Determining Maximum Wavelength of Incident Radiation

In summary: So Kmax is the energy of the electron, not the photon.In summary, to determine the maximum wavelength of incident radiation on a metallic surface that will cause photo-emission to occur, we can use the equations Kmax = hc/λ + ∅ and [λ][/c] = hc/∅. By solving for the work function ∅ using the values obtained for the kinetic energies at different wavelengths, we can then use the work function to find the wavelength that results in a kinetic energy of zero. This is the maximum wavelength that will cause photo-emission on the surface.
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Homework Statement


When a certain metallic surface is illuminated with electromagnetic radiation of wavelength λ
max kinetic energy of photoelectrons is 40.5 eV. On same surface infrared radiation of 3λ, the ma kinetic energy is 5% less than that of incident radiation. Determine the maximum wavelength of incident radiation on this surface that will cause photo-emission to occur.

Homework Equations



Kmax = hc/λ + ∅

[λ][/c] = hc/∅

The Attempt at a Solution



okay, for wavelength λ I said that

∅= Kmax - hc/λ = 40.5 eV - 1240eV / λ

then for wavelength 3λ

∅= 38.475eV - 1240eV/ 3λ

Now, I want to plug in these values obtained for the work function ∅ into the Max wavelength equation (or cutoff wavelength equation) , but since I have two values what do I do?

Is this the write route
 
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I think "the ma kinetic energy is 5% less than that of incident radiation" means .95*40.5 eV.

If you sub the wavelength and Kmax for each of the two wavelengths into your first formula, you will have two equations with two unknowns, ∅ and λ. If you solve them for the ∅ characteristic of that surface, you will then have an equation relating Kmax to λ with no other unknowns. Use it to find the λ that results in a Kmax of zero. That is the wavelength that just barely causes emission. Any longer wavelength will result in negative Kmax, which is no emission at all.

hc/λ is the energy of the photon. -∅ is the energy required to break an electron out of the metal surface. Kmax is the remaining energy of the electron. That formula is usually written Kmax = hc/λ - W where W is called the Work function of the metal and is the energy required to pop an electron out of the metal.
 

1. What is the purpose of determining the maximum wavelength of incident radiation?

Determining the maximum wavelength of incident radiation is important in various fields of science, including optics, spectroscopy, and astronomy. It helps in understanding the behavior of light and its interactions with matter, as well as in identifying the chemical composition of substances.

2. How is the maximum wavelength of incident radiation measured?

The maximum wavelength of incident radiation can be measured using a spectrometer or a spectrophotometer. These instruments use diffraction or interference patterns to separate the different wavelengths of light and determine the maximum wavelength.

3. What factors affect the maximum wavelength of incident radiation?

The maximum wavelength of incident radiation is primarily affected by the properties of the light source, such as its temperature and composition. It is also influenced by the medium through which the light travels, as well as the physical properties of the object or substance being studied.

4. How does the maximum wavelength of incident radiation relate to the energy of light?

The maximum wavelength and energy of light are inversely proportional to each other. This means that as the wavelength increases, the energy decreases. This relationship is described by the equation: E = hc/λ, where E is energy, h is Planck's constant, c is the speed of light, and λ is the wavelength.

5. Can the maximum wavelength of incident radiation be calculated?

Yes, the maximum wavelength of incident radiation can be calculated using the Wien's displacement law, which states that the product of the maximum wavelength and the temperature of the light source is a constant value. This law is often used in thermal and astronomical studies to determine the temperature of a light source.

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