From 6ce0bb9a8f9fd7d169cbb414a9537d68c5290aae Mon Sep 17 00:00:00 2001 From: Prefetch Date: Fri, 14 Oct 2022 23:25:28 +0200 Subject: Initial commit after migration from Hugo --- source/know/concept/reduced-mass/index.md | 134 ++++++++++++++++++++++++++++++ 1 file changed, 134 insertions(+) create mode 100644 source/know/concept/reduced-mass/index.md (limited to 'source/know/concept/reduced-mass') diff --git a/source/know/concept/reduced-mass/index.md b/source/know/concept/reduced-mass/index.md new file mode 100644 index 0000000..12c2ce5 --- /dev/null +++ b/source/know/concept/reduced-mass/index.md @@ -0,0 +1,134 @@ +--- +title: "Reduced mass" +date: 2021-07-05 +categories: +- Physics +layout: "concept" +--- + +Problems with two interacting objects can be simplified +by combining them into a pseudo-object with **reduced mass** $\mu$, +whose position equals the relative position of the objects. +For bodies 1 and 2 with respective masses $m_1$ and $m_2$: + +$$\begin{aligned} + \boxed{ + \mu \equiv \frac{m_1 m_2}{m_1 + m_2} + } +\end{aligned}$$ + +If $\va{x}_1$ and $\va{x}_2$ are the objects' respective positions, +then we define +the relative position $\va{x}_r$, +the relative velocity $\va{v}_r$, +and the relative acceleration $\va{a}_r$: + +$$\begin{aligned} + \va{x}_r + \equiv \va{x}_1 - \va{x}_2 + \qquad + \va{v}_r + \equiv \va{v}_1 - \va{v}_2 + = \dv{\va{x}_r}{t} + \qquad \quad + \va{a}_r + \equiv \va{a}_1 - \va{a}_2 + = \dvn{2}{\va{x}_r}{t} +\end{aligned}$$ + +We now choose the coordinate system's origin +to be the center of mass of both objects: + +$$\begin{aligned} + m_1 \va{x}_1 + m_2 \va{x}_2 = 0 +\end{aligned}$$ + +Rearranging and differentiating then yields the following useful equations: + +$$\begin{aligned} + \va{x}_2 = - \frac{m_1}{m_2} \va{x}_1 + \qquad \quad + \va{v}_2 = - \frac{m_1}{m_2} \va{v}_1 + \qquad \quad + \va{a}_2 = - \frac{m_1}{m_2} \va{a}_1 +\end{aligned}$$ + +Using these relations, we can rewrite the relative quantities we defined earlier: + +$$\begin{aligned} + \va{x}_r + = \Big( 1 + \frac{m_1}{m_2} \Big) \va{x}_1 + = \frac{m_1 + m_2}{m_2} \va{x}_1 + \qquad + \va{v}_r + = \frac{m_1 + m_2}{m_2} \va{v}_1 + \qquad + \va{a}_r + = \frac{m_1 + m_2}{m_2} \va{a}_1 +\end{aligned}$$ + +Meanwhile, Newton's third law states that +if object 1 experiences a force $\va{F}_1 = m_1 \va{a}_1$ caused by object 2, +then object 2 experiences an opposite and equal force $\va{F}_2 = - \va{F}_1$. +In fact, our earlier relation between $\va{a}_1$ and $\va{a}_1$ +boils down to Newton's third law: + +$$\begin{aligned} + \va{F}_2 = m_2 \va{a}_2 = - m_1 \va{a}_1 = - \va{F}_1 + \quad \implies \quad + \va{a}_2 = - \frac{m_1}{m_2} \va{a}_1 +\end{aligned}$$ + +With all that in mind, let us take a closer look at the relative acceleration $\va{a}_r$: + +$$\begin{aligned} + \va{a}_r + = \frac{m_1 + m_2}{m_2} \Big( \frac{m_1}{m_1} \Big) \va{a}_1 + = \frac{m_1 + m_2}{m_1 m_2} \big( m_1 \va{a}_1 \big) + = \frac{\va{F}_1}{\mu} + = - \frac{\va{F}_2}{\mu} +\end{aligned}$$ + +Where $\mu$ is the reduced mass, as defined above. +In other words, the relative acceleration $\va{a}_r$ +is just $\va{a}_1 = \va{F}_1 / m_1$ multiplied by $m_1 / \mu$. +This can be regarded as focusing on the dynamics of body 1, +while correcting for the effects of body 2. + +This also suggests the following way +to recover the original positions $\va{x}_1$ and $\va{x}_2$ +from $\va{x}_r$, which you can easily verify for yourself: + +$$\begin{aligned} + \va{x}_1 + = \frac{\mu}{m_1} \va{x}_r + = \frac{m_2}{m_1 + m_2} \va{x}_r + \qquad \quad + \va{x}_2 + = \frac{\mu}{m_2} \va{x}_r + = - \frac{m_1}{m_1 + m_2} \va{x}_r +\end{aligned}$$ + +With this, we can rewrite the total kinetic energy $T$ in an elegant way: + +$$\begin{aligned} + T + &= \frac{1}{2} m_1 \va{v}_1^2 + \frac{1}{2} m_2 \va{v}_2^2 + = \frac{1}{2} m_1 \Big( \frac{\mu}{m_1} \va{v}_r \Big)^2 + \frac{1}{2} m_2 \Big( \frac{\mu}{m_2} \va{v}_r \Big)^2 + \\ + &= \frac{1}{2} \frac{\mu^2}{m_1} \va{v}_r^2 + \frac{1}{2} \frac{\mu^2}{m_2} \va{v}_r^2 + = \frac{1}{2} \Big( \frac{m_2 \mu^2}{m_1 m_2} + \frac{m_1 \mu^2}{m_1 m_2} \Big) \va{v}_r^2 + \\ + &= \frac{1}{2} \frac{(m_1 + m_2) \mu^2}{m_1 m_2} \va{v}_r^2 + = \frac{1}{2} \frac{\mu^2}{\mu} \va{v}_r^2 + = \frac{1}{2} \mu \va{v}_r^2 +\end{aligned}$$ + +Then, assuming that the system's potential energy $V$ +only depends on the distance between the two objects, +i.e. $V = V(|\va{x}_1 - \va{x}_2|) = V(|\va{x}_r|)$, +we just showed that we can rewrite both $T$ and $V$ +to contain only $\mu$ and relative quantities. +This is relevant for both [Lagrangian mechanics](/know/concept/lagrangian-mechanics/) +and [Hamiltonian mechanics](/know/concept/hamiltonian-mechanics/), +where $L = T - V$ and $H = T + V$ respectively. -- cgit v1.3