Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB
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154 CHAPTER 6. DYNAMICS: ENERGY AND ...<br />
You may recall seeing an expressi<strong>on</strong> like (6.6) in some of your homework. It<br />
came up there because it gives the first few terms in the Taylor’s series expansi<strong>on</strong><br />
of the time-dilati<strong>on</strong> factor,<br />
1<br />
√<br />
1 − v2 /c = 1 + 1 v 2<br />
+ small correcti<strong>on</strong>s, (6.7)<br />
2 2 c2 a factor which has appeared in almost every equati<strong>on</strong> we have due to its c<strong>on</strong>necti<strong>on</strong><br />
to the interval <strong>and</strong> Minkowskian geometry.<br />
It is therefore natural to guess that the correct relativistic formula for the total<br />
energy of a moving object is<br />
E =<br />
m 0 c 2<br />
√<br />
1 − v2 /c 2 = m 0c 2 coshθ. (6.8)<br />
This is exactly the formula 9 that will be derived in secti<strong>on</strong> 6.6.<br />
6.4.2 Momentum <strong>and</strong> Mass<br />
Momentum is a little trickier, since we <strong>on</strong>ly have <strong>on</strong>e term in the expansi<strong>on</strong><br />
so far: p = mv + small correcti<strong>on</strong>s. Based <strong>on</strong> the analogy with energy, we<br />
expect that this is the expansi<strong>on</strong> of something native to Minkowskian geometry<br />
– probably a hyperbolic trig functi<strong>on</strong> of the boost parameter θ. Unfortunately<br />
there are at least two natural c<strong>and</strong>idates, m 0 c sinhθ <strong>and</strong> m 0 c tanhθ (which is<br />
of course just m 0 v). The detailed derivati<strong>on</strong> is given in 6.6, but it should come<br />
as no surprise that the answer is the sinhθ <strong>on</strong>e that is simpler from the point<br />
of Minkowskian geometry <strong>and</strong> which is not the Newt<strong>on</strong>ian answer. Thus the<br />
relativistic formula for momentum is:<br />
p =<br />
m 0 v<br />
√<br />
1 − v2 /c 2 = m 0c sinhθ. (6.9)<br />
If you d<strong>on</strong>’t really know what momentum is, d<strong>on</strong>’t worry too much about it.<br />
We will <strong>on</strong>ly touch <strong>on</strong> momentum briefly <strong>and</strong> the brief introducti<strong>on</strong> in secti<strong>on</strong><br />
6.2.2 should suffice. I should menti<strong>on</strong>, however, that the relativistic formulas for<br />
energy <strong>and</strong> momentum are very important for things you encounter everyday –<br />
like high resoluti<strong>on</strong> computer graphics! The light from your computer m<strong>on</strong>itor 10<br />
is generated by electr<strong>on</strong>s traveling at 10 − 20% of the speed of light <strong>and</strong> then<br />
hitting the screen. This is fast enough that, if engineers did not take into<br />
account the relativistic formula for momentum <strong>and</strong> tried to use just p = mv,<br />
the electr<strong>on</strong>s would not l<strong>and</strong> at the right places <strong>on</strong> the screen <strong>and</strong> the image<br />
would be all screwed up. There are some calculati<strong>on</strong>s about this in homework<br />
problem (5).<br />
9 The old c<strong>on</strong>venti<strong>on</strong> that you will see in some books (but not in my class!!) is to define<br />
m<br />
a ‘velocity-dependent mass’ m(v) through m(v) = √ 0<br />
= 1−v 2 /c 2 E/c2 . This is an outdated<br />
c<strong>on</strong>venti<strong>on</strong> <strong>and</strong> does not c<strong>on</strong>form to the modern use of the term ‘mass.’<br />
10 So l<strong>on</strong>g as it is not an LCD display.