Friday, March 25, 2016

homework and exercises - Write Equation of Motion in Polar Coordinates




a point of mass m moves on the xyPlane and has the potential energy U(x,y)=A2(x2+y2)+B with A,B>0 being two constants.


Let r denote the position of the mass on the xyPlane.


We knoe that m¨r=U(x,y)


We first write U(r,φ)=A2r2+B


so we get U(r,φ)=(Ar0)


We now calculate ¨r in polar coordinates.


We have


r=r(cos(φ)sin(φ))


˙r=˙r(cos(φ)sin(φ))+r(sin(φ)cos(φ))˙φ


¨r=¨r(cos(φ)sin(φ))+2˙r(sin(φ)cos(φ))˙φr(cos(φ)sin(φ))˙φ2+r(sin(φ)cos(φ))¨φ



we put everything together:


¨r=¨r(cos(φ)sin(φ))+2˙r(sin(φ)cos(φ))˙φr(cos(φ)sin(φ))˙φ2+r(sin(φ)cos(φ))¨φ=1m(Ar0)


(*)Since (cos(φ)sin(φ))=ˆer and (sin(φ)cos(φ))=ˆeφ and also (Ar0)=Arˆer+0ˆeφ we get:


(**)(¨rr˙φ22˙r˙φ+r¨φ)=1m(Ar0)


My lecture notes now write it down like this:


(***)(¨rr¨φ)=(Arm+r˙φ22˙r˙φ)


Question 1: Is (sin(φ)cos(φ))=ˆeφ true or is it rather (sin(φ)cos(φ))=ˆeφ?


Question 2: Is there a reason why we wrote ( ** ) as ( * ** )? Does the left side of (***) tell us something?


Question 3: Is it possible that my potential depends on r and φ? And if so, could I write down the general formula like that:


(m¨rmr¨φ)=(Kr(r,φ)+r˙φ2Kφ(r,φ)2m˙r˙φ)



With K(r,φ) being a conservative force field (so K=U applies)


Question 4: Why don't I have to transform the constants?



Answer



Question 1:


It's up to you to chose a basis to your problem. They can differ only by a global fase (such a minus sign, since eiπ=1).


Question 2:


As you might see, both expressions are the same. It's up to you chose the one you prefer. However, when you get something equals to a constant is always a good thing, since means that a quantity is conserved (in your case, \frac{d}{dt}2\dot{r}\dot{φ}+r\ddot{φ})


Question 3:


you can get (at least, theoretically) a potential V=V(r,\varphi) and there will be a general formula (take into account that \nabla U=\frac{\partial U}{\partial r}+\frac{1}{r}\frac{\partial U}{\partial \varphi})


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