Central Forces Flashcards

1
Q

For planar motion in a central field, what is the angular momentum L equal to?

A

L = r x p, where r & p define a plane

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2
Q

What is the Lagrangian equal to for planar motion?

A

L = 1/2 m(r’^2 + r^2 *θ’^2) - V(r)

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3
Q

What does the canonical momenta p(θ) equal for the planar motion? What is the case for circular and elliptical orbit?

A

p(θ) = dL/dθ’ = mr^2 *θ’

Circular orbit: r fixed, θ’ const, elliptical orbit: r varies, θ’ varies to make r^2 *θ’ const

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4
Q

How do we find equations for the central and centrifugal forces for the planar motion?

A
  • Use E-L equation in r, and rearrange to make m*r’’ the subject
  • dV/dr term if the central force and mr*θ’^2 term is the centrifugal force (not real force, consequence of the rotational motion)
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5
Q

How can we write the centrifugal force in terms of the angular momentum?

A

Fc = |L|^2/(m*r^3) = -dUc/dr, where Uc(r) is a potential energy

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6
Q

How can we write the equation of motion for planar motion in terms of Uc(r)?

A

m*r’’ = -d/dr(Uc + V) = -d/dr Ueff, where Ueff is the effective potential energy.= Uc + V

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7
Q

What is the equation for the Hamiltonian in terms of Ueff for planar motion?

A

H = p(r)^2/2m + Uc(r) + V(r) = p(r)^2/2m + Ueff(r) = E

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8
Q

What is the equation for p(r)?

A

p(r) = sqrt(2m*(E-Ueff(r)))

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9
Q

What is the equation for E if we look at p(r) = 0 and what can we learn from this?

A

E-Ueff(r) = 0. From this we learn that there is no radial motion when p(r) = 0 - closest or furthest approach in an orbit

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10
Q

What does a sketch of Ueff look like?

A

Like the strong nuclear force graph - high at first then comes down past x axis then back up and tends to -0.

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11
Q

On the Ueff graph, where are E1, E2 and E3 and their corresponding radii?

A

y-axis is E, x-axis is r, E1 is at start, E2 is halfway between crossing x-axis and tunring point, and E3 is just after turning point. r values can be read off from that.

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12
Q

What happens at E = 0, E=E2 and E = E3?

A

E=0 is parabola, E=E2 has 2 rotts, r2 and r2’ where p(r) = 0, E=E3 is a circular orbit, here 2 repeated roots at r = r3

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13
Q

For 2 masses, what do we make the Lagrangian a function of?

A

The centre of mass coordinates: L(x0, y0, r, θ, x0’, y0’, r’, θ’), where θ is the angle from horizontal the line joining the masses is and (x0, y0) is the centre of mass

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14
Q

What is the equation for the kinetic energy of the centre of mass for the 2mass system?

A

T(CoM) = 1/2 (2m)(x0’^2 + y0’^2)

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15
Q

What is the equation for the potential energy of the 2 mass system?

A

V = 1/2 k(r-r0)^2, where r0 is the equilibrium value of r

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16
Q

What is the kinetic energy o the 2 mass system relative to the CoM?

A

T(rel) = 1/4mr^2 θ’^2 + 1/4m*r’^2

17
Q

What is the equation for the Lagrangian of the 2 mass system?

A

L = m(x0’^2 + y0’^2) + 1/4m(r’^2 + r^2 θ’^2) - 1/2k(r-r0)^2

18
Q

What do we find if we look at the E-L equation in x0 for the 2 masses connected by a spring system?

A

No x0 dependence in L, so total momentum along x-direction is conserved.

19
Q

What do we find if we look at the E-L equation in y0 for the 2 masses connected by a spring system?

A

Momentum along y-direction is conserved.

20
Q

What do we find if we look at the E-L equation in r for the 2 masses connected by a spring system?

A

Find equation of motion r’’ = -2k/m (r-r0) +rθ’^2

21
Q

What do we find if we look at the E-L equation in θ for the 2 masses connected by a spring system?

A

Find that angular momentum is conserved

22
Q

If we set the angular momentum θ’ to zero, what do we find for the 2 mass system?

A

Motion split into several ‘modes’: 2 translational modes up and across, 1 vibrational mode (side to side) and 1 rotational mode

23
Q

What are normal modes?

A

A pattern of motion where all particles are moving with same frequency.

24
Q

How can we build up the overall motion of the system?

A

By using a superposition of normal modes.

25
Q

How do we determine how many normal modes we have?

A

If we have n generalised coordinates, we have n normal modes with n frequencies (in total).

26
Q

What is a good example of normal modes?

A

2 coupled oscillators (2 masses, 3 springs, connect to walls either side.

27
Q

What is the Lagrangian for the 2 coupled oscillator problem?

A

L = 1/2mx1’^2 + 1/2mx2’^2 - (1/2kx1^2 + 1/2kx2^2+1/2*k12(x1-x2)^2)

28
Q

Which 2 variables for we apply the E-L equation to for the 2 coupled oscillator problem?

A

x1 and x2.

29
Q

What solutions do we try for x1 and x2 for the 2 coupled oscillator problem?

A

x1(t) = A1exp(iωt), x2(t) = A2exp(iωt)

30
Q

What do we do with the trial solutions for x1 and x2 for the 2 coupled oscillator problem?

A

Sub them into E-L equations and rearrange to make A1 the subject in each. Then set these equal to eachother and rearrange to fine ω1 and ω2.

31
Q

How do we compare the motion of ω1 and ω2?

A

Use equation found for A1 (relative displacement of particle 1 & 2), and find that ω1 is symmetric mode (moves in same direction) whereas ω2 is anti-symmetric mode (moves towards eachother)

32
Q

What is another expression for T to find the inertia matrix?

A

T = 1/2 sum over i,j of qi’mij*qj’, where mij = m = (m11, m12, m21, m22) = 4x4 matrix

33
Q

What can we write mij as? What does this mean?

A

mij = d^2T/dqi’dqj’ = d^2T/dqj’dqi’ = mji -> matrix m is symmetric about diagonal: is the inertia matrix

34
Q

What is a second example we can use for the inertia matrix?

A

Mass m2 moving at x2’ to a mass m1 (moving at x1’), so T = 1/2m1x1’^2 + 1/2m2(x2’-x1’)^2

35
Q

How do we find the inertia matrix M from T?

A

Using d^2T/dqi’dqj’, so m11 = d^2T/dx1’^2, m12 = d^2T/dxq’dx2’, m22 = d^2T/dx2’^2

36
Q

What does M equal for the two masses moving problem?

A

M = (m1+m2, -m2, -m2, m2) = matrix