Saw
Gold Member
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That’s a good point, bringing in the concept of reduced mass! It converges with the progress I was making in the domain of collisions (see the thread “Acceleration in an elastic collision”), where the conclusion seems to be that the force intervening in the collision can also be defined as:
F = \mu (1 + \varepsilon )v_{rel}^{initial}
where:
<br /> \begin{gathered}<br /> \mu = \frac{{m_1 m_2 }}<br /> {{m_1 + m_2 }} = {\text{reduced mass}} \hfill \\<br /> \varepsilon = \frac{{v_{rel}^{final} }}<br /> {{v_{rel}^{initial} }} = {\text{coefficient of restitution}} \hfill \\<br /> a = (1 + \varepsilon )v_{rel}^{initial} = {\text{relative acceleration}} \hfill \\ <br /> \end{gathered} <br />
On the other hand, if you want to consider the possibility that gravitational masses (included in the relative acceleration term) differ from inertial masses (those included in the reduced mass term), then you have to set an upper limit to the former.
In the collision formula, that limit, derived from the conservation of kinetic energy, is that relative acceleration cannot exceed 2 times relative velocity, since the coefficient of restitution can range from 0 to 1. Certainly, if you know that coefficient based on the ratio final/initial relative velocity, the formula is not very useful. But the idea is that you could also obtain it empirically as a coefficient inherent to the material that each body is composed of. In particular, one would have to use, together with “reduced or effective mass”, the “effective coefficient” of the two materials, as if they were one = k1k2/(k1+k2). I still haven’t thought, however, how to translate this to the gravity formula.
F = \mu (1 + \varepsilon )v_{rel}^{initial}
where:
<br /> \begin{gathered}<br /> \mu = \frac{{m_1 m_2 }}<br /> {{m_1 + m_2 }} = {\text{reduced mass}} \hfill \\<br /> \varepsilon = \frac{{v_{rel}^{final} }}<br /> {{v_{rel}^{initial} }} = {\text{coefficient of restitution}} \hfill \\<br /> a = (1 + \varepsilon )v_{rel}^{initial} = {\text{relative acceleration}} \hfill \\ <br /> \end{gathered} <br />
On the other hand, if you want to consider the possibility that gravitational masses (included in the relative acceleration term) differ from inertial masses (those included in the reduced mass term), then you have to set an upper limit to the former.
In the collision formula, that limit, derived from the conservation of kinetic energy, is that relative acceleration cannot exceed 2 times relative velocity, since the coefficient of restitution can range from 0 to 1. Certainly, if you know that coefficient based on the ratio final/initial relative velocity, the formula is not very useful. But the idea is that you could also obtain it empirically as a coefficient inherent to the material that each body is composed of. In particular, one would have to use, together with “reduced or effective mass”, the “effective coefficient” of the two materials, as if they were one = k1k2/(k1+k2). I still haven’t thought, however, how to translate this to the gravity formula.