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A 75-W light source consumes 75 W of electrical power. Assume all this energy goes into emitted light of wavelength 600 nm. (a) Calculate the frequency of the emitted light. (b) How many photons per second does the source emit? (c) Are the answers to parts (a) and (b) the same? Is the frequency of the light the same thing as the number of photons emitted per second? Explain.

Short Answer

Expert verified
Frequency is about \(5 \times 10^{14}\) Hz; emits about \(2.26 \times 10^{20}\) photons/sec. Frequency is not the same as the number of photons emitted.

Step by step solution

01

Understanding Wavelength and Frequency

The wavelength of the light is given as 600 nm. To calculate frequency, we use the formula \( c = \lambda u \), where \( c \) is the speed of light (\( 3 \times 10^8 \) m/s), \( \lambda \) is the wavelength, and \( u \) is the frequency. Convert 600 nm to meters: \( 600 \times 10^{-9} \) m.
02

Calculate Frequency

Rearrange the formula \( \lambda u = c \) to solve for \( u \): \( u = \frac{c}{\lambda} \). Substitute the values to find frequency; \( u = \frac{3 \times 10^8}{600 \times 10^{-9}} \approx 5 \times 10^{14} \) Hz.
03

Calculate Energy of One Photon

The energy \( E \) of one photon can be calculated using the formula \( E = h u \), where \( h \) is Planck's constant (\( 6.63 \times 10^{-34} \) Js). Thus, \( E = 6.63 \times 10^{-34} \times 5 \times 10^{14} \approx 3.315 \times 10^{-19} \) J/photon.
04

Calculate Number of Photons Emitted

The power of the light source is 75 W, which means 75 J/s are being emitted. To find the number of photons emitted per second, divide power by the energy per photon: \( \frac{75}{3.315 \times 10^{-19}} \approx 2.26 \times 10^{20} \) photons per second.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Frequency Calculation
Frequency is a way to describe how often a wave oscillates in a given amount of time. Specifically for light, frequency is how many wave crests pass by a point each second. It's a central property of electromagnetic waves and is measured in hertz (Hz), where 1 Hz equals one wave per second.

To calculate the frequency of light when you know its wavelength, you use the equation \( c = \lambda u \), where \( c \) is the speed of light (\(3 \times 10^8\) meters per second), \( \lambda \) is the wavelength, and \( u \) is the frequency. When you rearrange this formula to solve for frequency, it becomes \( u = \frac{c}{\lambda} \).

For example, if a light source emits a wavelength of 600 nm (nanometers), you first convert this wavelength into meters: \(600 \times 10^{-9}\) m. Plugging this into the frequency formula, you divide the speed of light by the wavelength in meters: \( u = \frac{3 \times 10^8}{600 \times 10^{-9}} \). This calculation results in a frequency of approximately \(5 \times 10^{14}\) Hz.

This frequency tells you how rapidly the light waves are oscillating, which is vital for differentiating colors in the visible spectrum.
Photon Energy
When it comes to photons, they are the tiny packets of energy that constitute light. Each photon carries energy, and the amount of this energy depends on the light's frequency.

To calculate the energy of a single photon, we use Planck's equation: \( E = h u \). Here, \( E \) represents the energy, \( h \) is Planck's constant (\(6.63 \times 10^{-34}\) Joule seconds), and \( u \) is the frequency of the light. The energy of a photon is directly proportional to its frequency: the higher the frequency, the more energy a photon possesses.

Applying this to our example with light of frequency \(5 \times 10^{14}\) Hz, the energy of one photon is \( E = 6.63 \times 10^{-34} \times 5 \times 10^{14} \approx 3.315 \times 10^{-19} \) Joules. This illustrates how each photon, although extremely small, carries a specific quantum of energy, which determines its interactions with matter.
Wavelength and Frequency Relationship
The relationship between wavelength and frequency of light is a fundamental aspect of wave physics. Wavelength and frequency are inversely related, meaning when one increases, the other decreases. This relationship is expressed by the formula \( c = \lambda u \), signifying the product of wavelength \( \lambda \) and frequency \( u \) equals the constant speed of light \( c \).

This explains why light with a longer wavelength has a lower frequency, and conversely, light with a shorter wavelength has a higher frequency. This interplay is crucial because it dictates the position of light within the electromagnetic spectrum, from gamma rays with very high frequencies and short wavelengths to radio waves with low frequencies and long wavelengths.

Understanding this relationship helps in identifying different types of electromagnetic waves based on their properties, such as visible light which falls between approximately 400 nm to 700 nm in wavelength, corresponding to frequencies ranging from about \(4.3 \times 10^{14}\) Hz to \(7.5 \times 10^{14}\) Hz.

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Most popular questions from this chapter

A laser used to weld detached retinas emits light with a wavelength of 652 nm in pulses that are 20.0 ms in duration. The average power during each pulse is 0.600 W. (a) How much energy is in each pulse in joules? In electron volts? (b) What is the energy of one photon in joules? In electron volts? (c) How many photons are in each pulse?

What would the minimum work function for a metal have to be for visible light (380-750 nm) to eject photoelectrons?

In developing night-vision equipment, you need to measure the work function for a metal surface, so you perform a photoelectric-effect experiment. You measure the stopping potential \(V_0\) as a function of the wavelength \(\lambda\) of the light that is incident on the surface. You get the results in the table. In your analysis, you use \(c\) = 2.998 \(\times\) 10\(^8\) m/s and \(e\) = 1.602 \(\times\) 10\(^{-19}\) C, which are values obtained in other experiments. (a) Select a way to plot your results so that the data points fall close to a straight line. Using that plot, find the slope and y-intercept of the best-fit straight line to the data. (b) Use the results of part (a) to calculate Planck's constant \(h\) (as a test of your data) and the work function (in eV) of the surface. (c) What is the longest wavelength of light that will produce photoelectrons from this surface? (d) What wavelength of light is required to produce photoelectrons with kinetic energy 10.0 eV?

A photon with wavelength \(\lambda\) = 0.0980 nm is incident on an electron that is initially at rest. If the photon scatters in the backward direction, what is the magnitude of the linear momentum of the electron just after the collision with the photon?

X rays are produced in a tube operating at 24.0 kV. After emerging from the tube, x rays with the minimum wavelength produced strike a target and undergo Compton scattering through an angle of 45.0\(^\circ\). (a) What is the original x-ray wavelength? (b) What is the wavelength of the scattered x rays? (c) What is the energy of the scattered x rays (in electron volts)?

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