I read the mathematical derivation of fictitious forces on Wikipedia and I'm having trouble understanding it. I went on a few other sites looking for a better derivation, but they're all basically the same. I've also seen this answer already.
What I'm having trouble understanding is that, in every derivation, at some point, the expression ∑3i=1ˆuixi (where ˆui represents a unit vector of the non-inertial frame in the inertial frame, and xi is a coordinate of the particle in the non-inertial frame) is equated with "→xA" or something similar (the position of the particle in the non-inertial frame). Likewise ∑3i=1ˆuidxidt is equated with →vA and ∑3i=1ˆuid2xidt2 with →aA.
This doesn't make any sense to me. The position vector in the accelerating frame is just (x1,x2,x3) since x1,x2,x3 were defined to be the coordinates of the particle in the accelerating frame. It is not ∑3i=1ˆuixi; that gives you the position vector in the inertial frame.
For example here's what Wikipedia says:
The interpretation of this equation [xB=∑3i=1xjuj] is that xB is the vector displacement of the particle as expressed in terms of the coordinates in frame B at time t.
Even though the derivation clearly gives the correct answers, I simply can't understand this step.
Answer
I personally think the descriptions on Wikipedia are rather confusing, so I'm going to write a self-contained derivation in my own words; hopefully this helps. Note: I'll use Einstein summation notation throughout.
In order to understand what's really going on in the derivation, I'm going to attempt to separate pure mathematics from physics. In particular, I'm going to derive a purely mathematically result, and then interpret that result at the end.
Some Pure Math
Let {ei} denote the standard ordered basis on R3. Namely e1=(1,0,0) etc. For each real number t, let {ui(t)} denote an orthonormal basis on R3, possibly different from the standard one at any given t, generated by a one-parameter family of rotations (elements of SO(3)) B(t); ui(t)=B(t)ei.
¨x(t)=¨X(t)+B(t)(¨riB(t)ei)+2˙B(t)(˙riB(t)ei)+¨B(t)(riB(t)ei)
What it all means physically.
Let a physicist named Alice set up a set of cartesian axes in an inertial frame, and let Bob set up cartesian axes in a non-inertial frame. The triples x(t)=(x1(t),x2(t),x3(t))X(t)=(X1(t),X2(t),X3(t))r(t)=(r1(t),r2(t),r3(t))
With all of this in mind, let's interpret the boxed equation. On the left is the acceleration of the particle as measured by Bob. On the right, the first term is just the acceleration ¨x of the particle as measured by Alice with an extra rotation Bt to account for the difference in the orientations of the axes of the two frames. The second term is the acceleration ¨X of the origin of Bob's frame as measured by Alice with an extra rotation Bt to account for the difference in orientations of the axes of the two frames. The third term is the familiar expression for the Coriolis acceleration, the fourth term is the centrifugal acceleration, and the last term is the Euler acceleration. In particular, multiplying through by the mass m of the particle, each of the expressions on the right gives the standard expression for each of the various corresponding fictitious forces. m¨rB=Bt(m¨x)−Bt(m¨X)−2mΩB×˙rB⏟Coriolis−mΩB×(ΩB×rB)⏟centrifugal−m˙ΩB×rB⏟Euler
The Vector ΩB - Important Subtlety.
Note that I defined the vector ΩB via the skew-symmetric matrix ΩB=Bt˙B. In particular, ΩB is the unique vector for which ΩBw=ΩB×w
I hope this was better than Wikipedia. I think this is all pretty clear in my own head, let me know if my wording and notation was clear. If not, I'll attempt to edit for clarity.
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