Elastic collision between ball and block

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SUMMARY

The discussion centers on analyzing an elastic collision between a block of mass M and a ball of mass m, where M >> m. The block slides towards a wall with initial speed V0, colliding elastically with the ball, which is initially at rest. Key equations derived include the velocities after collision: V1 = (M-m)/(M+m) V0 and v1 = (2M/(M+m)) V0. The participants explore the distance of closest approach of the block to the wall and the number of bounces the ball makes off the block before this occurs, utilizing conservation of momentum and the law of restitution.

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  • #31
Try converting your expression for Ln (Post #3) into a differential equation dL/dn.
 
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  • #32
dauto said:
Try converting your expression for Ln (Post #3) into a differential equation dL/dn.

OK. I could transform it into something like this:

\dfrac{dL}{dn} = \left( \dfrac{-2 \mu P }{p} \right) L

I followed a similar approach to find p(n) and got

p = 2mv_0 \sin (2 \sqrt{\mu}n)

If I plug the values for P and p in the DE, I get

\dfrac{dL}{L} = \dfrac{-\cos(2\sqrt{\mu}n)}{\sin(2\sqrt{\mu}n)} dn

Integrating both sides,

\log L = \dfrac{-1}{2 \sqrt{\mu}} \log \left( \sin 2 \sqrt{\mu} n \right) + c

For n=0, L=L. But then the logarithmic term tends to infinity. What's wrong here?
 
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  • #33
I'm getting

(1/L) dL/dn = -2P/(P+p/μ).

Try integrating that instead.
 
  • #34
dauto said:
I'm getting

(1/L) dL/dn = -2P/(P+p/μ).

Try integrating that instead.

But if you further approximate it, you will arrive at the same equation as mine.
 
  • #35
dauto said:
I'm getting

(1/L) dL/dn = -2P/(P+p/μ).

Try integrating that instead.

\dfrac{dL}{L} = \dfrac{-2 \cos \lambda n}{\cos \lambda n + 2 \sin \lambda n} dn \\<br /> \lambda = 2 \sqrt{\mu}

Assuming sinλn = t, the RHS transforms to

\dfrac{-2}{\lambda (\sqrt{1-t^2}+2t)} dt

I'm stuck here. Please help.
 
  • #36
utkarshakash said:
\dfrac{dL}{L} = \dfrac{-2 \cos \lambda n}{\cos \lambda n + 2 \sin \lambda n} dn \\<br /> \lambda = 2 \sqrt{\mu}

I'm getting
\dfrac{dL}{L} = \dfrac{-2 \cos \lambda n}{\cos \lambda n + \mu^{-1/2} \sin \lambda n} dn
 
  • #37
dauto said:
I'm getting
\dfrac{dL}{L} = \dfrac{-2 \cos \lambda n}{\cos \lambda n + \mu^{-1/2} \sin \lambda n} dn

I'm posting my solution step-by-step.

\dfrac{dL}{L} = \dfrac{-2 Mv_0 \cos \lambda n}{Mv_0 \cos \lambda n + (2 mv_0/ \mu) \sin \lambda n} dn

If I substitute the value of μ, I get my equation. What's wrong with it?
 
  • #38
I don't think that's correct either. I'll have to go now. I'll have more time later today
 
  • #39
dauto said:
I don't think that's correct either. I'll have to go now. I'll have more time later today

OK. Please take your time.
 
  • #40
OK. Here's what I got

Li+1=Li(1−2Vi/(Vii+v))

(1/L) dL/dn = -2V/(V+v)

(1/L) dL/dn = -2P/(P+p/μ)

(1/L) dL/dn = -2cos(λn)/[cos(λn)+μ1/2sin(λn)/μ]

(1/L) dL/dn = -2cos(λn)/[cos(λn)+μ-1/2sin(λn)],

where I used

P=P0cos(λn)

and

p=μ1/2P0sin(λn)
 
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  • #41
dauto said:
OK. Here's what I got

Li+1=Li(1−2Vi/(Vii+v))

(1/L) dL/dn = -2V/(V+v)

(1/L) dL/dn = -2P/(P+p/μ)

(1/L) dL/dn = -2cos(λn)/[cos(λn)+μ1/2sin(λn)/μ]

(1/L) dL/dn = -2cos(λn)/[cos(λn)+μ-1/2sin(λn)],

where I used

P=P0cos(λn)

and

p=μ1/2P0sin(λn)


Looks like there was a mistake in my equation for p(n). OK, how do you integrate it then? Substitutions aren't working here. What else should I try?
 
  • #42
Here's the trick

\frac{cos\theta}{cos\theta+A sin\theta} = \frac{cos\theta}{cos\theta+A sin\theta} +\xi -\xi,
where \xi is to be chosen later to our own convenience.
\frac{cos\theta d\theta}{cos\theta+A sin\theta} = \frac{[(1+\xi)cos\theta+\xi A sin\theta]d\theta}{cos\theta+A sin\theta} -\xi d\theta,
We are planning on making the change of variables
u=cos\theta+A sin\theta, and du=(-sin\theta+A cos\theta)d\theta,
So we want to chose \xi in such a way that the numerator [(1+\xi)cos\theta+\xi A sin\theta]d\theta is proportional to du
[(1+\xi)cos\theta+\xi A sin\theta]d\theta = \eta du = \eta (-sin\theta+A cos\theta)d\theta which gives us two equations
(1+\xi) = \eta A and
\xi A = - \eta The set is easily solved to \xi = -\frac{1}{1+A^2} and \eta=\frac{A}{1+A^2}. Now that we know what \xi and \eta are, we have
\frac{cos\theta d\theta}{cos\theta+A sin\theta} = \frac{[(1+\xi)cos\theta+\xi A sin\theta]d\theta}{cos\theta+A sin\theta} -\xi d\theta = \frac{\eta du}{u} - \xi d\theta.
Integration now is a trivial matter.
 
  • #43
dauto said:
Here's the trick

\frac{cos\theta}{cos\theta+A sin\theta} = \frac{cos\theta}{cos\theta+A sin\theta} +\xi -\xi,
where \xi is to be chosen later to our own convenience.
\frac{cos\theta d\theta}{cos\theta+A sin\theta} = \frac{[(1+\xi)cos\theta+\xi A sin\theta]d\theta}{cos\theta+A sin\theta} -\xi d\theta,
We are planning on making the change of variables
u=cos\theta+A sin\theta, and du=(-sin\theta+A cos\theta)d\theta,
So we want to chose \xi in such a way that the numerator [(1+\xi)cos\theta+\xi A sin\theta]d\theta is proportional to du
[(1+\xi)cos\theta+\xi A sin\theta]d\theta = \eta du = \eta (-sin\theta+A cos\theta)d\theta which gives us two equations
(1+\xi) = \eta A and
\xi A = - \eta The set is easily solved to \xi = -\frac{1}{1+A^2} and \eta=\frac{A}{1+A^2}. Now that we know what \xi and \eta are, we have
\frac{cos\theta d\theta}{cos\theta+A sin\theta} = \frac{[(1+\xi)cos\theta+\xi A sin\theta]d\theta}{cos\theta+A sin\theta} -\xi d\theta = \frac{\eta du}{u} - \xi d\theta.
Integration now is a trivial matter.


Integrating the equation I get

\log L = \left( \dfrac{A}{1+A^2} \log (\cos \theta + A \sin \theta) + \dfrac{\theta}{1+A^2} \right) (-2) + \log L_0

Substituting n=\frac{\pi}{4 \sqrt{\mu}}

\log L = \dfrac{\sqrt{\mu}}{1+\mu} \log \mu - \dfrac{\mu \pi}{1+\mu} + \log L_0

But this is not even close to the correct answer. :cry: Are you getting the same result?
 
  • #44
utkarshakash said:
Integrating the equation I get

\log L = \left( \dfrac{A}{1+A^2} \log (\cos \theta + A \sin \theta) + \dfrac{\theta}{1+A^2} \right) (-2) + \log L_0

Substituting n=\frac{\pi}{4 \sqrt{\mu}}

\log L = \dfrac{\sqrt{\mu}}{1+\mu} \log \mu - \dfrac{\mu \pi}{1+\mu} + \log L_0

But this is not even close to the correct answer. :cry: Are you getting the same result?

I got

log (L/L_0) =-\left[\frac{log [\mu^{1/2}cos\theta +sin\theta] + \mu^{1/2}\theta}{1+\mu} \right]_{\theta=0}^{\pi/2}

What do you think the correct answer should be?
 
  • #45
dauto said:
I got

log (L/L_0) =-\left[\frac{log [\mu^{1/2}cos\theta +sin\theta] + \mu^{1/2}\theta}{1+\mu} \right]_{\theta=0}^{\pi/2}

What do you think the correct answer should be?

The correct answer is L0 √μ. Your equation seems to give a different answer.
 
  • #46
utkarshakash said:
The correct answer is L0 √μ. Your equation seems to give a different answer.

Look closely. There are a couple of terms that are negligible. One of the terms in the numerator may be dropped. And the term μ1/2 in the numerator is also negligible. It simplifies as

log (L/L_0) =-\left[log [\mu^{1/2}cos\theta +sin\theta] \right]_{\theta=0}^{\pi/2}

Do you see it now?
 
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  • #47
Here is another approach to part (a). In post #3 you have $$L_{i+1} = \frac{v_i-V_i}{v_i+V_i}L_i$$
So, in particular,

$$L_2 = \frac{v_1-V_1}{v_1+V_1}L_1$$ and $$L_3= \frac{v_2-V_2}{v_2+V_2}L_2 = \frac{v_2-V_2}{v_2+V_2} \frac{v_1-V_1}{v_1+V_1}L_1$$

For an elastic collision, the relative speed of approach before the collision equals the relative speed of separation after the collision.

For example, at the first collision

## V_0 =v1-V_1 ##, which means ##L_2 = \frac{V_0}{v_1+V_1}L_1##

For the second collision

##v_1+V_1=v2-V_2 ## which can be used to show ##L_3= \frac{V_0}{v_2+V_2}L_1##.

Generalize this to write ##L_N## in terms of ##L_1, v_{N-1}, V_{N-1}## and ##V_0##.

See if you can apply this to the case where ##\small N -1## is the index of the collision for which ##\small M## essentially comes to rest.
 
  • #48
This is an intriguing question. I wasn't sure what approximation would be reasonable, so I set out to solve it exactly to start with - looks like I did what TSny suggests. I took un, vn to be the speeds, to the right, of M, m respectively, just before each time they collide (so the vn are negative). I got ##\left[\stackrel{u_n}{v_n}\right] = \left(\frac{M-m}{M+m}\right)^nPD^nP^{-1}\left[^u_0\right]##, where u is the initial speed of M, and PDP-1 is the diagonalisation of ##A = \left[\begin{array}{cc} 1 & b \\ a & 1 \end{array} \right]##, ##a = \frac{2m}{M-m}##, ##b = -\frac{2M}{M-m}##. For un = 0, this gave
##(1+\sqrt{ab})^n = -(1-\sqrt{ab})^n##. (Note that b is negative.) I.e. ##n = \frac{i \pi}{\ln(\frac{1+i\mu}{1-i\mu})}##, where ##\mu = \frac{2\sqrt{Mm}}{M-m}##. For M>>m this reduces to ##n = \frac{\pi}{4}\sqrt{\frac Mm}##.
I'm sure this was all a lot harder than picking the right approximation up front, but it was interesting.
Applying the same approach to the distance, I got this dreadful formula, where xn is the remaining distance at the nth collision:
##x_{n+1} = x_n\frac{(1+i\rho)^n(1-i\alpha)-(1-i\rho)^n(1+i\alpha)}{(1+i\rho)^n(1+i\alpha)-(1-i\rho)^n(1-i\alpha)}##, where ##\rho = 2\frac{\sqrt{Mm}}{M-m}, \alpha = \sqrt{\frac mM}##.
For M>>m, ##\rho ≈ 2\alpha << 1##, reducing it to ##\frac{\tan(2n\alpha)-\alpha}{\tan(2n\alpha)+\alpha}##, further approximating to ##\frac{2n-1}{2n+1}##. Thus xn ≈ x1/(2n-1). Does that give the right answer?
 
  • #49
dauto said:
Look closely. There are a couple of terms that are negligible. One of the terms in the numerator may be dropped. And the term μ1/2 in the numerator is also negligible. It simplifies as

log (L/L_0) =-\left[log [\mu^{1/2}cos\theta +sin\theta] \right]_{\theta=0}^{\pi/2}

Do you see it now?

Yes. I got the correct answer. Thanks for helping ! :smile:
 
  • #50
haruspex said:
This is an intriguing question. I wasn't sure what approximation would be reasonable, so I set out to solve it exactly to start with - looks like I did what TSny suggests. I took un, vn to be the speeds, to the right, of M, m respectively, just before each time they collide (so the vn are negative). I got ##\left[\stackrel{u_n}{v_n}\right] = \left(\frac{M-m}{M+m}\right)^nPD^nP^{-1}\left[^u_0\right]##, where u is the initial speed of M, and PDP-1 is the diagonalisation of ##A = \left[\begin{array}{cc} 1 & b \\ a & 1 \end{array} \right]##, ##a = \frac{2m}{M-m}##, ##b = -\frac{2M}{M-m}##. For un = 0, this gave
##(1+\sqrt{ab})^n = -(1-\sqrt{ab})^n##. (Note that b is negative.) I.e. ##n = \frac{i \pi}{\ln(\frac{1+i\mu}{1-i\mu})}##, where ##\mu = \frac{2\sqrt{Mm}}{M-m}##. For M>>m this reduces to ##n = \frac{\pi}{4}\sqrt{\frac Mm}##.
I'm sure this was all a lot harder than picking the right approximation up front, but it was interesting.
Applying the same approach to the distance, I got this dreadful formula, where xn is the remaining distance at the nth collision:
##x_{n+1} = x_n\frac{(1+i\rho)^n(1-i\alpha)-(1-i\rho)^n(1+i\alpha)}{(1+i\rho)^n(1+i\alpha)-(1-i\rho)^n(1-i\alpha)}##, where ##\rho = 2\frac{\sqrt{Mm}}{M-m}, \alpha = \sqrt{\frac mM}##.
For M>>m, ##\rho ≈ 2\alpha << 1##, reducing it to ##\frac{\tan(2n\alpha)-\alpha}{\tan(2n\alpha)+\alpha}##, further approximating to ##\frac{2n-1}{2n+1}##. Thus xn ≈ x1/(2n-1). Does that give the right answer?

This was indeed a difficult problem, much difficult than what I assumed. Lots of approximations are required. Your method seems complicated to me. But, anyways, thanks for posting your solution. Knowing different methods to solve a problem is certainly beneficial.
 
  • #51
Using the fact that the relative speed of approach equals the relative speed of separation at each collision, you can iterate ##L_{i+1} = \frac{v_i-V_i}{v_i+V_i}L_i## to get

##L_{N+1} = \frac{V_0}{v_N+V_N}L_1##.

Suppose ##\small M## essentially comes to rest at the ##\small N^{th}## collision. Then to a good approximation

##L_{N+1} = L_{N} = L_{closest}## and ##V_{N}=0##. So,

##L_{closest} = \frac{V_0}{v_N}L_1##. Conservation of energy implies ##\frac{1}{2}MV_0^2 = \frac{1}{2}mv_N^2##. So, ##L_{closest} = \sqrt{\frac{m}{M}}L_1##
 
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  • #52
TSny said:
Using the fact that the relative speed of approach equals the relative speed of separation at each collision, you can iterate ##L_{i+1} = \frac{v_i-V_i}{v_i+V_i}L_i## to get

##L_{N+1} = \frac{V_0}{v_N+V_N}L_1##.

Suppose ##\small M## essentially comes to rest at the ##\small N^{th}## collision. Then to a good approximation

##L_{N+1} = L_{N} = L_{closest}## and ##V_{N}=0##. So,

##L_{closest} = \frac{V_0}{v_N}L_1##. Conservation of energy implies ##\frac{1}{2}MV_0^2 = \frac{1}{2}mv_N^2##. So, ##L_{closest} = \sqrt{\frac{m}{M}}L_1##
Brilliant.
 
  • #53
TSny said:
Using the fact that the relative speed of approach equals the relative speed of separation at each collision, you can iterate ##L_{i+1} = \frac{v_i-V_i}{v_i+V_i}L_i## to get

##L_{N+1} = \frac{V_0}{v_N+V_N}L_1##.

Suppose ##\small M## essentially comes to rest at the ##\small N^{th}## collision. Then to a good approximation

##L_{N+1} = L_{N} = L_{closest}## and ##V_{N}=0##. So,

##L_{closest} = \frac{V_0}{v_N}L_1##. Conservation of energy implies ##\frac{1}{2}MV_0^2 = \frac{1}{2}mv_N^2##. So, ##L_{closest} = \sqrt{\frac{m}{M}}L_1##

Nice.
 
  • #54
TSny said:
##L_{closest} = \frac{V_0}{v_N}L_1##. Conservation of energy implies ##\frac{1}{2}MV_0^2 = \frac{1}{2}mv_N^2##. So, ##L_{closest} = \sqrt{\frac{m}{M}}L_1##
Can you tell me if that formula allows for a case when M crashes into the wall?
- isn't V/L a relevant factor?

Thanks .
 
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  • #55
bobie said:
Can you tell me if that formula allows for a case when M crashes into the wall?
- isn't V/L a relevant factor?

Thanks .

It's interesting that M never crashes into the wall no matter how large the initial speed of M or how small the mass of the ball!

The distance of closest approach depends only on the initial distance and the ratio of the masses.

Changing the initial speed V of the block just changes the time at which the block reaches the distance of closest approach. If you took a video of the motion, then doubling the initial speed would be equivalent to speeding up the video by a factor of 2.

(Here I'm assuming Newtonian mechanics. If the mass of the ball is extremely small compared to M and if the initial speed of the block is large enough, then the ball could attain relativistic speeds even if V is not relativistic. It might be interesting to think about how that would modify things.)
 
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  • #56
TSny said:
Changing the initial speed V of the block just changes the time at which the block reaches the distance of closest approach.
Thanks for your response,TSny.
TSny said:
. So, ##L_{closest} = \sqrt{\frac{m}{M}}L_1##

If M/m = 106, should M stop at 1/1000 L?
suppose V=L= 1m, and the size of the ball is >1 mm, won't the block crash into the ball and the wall? but does really M reach that far?
 
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  • #57
bobie said:
If M/m = 106, should M stop at 1/1000 L?
suppose V=L= 1m, and the size of the ball is >1 mm, won't the block crash into the ball and the wall?

Yes, you are right. If the ball has a finite size greater than the formula's minimum distance of approach then things get complicated. For that situation I guess you would need to add assumptions about the elastic properties of the ball. Ugh. If the ball doesn't "give" at all, then of course the closest the block could make it to the wall would be the diameter of the ball.

I always had in mind a point mass for the ball - an unrealistic assumption to go along with the perfect elastic collisions! Even under these ideal assumptions, the problem is interesting to me.
 
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  • #58
TSny said:
, the problem is interesting to me.
It is really an intriguing problem, but probably the formula needs to be refined.
Please check if what I found is correct :

when M/m = 3 , Lclosest = 1/√4 = 1/2 L
when M/m ≈ ∞ Lclosest = 1/√49 = , in our example: ≈ .14m
ather the collision N0 (at L = 1) V1 = 1 ( and stays practically the same) and

Thanks for your attention
 
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  • #59
bobie said:
It is really an intriguing problem, but probably the formula needs to be refined.
Please check if what I found is correct :

when M/m = 3 , Lclosest = 1/√4 = 1/2 L
when M/m ≈ ∞ Lclosest = 1/√49 = , in our example: ≈ .14m[/QUOUTE]

ather the collision N0 (at L = 1) V1 = 1 ( and stays practically the same) and v1 = 2 (and grows by 2v+1)
N

Thanks


Can you show how you got these results?
 
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  • #60
TSny said:
Can you show how you got these results?

v1 = 2 (and grows by 2v+1)
N1 takes place at L1 = 1/3 .333m
N2 at L = .2222m (L1- 1/3)
N3 at L = .185 (L2-1/6) and then it decreases very slowly .1697, .1626,.159,.157,.1568,.1564,.1562,.15609 etc ...
probably it won't even be less than .1559 ≈ 1/√41 ,
if M/m varies from
3 to , L should vary from
1/2 to 1/6.4

on my pocket calculator I managed by: 1/3, and then: ANS-ANS/3*2n up to n=30

you surely can work it out by your computer program
 
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