31.6: Collisions in Two Dimensions
- Page ID
- 92256
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)Now consider a collision in two dimensions between two masses \(m_{1}\) and \(m_{2}\) (Fig. \(\PageIndex{1}\)). Without loss of generality, we can work in a coordinate system that is at rest with respect to mass \(m_{2}\), and in which mass \(m_{1}\) is moving in the \(+x\) direction, as shown in the figure. Then before the collision, mass \(m_{1}\) is moving with velocity \(\mathbf{v}_{1 i}=v_{1 i} \mathbf{i}\). After the collision, mass \(m_{1}\) moves with velocity \(\mathbf{v}_{1 f}=\left(v_{1 f} \cos \theta_{1}\right) \mathbf{i}-\left(v_{1 f} \sin \theta_{1}\right) \mathbf{j}\); mass \(m_{2}\) moves with velocity \(\mathbf{v}_{2 f}=\left(v_{2 f} \cos \theta_{2}\right) \mathbf{i}+\left(v_{2 f} \sin \theta_{2}\right) \mathbf{j}\).
By conservation of momentum, we know that both the \(x\) and \(y\) components of the total system momentum are independently conserved. This gives two equations: in the \(x\) direction,
\[p_{i x} =p_{f x} \]
\[m_{1} v_{1 i} =m_{1} v_{1 f} \cos \theta_{1}+m_{2} v_{2 f} \cos \theta_{2}\]
and in the \(y\) direciton,
\[p_{i y} =p_{f y} \]
\[0 =-m_{1} v_{1 f} \sin \theta_{1}+m_{2} v_{2 f} \sin \theta_{2} .\]
So Eqs. \(\PageIndex{2}\) and \(\PageIndex{4}\) give us two equations - but in this case there are four unknowns ( \(v_{1 f}, v_{2 f}, \theta_{1}\), and \(\theta_{2}\) ). To determine the four unknowns, we need as many equations as we have unknowns, so we're two equations short and we need to provide some more information. For example, if we assume that the collision is perfectly elastic, then we can add another equation, since kinetic energy will be conserved in this case:
\[K_{i} =K_{f} \]
\[\frac{1}{2} m_{1} v_{1 i}^{2} =\frac{1}{2} m_{1} v_{1 f}^{2}+\frac{1}{2} m_{2} v_{2 f}^{2}\]
Now we have three equations (Eqs. \(\PageIndex{2}\), \(\PageIndex{4}\), and \(\PageIndex{6}\)), but we still have four unknowns—we still need more information to find the final velocities. To solve the problem, we could be given one of the four unknowns, for example. But the piece of information that's really missing here is the impact parameter of the collision, which is the perpendicular distance between the center of mass \(m_{2}\) and the line along the the initial velocity vector \(\mathbf{v}_{1 i}\). If the impact parameter is zero, then mass \(m_{1}\) hits mass \(m_{2}\) head-on. If the impact parameter is equal to the sum of the radii of \(m_{1}\) and \(m_{2}\), then the two masses will barely touch in a glancing blow. Knowing the impact parameter is necessary for finding the angles \(\theta_{1}\) and \(\theta_{2}\).
Collisions in two dimensions are more general that you might think: under a central-force law, motion will be in a plane, so the particles will move in two dimensions. Analyzing two-dimensional collisions of this type is common in particle physics. There the particles typically do not actually touch, but are repelled or attracted by the electrostatic force. The same laws apply in particle physics as what we've described here.