Relativistic Kinetic Energy Derivation

In summary, jtbell's work provides a derivation for relativistic kinetic energy, but he cannot figure out why equation 1 does not equal equation 2. He is using relativistic p, which is the relativistic momentum, and he assumes that the kE imparted on an object is 1/2E when the reference frame is independent of the Object and the object or whatever that imparted the energy onto the Object, and thus half the energy is imparted on the object and half is imparted equally and oppositely on the "whatever object". jtbell is looking into writing in Latex.
  • #1
PCB
20
0
Hello,
I tried a different route to derive relativistic kinetic energy and I cannot see why it doesn't work. Here is my work:
8.00000000000000E+01 RM, Rest mass of object
7.50000000000000E+05 v, velocity of object
6.00001877636573E+07 Momentum, p,= RM/Sqrt(1-(v^2/c^2))*v
4.50001408227429E+13 Energy= p*v = RM/Sqrt(1-(v^2/c^2))*v^2 equation 1

4.50002112348160E+13 kE= 2*((RM/Sqrt(1-(v^2/c^2))*c^2)-(RM*c^2)) equation 2
My question is, why doesn't equation 1 yield the same quantity as equation 2?
 
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  • #2
What units are you using? When you say ##v=7.5\times{10}^5## I'm assuming that is not in nanofurlongs per megafortnight... But it would be nice to know what units you are using if only so we know what value to use for ##c##.

Does your equation 2 have an extraneous factor of two? It looks like ##E_k=2(m_0c^2/\sqrt{1-v^2/c^2}-m_0c^2)##... Posts are much easier to read, and you'll get better answers, if you use Latex. To see how I did that, reply to this post and look at the quoted text.

And finally, did you actually calculate those two values or did you just key them into a calculator? The latter technique can easily introduce and magnify rounding errors.
 
  • #3
PCB said:
Energy= p*v

That doesn't look like any formula for relativistic energy that I know of, either for total energy or kinetic energy. Where did you get it?
 
  • #4
Nugatory,
The units I am using are kg, meters, seconds. Specifically, v = 750,000 m/s and 299,790,000 m/s for c.
I will look into writing in Latex. I write in "Excel" presently. Because I do not trust my algebra, I calculate with real numbers so I can check the calculations.

jtbell,
I didn't get equation 1 from anywhere specifically, I am trying to derive relativistic kE by this particular route.
 
  • #5
PCB said:
Energy= p*v=

jtbell said:
That doesn't look like any formula for relativistic energy that I know of, either for total energy or kinetic energy. Where did you get it?

PCB said:
jtbell,
I didn't get equation 1 from anywhere specifically, I am trying to derive relativistic kE by this particular route.

Try
##K=\int{v\ dp}##
 
  • #6
Thanks robphy. I am aware of several different derivations of relativistic kE, but I am trying to find out why my derivation does not work
 
  • #7
My point was, more explicitly, what made you think E = pv might work? robphy's ##K = \int {vdp}## does give ##K=\frac{1}{2}mv^2## in classical (non-relativistic) mechanics, but that equals ##K=\frac{1}{2}pv## not ##K=pv##. And then there's the difference between [total] energy (your equation 1) and kinetic energy (your equation 2)... unless that was just a typo on your part.
 
  • #8
robphy said:
Try
##K=\int{v\ dp}##

If p is the relativistic momentum,
you get the relativistic kinetic energy.
 
  • #9
jtbell,
First of all, thank you for your response(s).
I think E=pv might work because I am using relativistic p, meaning m/gamma*v. (Sorry, I haven't figured out LaTex yet).
Concerning the extraneous 2, I am assuming that the kE imparted on an object is 1/2E when the reference frame is independent of the Object and the object or whatever that imparted the energy onto the Object, and thus half the energy is imparted on the object and half is imparted equally and oppositely on the "whatever object". I am assuming the reference frame of the "whatever object" which means 100% of the energy is imparted onto the Object.
 
  • #10
robphy,
I post above was made just as you added to your latest post.
Yes, p is relativistic momentum, as can be seen in the equation 1. Thus my problem--I cannot figure out why my equation 1 doesn't equal equation 2.
 
  • #11
robphy said:
Try
##K=\int{v\ dp}##

This is integrates to ##(\gamma-1)m##.
 
  • #12
robphy,
Yes, it integrates into equation 2.
 
  • #13
##K=\int{v\ dp}##, which is not equal to your Eq.1,
does integrate to twice your Eq. 2.

Added in edit: Note that in the integrand, v is not the "final" velocity.

Added in edit: I didn't see that extra factor of 2. I just went on what you said.
 
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  • #14
Yes I know. Your equation is equivalent to my equation 2.
The p in my equation 1 is relativistic momentum, thus (I think) equation 1 should equal equation 2.
 
  • #15
[itex]K=\int_0^{p_f} v(p)\ dp=m\left(\frac{1}{\sqrt{1-v_f^2}}-1\right)\quad \neq\quad v_f p_f = v_f \left(mv_f\frac{1}{\sqrt{1-v_f^2}}\right)[/itex]
 
  • #16
PCB said:
The p in my equation 1 is relativistic momentum, thus (I think) equation 1 should equal equation 2.
Even if ##p## is relativistic momentum, ##p=\gamma{m_0}##, neither total nor kinetic energy is given by ##pv##. However, when ##p## is the classical momentum, ##pv## is twice the classical kinetic energy.

Meanwhile, your equation 2 is the correct expression for twice (because of that extraneous factor of two) the relativistic kinetic energy.

Finally, the speed value you're using, ##7.5\times{10}^5## m/sec, is only about .2% of the speed of light so relativistic effects are going to be very small. Thus equation 1 is wrong for the classical kinetic energy but not by much... All you've discovered is that when the speed is small compared with the speed of light, the correct relativistic value of the kinetic energy (equation 2) doesn't differ much from the classical kinetic energy, whether computed correctly (##E_k=pv/2=mv^2/2##) or using your incorrect (if ##p## is relativistic momentum) equation one. And that's why you have to look out to six decimal places to see a difference between the two.
 
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  • #17
The most simple derivation of the expression for relativistic kinetic energy is through Hamilton's principle. The only scalar action you can built from ##\dot{\vec{x}}## alone is given by
$$S[\vec{x}]=-m c^2 \int \mathrm{d} t \sqrt{1-\dot{\vec{x}^2/c^2}}.$$
Energy, by definition is the conserved quantity due to time-translation invariance according to Noether's theorem, and that's the Hamilton function
$$H=\vec{p} \cdot \dot{\vec{x}}-L$$
with the canonical momentum
$$\vec{p}=\frac{\partial L}{\partial \dot{\vec{x}}}=m \frac{\dot{\vec{x}}}{\sqrt{1-\dot{\vec{x}}^2/c^2}},$$
leading to
$$E=H=\frac{m c^2}{\sqrt{1-\dot{\vec{x}}^2/c^2}}.$$
The momentum due to Noether's theorem is the canonical momentum and thus four-momentum
$$(p^{\mu})=(E/c,\vec{p})=\frac{m}{\sqrt{1-\dot{\vec{x}}^2/c^2}}(c,\dot{\vec{x}}).$$
This leads to
$$p_{\mu} p^{\mu}=\frac{m^2}{1-\dot{\vec{x}}^2/c^2}(c^2-\dot{\vec{x}}^2)=m^2 c^2,$$
identifying ##m## with the invariant mass.
 
  • #18
Thanks vanhees71 but you have missed my point in that I am trying to fin why my derivation is wrong.
And thanks Nugatory. I know there is a difference between classical and relativistic P and kE etc... What I am trying to do is relativise the classic formula which is why I am using gamma. You say my equation 1 is wrong, and I agree, I agreed in my original post. Thus I come back to asking why it is wrong. I am asking why equation 1 does not equal equation 2. It cannot be pure chance they are very close.
 
  • #19
PCB said:
Thus I come back to asking why it is wrong. I am asking why equation 1 does not equal equation 2. It cannot be pure chance they are very close.

So, we agree that your expression 1 ( ##m \gamma v^2## ) is not the expression for relativistic kinetic energy.
So, we agree that your expression 2 ( ##2m(\gamma -1)## ) is not the expression for relativistic kinetic energy [it is actually twice the relativistic kinetic energy].

Note that your velocity is small compared to c (that is, ##v/c\ll 1##)
The Taylor expansion of the "difference between your equation 2 and equation 1" has a leading term of order ##(v/c)^4##, which is very tiny
[tex]\frac{v^4}{4}+\frac{v^6}{4}+\frac{15}{64} v^8+O(v^{10})[/tex]
http://www.wolframalpha.com/input/?i=series(2*(1/sqrt(1-v^2)-1)-v^2/sqrt(1-v^2)))

So, in conclusion, your two expressions (neither of which is the relativistic energy) agree to order ##(v/c)^4## for small ##(v/c)##.
 
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  • #20
PCB said:
What I am trying to do is relativise the classic formula which is why I am using gamma.

You can't "relativise" a classical formula just by plugging in ##\gamma## in various places. That's not a valid method, so it's not surprising that it gives you a wrong answer. The reason the answer is still close for ##v \ll c## is simply that ##2 \left( \gamma - 1 \right)## is very close to ##\gamma v^2##, so your incorrect formula just happens to be very close to the correct formula.
 
  • #21
PCB said:
Thus I come back to asking why it is wrong. I am asking why equation 1 does not equal equation 2. It cannot be pure chance they are very close.

It's not pure chance that they're so close - they are so close because you chose a value for ##v## that is small compared with the speed of light so ##v/c## is small; because the error in equation one is more or less proportional to ##v/c## a small value of ##v/c## means a small error in the results.

And as for why equation 1 is wrong: @robphy already answered that in post #15 of this thread. and as PeterDonis saud just above, there's no reason to assume that plugging the odd ##\gamma## into a classical equation will give you a valid relativistic equation. Sometimes it works (as it does for momentum: ##p=\gamma{m}_0v##) but when it does it's just luck - there's no substitute for doing the math as robphy did above.
 
  • #22
robphy said:
If p is the relativistic momentum,
you get the relativistic kinetic energy.

Wait, is that right?

I know that classical momentum is the velocity-derivative of classical kinetic energy, but I'm not getting the same results when I differentiate relativistic kinetic energy with respect to velocity. For the relativistic case, I get ##\gamma^3m\mathbf v##, whereas relativistic momentum is ##\gamma m \mathbf v##.

But then again, my calculus isn't so good.
 
  • #23
Oh, I think I read what you wrote backwards. (Got the v and p swapped.) Sorry.
 

What is relativistic kinetic energy?

Relativistic kinetic energy is the energy an object possesses due to its motion, taking into account the effects of special relativity. It is an extension of classical kinetic energy, which only applies to objects moving at non-relativistic speeds.

How is relativistic kinetic energy derived?

The derivation of relativistic kinetic energy involves using the principles of special relativity, such as time dilation and length contraction, to modify the classical kinetic energy equation. This results in the famous equation E = mc^2, where E is the relativistic kinetic energy, m is the mass of the object, and c is the speed of light.

What is the difference between classical and relativistic kinetic energy?

The main difference between classical and relativistic kinetic energy is that the latter takes into account the effects of special relativity, such as time dilation and length contraction, which become significant at high speeds. This means that the relativistic kinetic energy of an object will be greater than its classical kinetic energy at high speeds.

Is relativistic kinetic energy important in everyday life?

Relativistic kinetic energy is not typically relevant in everyday life, as most objects we encounter move at non-relativistic speeds. However, it is crucial in fields such as particle physics and astronomy, where objects can reach speeds close to the speed of light and the principles of special relativity must be considered.

What are some practical applications of relativistic kinetic energy?

Some practical applications of relativistic kinetic energy include particle accelerators, where particles are accelerated to high speeds and their relativistic kinetic energy is used to create new particles and study their behavior. Additionally, the energy released in nuclear reactions is also an example of relativistic kinetic energy at work.

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