frequency gives more energy per photon but fewer incident photons per second. That is why current comparisons require more than frequency alone.
20. Reading Photocurrent–Voltage Curves
21. Why Electron Energies Form a Distribution
Electrons begin in different material states and depths. Some lose energy through interactions before escaping, and their paths toward the collector differ. Consequently, a photocurrent curve samples a range of kinetic energies.
The Einstein equation specifies the maximum kinetic energy for the most favorable electrons, not that every emitted electron has exactly \(hf-\phi\).
22. Classical Prediction Versus Photon Evidence
| Question | Continuous classical transfer | Photon model | Observation |
|---|---|---|---|
| Weak light | long energy-accumulation delay | fewer events, but each sufficient photon acts promptly | no measurable buildup delay |
| Higher intensity | greater electron kinetic energy | more photons and usually more emitted electrons | current rises; \(K_{\max}\) does not |
| Low frequency | enough time or intensity should eventually eject electrons | each photon lacks the work-function energy | sharp material-dependent threshold |
23. Experimental Limits and Extensions
- The ideal equation uses a clean, specified surface; oxidation and contamination can change an effective work function.
- Contact potentials and instrument calibration can shift measured voltages.
- Very intense laser fields can enable multiphoton emission, which lies beyond the ordinary one-photon AP model.
- In semiconductors, internal photoelectric processes and band gaps require a different device model.
Use the stated ideal assumptions unless a problem provides additional surface or material information.
24. Open Simulation Investigation
- Open PhET Photoelectric Effect.
- Select one metal and keep light intensity fixed.
- Scan wavelength from long to short and bracket the onset of current.
- Convert the threshold wavelength to a work function and compare materials.
- Choose a wavelength above threshold and measure stopping potential.
- Change only intensity; record current and stopping potential.
- Restore intensity, change frequency, and repeat.
- Write two evidence-based claims: one about photon energy and one about photon number.
25. Data-Quality Investigation
- Measure \(V_s\) for at least five frequencies above threshold.
- Plot \(V_s\) versus \(f\) with uncertainties and fit a straight line.
- Infer \(h/e\), \(\phi/e\), and \(f_0\), including units.
- Inspect residuals rather than forcing a conclusion from correlation alone.
Use a simulation or supervised low-voltage apparatus. Do not construct high-voltage or ultraviolet equipment without qualified supervision and appropriate eye protection.
26. Common Reasoning Traps
- “Brighter means faster electrons.” At fixed frequency, brightness mainly changes electron rate, not \(K_{\max}\).
- Reversing the wavelength test: emission requires \(\lambda\le\lambda_0\).
- Giving negative kinetic energy: if \(hf-\phi<0\), report no emission in the ideal model.
- Equating all electron energies with \(K_{\max}\): the measured population has a distribution.
- Confusing stopping and accelerating voltages: stopping voltage opposes electron collection.
- Reading the wrong graph slope: \(K_{\max}\)-versus-\(f\) has slope \(h\); \(V_s\)-versus-\(f\) has slope \(h/e\).
27. AP-Style Reasoning Checks
- Light below threshold becomes ten times as intense. What changes in the ideal model?
- Above threshold, frequency rises while intensity stays fixed. What happens to \(K_{\max}\)?
- Above threshold, intensity doubles at fixed frequency. Compare \(V_s\) and saturation current.
- What does the horizontal intercept of a \(K_{\max}\)-versus-\(f\) graph represent?
- A metal has \(\phi=4.0\,\mathrm{eV}\). Can a 400 nm photon eject an electron?
- Why does zero current at the stopping potential identify a maximum energy?
Answers: no photoemission begins; it increases by \(h\Delta f\); \(V_s\) stays fixed while saturation current generally doubles; threshold frequency; no, the photon has about 3.10 eV; even the fastest electrons are turned back, so all slower ones are also stopped.
Explain how photon thresholds in the photoelectric effect supports or limits this conclusion: Kmax=5-2=3 eV.
Official curriculum reference: College Board AP Physics 2 course page. The explanation and worked example are independently written for this study site.