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If the eye receives an average intensity greater than 1.0 \(\times\) 10\(^2\) W/m\(^2\), damage to the retina can occur. This quantity is called the \(damage\) \(threshold\) of the retina. (a) What is the largest average power (in mW) that a laser beam 1.5 mm in diameter can have and still be considered safe to view head-on? (b) What are the maximum values of the electric and magnetic fields for the beam in part (a)? (c) How much energy would the beam in part (a) deliver per second to the retina? (d) Express the damage threshold in W/cm\(^2\).

Short Answer

Expert verified
(a) 0.1767 mW, (b) 274.57 V/m (electric), 9.15 × 10⁻⁷ T (magnetic), (c) 0.1767 mJ/s, (d) 0.01 W/cm².

Step by step solution

01

Calculate Cross-sectional Area

First, we calculate the cross-sectional area of the laser beam. The diameter is given as 1.5 mm, which is 0.0015 meters. The radius is half of that: \( r = \frac{0.0015}{2} \text{ m} = 0.00075 \text{ m} \). The area \( A \) is given by the formula for the area of a circle: \( A = \pi r^2 = \pi (0.00075)^2 \approx 1.767 \times 10^{-6} \text{ m}^2 \).
02

Calculate Maximum Power (a)

The intensity (given in the problem as the damage threshold) is power per unit area. Therefore, the maximum power \( P \) is given by \( P = I \times A \), where \( I = 1.0 \times 10^2 \text{ W/m}^2 \) and \( A = 1.767 \times 10^{-6} \text{ m}^2 \). Hence, \( P = 1.0 \times 10^2 \times 1.767 \times 10^{-6} = 1.767 \times 10^{-4} \text{ W} \). To convert to milliwatts (mW), multiply by 1000: \( 1.767 \times 10^{-4} \times 1000 = 0.1767 \text{ mW} \).
03

Calculate Maximum Electric Field (b)

The average intensity \( I \) is related to the maximum electric field \( E_{max} \) by the equation \( I = \frac{1}{2} \varepsilon_0 c E_{max}^2 \), where \( \varepsilon_0 = 8.85 \times 10^{-12} \text{ F/m} \) (the permittivity of free space) and \( c = 3.00 \times 10^8 \text{ m/s} \) (the speed of light). Solving for \( E_{max} \), we get: \( E_{max} = \sqrt{\frac{2I}{\varepsilon_0 c}} = \sqrt{\frac{2 \times 1.0 \times 10^2}{8.85 \times 10^{-12} \times 3.00 \times 10^8}} \approx 274.57 \text{ V/m} \).
04

Calculate Maximum Magnetic Field (b)

The maximum magnetic field \( B_{max} \) is related to the maximum electric field \( E_{max} \) by \( B_{max} = \frac{E_{max}}{c} \). Using \( E_{max} = 274.57 \text{ V/m} \) and \( c = 3.00 \times 10^8 \text{ m/s} \), we find \( B_{max} = \frac{274.57}{3.00 \times 10^8} \approx 9.15 \times 10^{-7} \text{ T} \).
05

Calculate Energy Delivered Per Second to Retina (c)

The energy delivered per second (power) to the retina is the same as the calculated maximum power from Step 2. Therefore, the energy delivered per second is 0.1767 mW, which equals 0.1767 millijoules per second, since 1 watt equals 1 joule per second.
06

Convert Damage Threshold to W/cm² (d)

Convert the given intensity from W/m² to W/cm². We know that 1 m² = 10,000 cm², hence \( 1.0 \times 10^2 \text{ W/m}^2 = \frac{1.0 \times 10^2}{10,000} \text{ W/cm}^2 = 0.01 \text{ W/cm}^2 \).

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Key Concepts

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

Laser Safety
Laser safety is a critical aspect when dealing with lasers, especially in environments like laboratories and industries. Lasers produce concentrated beams of light that can be harmful, particularly to the eyes.
The damage threshold of the retina, which is the eye's sensitivity limit to laser intensity, is a key concept in laser safety. By determining the damage threshold, industries can ensure that laser devices operate within safe limits and do not cause harm to human eyes.
For instance, if a laser emits light above 100 W/m², it surpasses the damage threshold for the retina. This is when safety measures, like protective eyewear and regulated exposure times, become essential. It's crucial to ensure that the power of the laser beam remains below this threshold to avoid permanent eye damage.
Intensity Calculation
Intensity is a measure of how much power is distributed over a particular area. It is calculated as power per unit area, typically expressed in watts per square meter (W/m²).
In laser applications, understanding intensity is vital for determining whether a laser beam is safe. For example, by calculating the laser's cross-sectional area and knowing the acceptable intensity threshold, one can determine the maximum safe power output.
This is done using the formula:
  • Intensity, I = Power, P / Area, A
This calculation helps in converting units and adjusting laser setups to adhere to safety guidelines. If the calculated power exceeds the threshold when the intensity formula is applied, adjustments must be made to prevent potential hazards.
Electromagnetic Fields
Electromagnetic fields (EMFs) are fundamental to understanding how lasers work. Lasers emit coherent light that comprises electric and magnetic fields oscillating perpendicular to each other.
In the context of determining laser safety levels, we often need to calculate the maximum electric and magnetic fields a laser beam can produce. The electric field (E) primarily affects how the intensity is perceived and is directly linked to the potential energy delivered.
Using relationships like:
  • Maximum electric field, Emax = \( \sqrt{\frac{2I}{\varepsilon_0 c}} \)
  • Maximum magnetic field, Bmax = Emax / c
Where \( \varepsilon_0 \) (epsilon naught) is the permittivity of free space and \( c \) is the speed of light, we can assess the electromagnetic properties associated with a laser beam.
These calculations help in adjusting the laser systems to comply with safety standards, ensuring that neither the electric nor the magnetic fields exceed safe levels for human exposure.

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Most popular questions from this chapter

The electric field of a sinusoidal electromagnetic wave obeys the equation \(E = (375 V/m)\) cos [(1.99 \(\times\) 107 rad/m)x + (5.97 \(\times\) 10\(^{15}\) rad/s)\(t\)]. (a) What is the speed of the wave? (b) What are the amplitudes of the electric and magnetic fields of this wave? (c) What are the frequency, wavelength, and period of the wave? Is this light visible to humans?

A standing electromagnetic wave in a certain material has frequency 2.20 \(\times\) 10\(^{10}\) Hz. The nodal planes of \(\vec{B}\) are 4.65 mm apart. Find (a) the wavelength of the wave in this material; (b) the distance between adjacent nodal planes of the \(\vec{E}\) field; (c) the speed of propagation of the wave.

The microwaves in a certain microwave oven have a wavelength of 12.2 cm. (a) How wide must this oven be so that it will contain five antinodal planes of the electric field along its width in the standing-wave pattern? (b) What is the frequency of these microwaves? (c) Suppose a manufacturing error occurred and the oven was made 5.0 cm longer than specified in part (a). In this case, what would have to be the frequency of the microwaves for there still to be five antinodal planes of the electric field along the width of the oven?

Interplanetary space contains many small particles referred to as \(interplanetary\) \(dust\). Radiation pressure from the sun sets a lower limit on the size of such dust particles. To see the origin of this limit, consider a spherical dust particle of radius \(R\) and mass density \(\rho\). (a) Write an expression for the gravitational force exerted on this particle by the sun (mass \(M\)) when the particle is a distance \(r\) from the sun. (b) Let L represent the luminosity of the sun, equal to the rate at which it emits energy in electromagnetic radiation. Find the force exerted on the (totally absorbing) particle due to solar radiation pressure, remembering that the intensity of the sun's radiation also depends on the distance \(r\). The relevant area is the cross-sectional area of the particle, \(not\) the total surface area of the particle. As part of your answer, explain why this is so. (c) The mass density of a typical interplanetary dust particle is about 3000 kg/m\(^3\). Find the particle radius R such that the gravitational and radiation forces acting on the particle are equal in magnitude. The luminosity of the sun is 3.9 \(\times\) 10\(^{26}\) W. Does your answer depend on the distance of the particle from the sun? Why or why not? (d) Explain why dust particles with a radius less than that found in part (c) are unlikely to be found in the solar system. [\(Hint\): Construct the ratio of the two force expressions found in parts (a) and (b).]

An intense light source radiates uniformly in all directions. At a distance of 5.0 m from the source, the radiation pressure on a perfectly absorbing surface is 9.0 \(\times\) 10\(^{-6}\) Pa. What is the total average power output of the source?

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