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Go outside in the sunlight and observe your shadow. It has fuzzy edges even if you do not. Is this a diffraction effect? Explain.

Short Answer

Expert verified

It's not a diffraction effect, no.

Step by step solution

01

Concept Introduction

A shadow is a dark region created by an opaque object blocking light from a light source. It takes up the entire three-dimensional volume behind a light-emitting device.

02

Explanation

It does not represent diffraction since various portions of the sun make distinct shadows.

Light converges or overlaps and forms dark or less dark shadows, similar to how waves converge or overlap.

A dark route will be generated when the shadows overlap and a fuzzy path will be created where they do not overlap.

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Most popular questions from this chapter

Figure 27.56shows a double slit located a distance xfrom a screen, with the distance from the center of the screen given by y. When the distance dbetween the slits is relatively large, there will be numerous bright spots, called fringes. Show that, for small angles (where sinฮธโ‰ˆฮธ, with ฮธ in radians), the distance between fringes is given by โˆ†y=xฮป/d.

Find the angle for the third-order maximum for 580-nm-wavelength yellow light falling on a diffraction grating having 1500 lines per centimeter.

(a) What is the smallest separation between two slits that will produce a second-order maximum for any visible light? (b) For all visible light?

What is the highest-order maximum for 400-nm light falling on double slits separated by 25.0 ยตm?

The \(300 - m\)-diameter Arecibo radio telescope pictured in Figure \(27.28\) detects radio waves with a \(4.00{\rm{ }}cm\) average wavelength.

(a) What is the angle between two just-resolvable point sources for this telescope?

(b) How close together could these point sources be at the \({\rm{2}}\) million light year distance of the Andromeda galaxy?

Figure \(27.28\) A \(305 - m\)-diameter natural bowl at Arecibo in Puerto Rico is lined with reflective material, making it into a radio telescope. It is the largest curved focusing dish in the world. Although \(D\) for Arecibo is much larger than for the Hubble Telescope, it detects much longer wavelength radiation and its difdfraction limit is significantly poorer than Hubble's. Arecibo is still very useful, because important information is carried by radio waves that is not carried by visible light. (credit: Tatyana Temirbulatova, Flickr)

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