Set up Lagrange’s equations in cylindrical coordinates for a particle of mass min a potential field V(r,θ,z). Hint: v=dsdt; writein cylindrical coordinates.

Short Answer

Expert verified

Lagrange’s equations in cylindrical coordinatesare mr¨-rθ˙2=-Vr, m2r˙θ˙-rθ¨=-1rVθ,and mz¨=-Vz, respectively, for potential field Vr,θ,z.

Step by step solution

01

Given Information

It is given that mass is mand potential field is Vr,θ,z.

02

Definition of Calculus

In the same way that geometry is the study of shape and algebra is the study of generalisations of arithmetic operations, calculus, sometimes known as infinitesimal calculus or "the calculus of infinitesimals," is the mathematical study of continuous change.. Differentiation and integration are the two main branches.

03

Lagrangian in cylindrical coordinates

Let the velocity vector be v¯, kinetic energy be Tand Lagrangian be L. Write the velocity vector and its kinetic energy in cylindrical coordinates.

v¯=r˙r^+rθ˙θ^+z˙z^

T=12mr˙2+r2θ˙2+z˙2

Now define the Lagrangian from kinetic energy and potential field.

L=T-VL=12mr˙2+r2θ˙2+z˙2-Vr,θ,z

04

Euler’s Equation of r

Write the Euler’s equation with ras its degree of freedom, and find it’s derivatives.

ddtLr˙-Lr=0Lr˙=mr˙ddtLr˙=mr¨Lr=0

Use the equations above and obtain, mr¨-rθ˙2=-Vr.

05

Euler’s Equation of θ

Write the Euler’s equation with θas its degree of freedom, and find it’s derivatives.

ddtLθ˙-Lθ=0Lθ˙=mr2θ˙ddtLθ˙=m2rr˙θ˙+r2θ¨Lθ=-Vθ

Use the equations above and obtain, m2r˙θ˙+rθ¨=-1rVθ.

06

Euler’s Equation of z

Write the Euler’s equation with zas its degree of freedom, and find it’s derivatives.

ddtLz˙-Lz=0Lz˙=mz˙ddtLz˙=mz¨Lz=-Vz

Use the equations above and obtain, mz¨=-Vz.

Therefore, Lagrange’s equations in cylindrical coordinates for a particle of mass min a potential field Vr,θ,z, are mr¨-rθ˙2=-Vr,m2r˙θ˙+rθ¨=-1rVθ, and mz¨=-Vz, respectively.

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Most popular questions from this chapter

Use Fermat’s principle to find the path followed by a light ray if the index of refraction is proportional to the given function

12. y-1

Write and solve the Euler equations to make the following integrals stationary. In solving the Euler equations, the integrals in Chapter 5, Section 1, may be useful.

4.x2x2xds

The speed of light in a medium of index of refraction n is v=dsdt=cn. Then the time of transit from AtoBis t=ABdt=c-1ABnds. By Fermat’s principle above, t is stationary. If the path consists of two straight line segments with n constant over each segment, then

ABnds=n1d1+n2d2,

and the problem can be done by ordinary calculus. Thus solve the following problems:

1. Derive the optical law of reflection. Hint: Let light go from the point A=(x1,y1)to B=(x2,y2)via an arbitrary point P=(x,0)on a mirror along thex-axis. Setdtdx=(nc)dDdx=0, where D=distanceAPB, and show that then θ=ϕ.

(a) Consider the case of two dependent variables. Show that if F=F(x,y,z,y',z')and we want to find y(x)and z(x)to make I=x1x2Fdxstationary, then yand zshould each satisfy an Euler equation as in (5.1). Hint: Construct a formula for a varied path Yfor yas in Section 2 [Y=y+εη(x)with η(x)arbitrary] and construct a similar formula for z[let Z=z+εζ(x), where ζ(x)is another arbitrary function]. Carry through the details of differentiating with respect to ε, putting ε=0, and integrating by parts as in Section 2; then use the fact that both η(x)and ζ(x)are arbitrary to get (5.1).

(b) Consider the case of two independent variables. You want to find the function u(x,y)which makes stationary the double integral y1y2x1x2F(u,x,y,ux,uy)dxdy.Hint: Let the varied U(x,y)=u(x,y)+εη(x,y)where η(x,y)=0at x=x1,x=x2,y=y1,y=y2but is otherwise arbitrary. As in Section 2, differentiate with respect to ε, ε=0set ε=0, integrate by parts, and use the fact that ηis arbitrary. Show that the Euler equation is then xFux+yFuy-Fu=0.

(c) Consider the case in which Fdepends on x,y,y'and y''. Assuming zero values of the variation η(x)and its derivative at the endpoints x1and x2, show that then the Euler equation becomesd2dx2Fy''-ddxFy'+Fy=0.

Write and solve the Euler equations to make the following integrals stationary. In solving the Euler equations, the integrals in Chapter 5, Section 1, may be useful.

8.x1x2xy'2+x2dx

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