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12.2: Translational acceleration of a reference frame

Last updated

Mar 14, 2021
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- 12.1: Introduction to Non-inertial Reference Frames
- 12.3: Rotating Reference Frame

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10.2.1.PNG — Figure $\PageIndex{1}$ : Inertial reference frame (unprimed), and translational accelerating frame (primed).

Consider an inertial system $(x_{fix},y_{fix},z_{fix})$ which is fixed in space, and a non-inertial system $(x^{\prime}_{mov}, y^{\prime}_{mov}, z^{\prime}_{mov})$ that is moving in a direction relative to the fixed frame such as to maintain constant orientations of the axes relative to the fixed frame, as illustrated in Figure $\PageIndex{1}$ . The fixed frame is designated to be the unprimed frame and, to avoid confusion the subscript $fix$ is attached to the fixed coordinates taken with respect to the fixed coordinate frame. Similarly, the translating reference frame, which is undergoing translational acceleration, has the subscript $mov$ attached to the coordinates taken with respect to the translating frame of reference. Newton’s Laws of motion are obeyed only in the inertial (unprimed) reference frame. The respective position vectors are related by

$\mathbf{r}_{fix} = \mathbf{R}_{fix}+\mathbf{r}^{\prime}_{mov} \label{12.1}$

where $\mathbf{r}_{fix}$ is the vector relative to the fixed frame, $\mathbf{r}^{\prime}_{mov}$ is the vector relative to the translationally accelerating frame and $\mathbf{R}_{fix}$ is the vector from the origin of the fixed frame to the origin of the accelerating frame. Differentiating Equation $\ref{12.1}$ gives the velocity vector relation

$\mathbf{v}_{fix} = \mathbf{V}_{fix}+ \mathbf{v}^{\prime}_{mov} \label{12.2}$

where $\mathbf{v}_{fix} = \frac{d\mathbf{r}_{fix}}{dt}$ , $\mathbf{v}^{\prime}_{mov} = \frac{d\mathbf{r}^{\prime}_{mov}}{dt}$ and $\mathbf{V}_{fix} = \frac{d\mathbf{R}_{fix}}{dt}$ . Similarly the acceleration vector relation is

$\mathbf{a}_{fix} = \mathbf{A}_{fix}+ \mathbf{a}^{\prime}_{mov} \label{12.3}$

where $\mathbf{a}_{fix} = \frac{d^2\mathbf{r}_{fix}}{dt^2}$ , $\mathbf{a}^{\prime}_{mov} = \frac{d^2\mathbf{r}^{\prime}_{mov}}{dt^2}$ and $\mathbf{A}_{fix} = \frac{d^2\mathbf{R}_{fix}}{dt^2}$ .

In the fixed frame, Newton’s laws give that

$\mathbf{F}_{fix} = m\mathbf{a}_{fix} \label{12.4}$

The force in the fixed frame can be separated into two terms, the acceleration of the accelerating frame of reference $\mathbf{A}_{fix}$ plus the acceleration with respect to the accelerating frame $\mathbf{a}^{\prime}_{mov}$ .

$\mathbf{F}_{fix} = m\mathbf{A}_{fix}+ m\mathbf{a}^{\prime}_{mov} \label{12.5}$

Relative to the accelerating reference frame the acceleration is given by

$m\mathbf{a}^{\prime}_{mov} = \mathbf{F}_{fix} - m\mathbf{A}_{fix} \label{12.6}$

The accelerating frame of reference can exploit Newton’s Laws of motion using an effective translational force $\mathbf{F}^{\prime}_{tran} \equiv \mathbf{F}_{fix} − m\mathbf{A}_{fix}$ . The additional $-m\mathbf{A}_{fix}$ term is called an inertial force; it can be altered by choosing a different non-inertial frame of reference, that is, it is dependent on the frame of reference in which the observer is situated.

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