here are the solutions to questions 6 and 7, translated into English.
Question 6: Photoelectric Effect
6. d) (i) Define the photoelectric effect
The photoelectric effect is the phenomenon of electron emission from a material (usually a metal) when it is exposed to electromagnetic radiation (light) of a sufficiently high frequency.
6. d) (ii) State two experimental observations concerning the photoelectric effect that classical physics could not explain.
- Observation 1: Threshold frequency. Electron emission only occurs if the frequency of the incident light is above a certain minimum value (threshold frequency), regardless of the light's intensity. Classical physics predicted that any frequency of light, given sufficient intensity and time, should be able to eject electrons.
- Observation 2: Instantaneous emission. Electrons are emitted almost instantaneously (in less than 10−9 seconds) as soon as light of the threshold frequency or higher strikes the metal, even at very low intensity. Classical physics predicted a time delay for electrons to accumulate enough energy from the light wave.
6. e) Describe an experiment to determine Planck's constant. Your account should include a diagram, procedure, precautions, observations, and conclusion.
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Diagram:
The experimental setup includes a vacuum tube with a photocathode (emitting metal) and an anode (collector). A monochromatic light source illuminates the photocathode. An external circuit is connected to the anode and cathode, including a variable voltage source, an ammeter in series to measure the photocurrent, and a voltmeter in parallel to measure the applied voltage.
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Procedure:
- Illuminate the photocathode with monochromatic light of a known frequency f.
- Apply a negative voltage to the anode relative to the cathode (stopping voltage Vs). Increase this negative voltage until the measured photocurrent becomes zero. Record this value of Vs.
- Repeat step 2 for several different frequencies of monochromatic light.
- Plot a graph of the stopping voltage Vs against the frequency f of the incident light.
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Observations:
The graph of Vs versus f is a straight line.
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Conclusion (Theory):
According to Einstein's photoelectric effect equation, the energy of an incident photon hf is used to overcome the work function ϕ and provide the maximum kinetic energy KEmax to the emitted electrons:
hf=ϕ+KEmax
The maximum kinetic energy is related to the stopping voltage Vs by KEmax=eVs, where e is the elementary charge of the electron. Substituting and rearranging for Vs:
Vs=ehf−eϕ
This equation is in the form y=mx+c. The slope (gradient) of the Vs versus f graph is equal to eh. Therefore, Planck's constant h can be determined by multiplying the slope of the graph by the elementary charge of the electron e:
h=slope×e
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Precautions:
- Use strictly monochromatic light for each measurement.
- Maintain the vacuum in the tube to prevent electron collisions with air molecules.
- Clean the metal surface to avoid impurities.
- Shield the apparatus from any stray light.
- Use a very sensitive ammeter.
6. f) A certain element has a work function of 1.90 eV. Determine:
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Constants used:
- Planck's constant h=6.626×10−34J⋅s
- Speed of light c=3.00×108 m/s
- Elementary charge e=1.602×10−19 C
- 1eV=1.602×10−19 J
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Given data:
- Work function ϕ=1.90 eV
- Wavelength of incident light λ=4.50×10−7 m
6. f) (i) Its threshold wavelength;
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Step 1: Convert the work function to Joules.
ϕ=1.90eV×1.602×10−19J/eV=3.0438×10−19J
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Step 2: Use the formula for work function in terms of threshold wavelength λ0.
ϕ=λ0hc
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Step 3: Calculate λ0.
λ0=ϕhc=3.0438×10−19J(6.626×10−34J⋯)×(3.00×108m/s)
λ0=3.0438×10−19J1.9878×10−25J\cdotm≈6.529×10−7m
The threshold wavelength is 6.53×10−7m.
6. f) (ii) The maximum kinetic energy of the emitted electrons when the element is illuminated by light of wavelength 4.50×10−7 m;
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Step 1: Calculate the energy of the incident photons.
Ephoton=λhc=4.50×10−7m(6.626×10−34J⋯)×(3.00×108m/s)
Ephoton=4.50×10−7m1.9878×10−25J\cdotm≈4.4173×10−19J
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Step 2: Use the photoelectric effect equation to find the maximum kinetic energy.
KEmax=Ephoton−ϕ
KEmax=4.4173×10−19J−3.0438×10−19J
KEmax=1.3735×10−19J
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Step 3: (Optional) Convert the maximum kinetic energy to eV.
KEmax=1.602×10−19J/eV1.3735×10−19J≈0.857eV
The maximum kinetic energy is 1.37×10−19J(or0.857eV).
6. f) (iii) The stopping potential of this element.
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Step 1: Use the relationship between maximum kinetic energy and stopping potential Vs.
KEmax=eVs
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Step 2: Calculate Vs.
Vs=eKEmax=1.602×10−19C1.3735×10−19J
Vs≈0.8573V
The stopping potential is 0.857V.
Question 7: Analysis of Semiconductor Diode Data
The given equation is I=I0eβV. To determine the constants β and I0 from a graph, we need to linearize this equation.
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Step 1: Linearization of the equation.
Take the natural logarithm (ln) of both sides of the equation:
ln(I)=ln(I0eβV)
Using logarithm properties (ln(ab)=ln(a)+ln(b) and ln(ex)=x):
ln(I)=ln(I0)+ln(eβV)
ln(I)=ln(I0)+βV
This equation is in the form y=mx+c, where:
- y=ln(I)
- x=V
- m=β (the slope of the graph)
- c=ln(I0) (the y-intercept)
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Step 2: Data preparation.
Convert current values I to Amperes (A) and voltage V to Volts (V), then calculate ln(I).
| I/×10−4 A | I (A) | ln(I) (unitless) | V/mV | V (V) |
|--------------------|-----------------------|---------------------|--------|---------|
| 0.004 | 4.00×10−7 | −14.524 | 255 | 0.255 |
| 0.016 | 1.60×10−6 | −13.347 | 315 | 0.315 |
| 0.036 | 3.60×10−6 | −12.533 | 345 | 0.345 |
| 0.089 | 8.90×10−6 | −11.630 | 385 | 0.385 |
| 0.182 | 1.82×10−5 | −10.913 | 410 | 0.410 |
| 0.552 | 5.52×10−5 | −9.802 | 455 | 0.455 |
| 0.903 | 9.03×10−5 | −9.313 | 475 | 0.475 |
| 1.400 | 1.40×10−4 | −8.874 | 495 | 0.495 |
| 1.820 | 1.82×10−4 | −8.611 | 505 | 0.505 |
| 2.230 | 2.23×10−4 | −8.408 | 515 | 0.515 |
a) Plot a suitable graph from which β and I0 could be obtained.
- Graph Title: Graph of ln(I) versus V.
- Axes:
- The y-axis should represent ln(I).
- The x-axis should represent voltage V in Volts (V).
- Scale: Choose appropriate scales for each axis so that the data points occupy most of the graph paper. For example, for the x-axis, a scale of 0.05 V per major grid line could be used, and for the y-axis, a scale of 1.0 per major grid line.
- Plotting Points: Plot each data point (V,ln(I)) from the prepared table on the graph.
- Line of Best Fit: Draw a straight line that passes as close as possible to all the plotted points. This line represents the linear relationship between ln(I) and V.
b) Determine the values of the constants β and I0.
We will use the slope of the straight line to find β and the y-intercept to find I0. For this, we will choose two widely separated points on the line of best fit (or the extreme points from our data for an estimation).
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Step 1: Calculate β (the slope).
Let's use the extreme points from our table to calculate the slope:
Point 1: (V1,ln(I1))=(0.255V,−14.524)
Point 2: (V2,ln(I2))=(0.515V,−8.408)
The slope β is given by:
β=V2−V1ln(I2)−ln(I1)
β=0.515V−0.255V−8.408−(−14.524)
β=0.260V6.116
β≈23.523V−1
Rounded to three significant figures:
\beta \approx \text{23.5 V^{-1}}
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Step 2: Calculate I0 (from the y-intercept).
The y-intercept c is equal to ln(I0). We can find it using the line equation ln(I)=βV+ln(I0) and one of the data points (e.g., Point 1) with the calculated value of β.
ln(I0)=ln(I1)−βV1
ln(I0)=−14.524−(23.523V−1×0.255V)
ln(I0)=−14.524−5.998365
ln(I0)=−20.522365
To find I0, we take the exponential of both sides:
I0=e−20.522365
I0≈1.22×10−9A
Rounded to three significant figures:
I_0 \approx \text{1.22 \times 10^{-9} A}
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