Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

A light detector (your eye) has an area of 2.00×10-6m2and absorbs 80% of the incident light, which is at wavelength 500 nm. The detector faces an isotropic source, 3.00 m from the source. If the detector absorbs photons at the rate of exactly4.000s-1at what power does the emitter emit light?

Short Answer

Expert verified

The emitter emits power 1.1×10-10W.

Step by step solution

01

Describe the expression of energy of the photon

The energy Eof a photon of wavelength λ is given by,

E=hcλ ……. (1)

Here, h is Planck’s constant, and c is the speed of light.

02

Determine the power that emitter emit

Let Remitbe the photon emission rate, then the absorption rate Rabs=4.00s-1in terms of the area of the eye Aabs=2.00×10-6m2

Rabs=PabsEp

Since the detector absorbs only of the incident light, then the absorbed power is,

Pabs=80100IAabsRabsEp=0.8PemitAemitAabsPemit=RabsEp0.84πr2Aabs....(2)

Substitute the below values in eq. 1

λ=500nm.h=6.626×10-34J.sc=3×108m/s

Ep=6.626×10-34J.s3×108m/s500nm=6.626×10-34J.s3×108m/s500nm1m109nm=3.93×10-19J.

Substitute the below values in eq. 2.

Rabs=4.00s-1Ep=3.93×10-19J.Aabs=2.00×10-6m2r=3m

Pemit=4.00s-13.93×10-19J0.84π3m22.00×10-6m2=1.1×10-10W

Therefore, the emitter emits power 1.1×10-10W.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

The Sun is approximately an ideal blackbody radiator with surface temperature of 5800 K.

(a) Find the wavelength at which its spectral radiancy is maximum and

(b) identify the type of magnetic wave corresponding to that wavelength.

(c) As we shall discuss in chapter 44, the universe is approximately an ideal blackbody radiator with radiation emitted when atoms first formed. Today the spectral radiancy of that radiation peaks at a wavelength of 1.06 mm (in the microwave region). What is the corresponding temperature of the universe?

What is the maximum wavelength shift for a Compton collision between a photon and a free photon?

Question: You will find in Chapter 39 that electrons cannot move in definite orbits within atoms, like the planets in our solar system. To see why, let us try to “observe” such an orbiting electron by using a light microscope to measure the electron’s presumed orbital position with a precision of, say, 10pm(a typical atom has a radius of about localid="1663132292844" 100pm). The wavelength of the light used in the microscope must then be about 10pm. (a) What would be the photon energy of this light? (b) How much energy would such a photon impart to an electron in a head-on collision? (c) What do these results tell you about the possibility of “viewing” an atomic electron at two or more points along its presumed orbital path? (Hint:The outer electrons of atomsare bound to the atom by energies of only a few electron-volts.)

Derive Eq. 38-11, the equation for the Compton shift, from Eqs. 38-8, 38-9, and 38-10 by eliminating v and θ.

A stream of protons, each with a speed of0.9900c, are directed into a two-slit experiment where the slit separation is 4.00×10-9m. A two-slit interference pattern is built up on the viewing screen. What is the angle between the center of the pattern and the second minimum (to either side of the center)?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free