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Problem 1 Problem 2 Problem 3 Problem 4 Problem 5 Problem 6 Problem 7 Problem 8 Problem 9 Problem 10 Problem 11 Problem 12 Problem 13 Problem 14 Problem 15 Problem 16 Problem 17 Problem 18 Problem 19 Problem 20 Problem 21 Problem 22 Problem 23 Problem 24 Problem 25 Problem 26 Problem 27 Problem 28 Problem 29 Problem 30 Problem 31 Problem 32 Problem 33 Problem 34 Problem 35 Problem 36 Problem 37 Problem 38 Problem 39 Problem 40 Problem 41 Problem 42 Problem 43 Problem 44 Problem 45 Problem 46 Problem 47 Problem 48 Problem 49 Problem 50 Problem 51 Problem 52 Problem 53 Problem 54 Problem 55 Problem 56 Problem 57 Problem 58 Problem 59 Problem 60 Problem 61 Problem 62 Problem 63 Problem 64 Problem 65 Problem 66

Problem 46 Easy Difficulty

In the theory of relativity, the energy of a particle is
$$E=\sqrt{m_{0}^{2} c^{4}+h^{2} c^{2} / \lambda^{2}}$$
where $m_{0}$ is the rest mass of the particle, $\lambda$ is its wave
length, and $h$ is Planck's constant. Sketch the graph of $E$ as
a function of $\lambda .$ What does the graph say about the energy?

Answer

$E=\sqrt{m_{0}^{2} c^{4}+h^{2} c^{2} / \lambda^{2}}$

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Calculus 1 / AB

Essential Calculus Early Transcendentals

Chapter 4

APPLICATIONS OF DIFFERENTIATION

Section 4

Curve Sketching

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Problem 46
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Problem 48
Problem 49
Problem 50
Problem 51
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Problem 53
Problem 54
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Video Transcript

So here in this equation we have f is a function of, um Lando. All right, so this is wave link. Um, the mass of the particle at rest. Speed of light. Planck's constant and wavelength, so really are variable is buidling Orland. Okay, so the domain here, um, let's make this a little smaller to fit everything. The domain here is gonna be X has to be positive. So X is gonna have to be greater than zero. And why is that? Because wavelength has to be positive because it's, you know, measuring wavelengths. Okay, so there are no points of intersection, but we do have asked him to. It's so vertical. Ask them to, um we can see because of the Lambda here. Dividing by zero. Can't do that. So, vertical ass in two we're gonna see at Lambda equals zero. Okay? And now we're gonna find the horizontal Lassen totes by looking as the limit. Right? Says limit as X approaches infinity over function. So off of Lambda. Let me see that it's gonna turn out to be. And that wrist see, C squared. All right, so I'm sorry. My bed. So here is not exits. Not our, um, variable. It's Linda. Great. So here we have a horizontal ask himto e equals and at rest, see X squared. All right. And now we know that half of Lando is going to be decreasing. Unstow ming, so it's decreasing. All right, so now if we look at the graph, this is Lando, and this is energy or f of lambda. We know that we haven't asked himto a x equal Lambda equals zero, which is here. And we know we have another ask himto at e equals e equals and initial C squared. And now we don't know what that is. What this is exactly. Because, for example, we know that, um, c squared is a constant speed of light squared. Um, but, um ah, and the mess initially, we're gonna have to, you know, gain that in another way. But let's just say that it's somewhere around here. So let's say that this is e equals and that wrist C squared. All right, so it's somewhere there, and we know that it's always decreasing or function is always decreasing over are doing. And it'll proto been on touch asthma, toots. So we can see that this is an inverse relationship. It's Enver Energy and, um, wavelength are inversely proportional meaning as energy as well as energy increases are as energy energy decreases as wavelength increases.

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James Stewart

Essential Calculus Early Transcendentals

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