Examples etc Flashcards

1
Q

What does is meant by homogeneity of space?

A

The motion is independent of position (i.e. no v(r))

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2
Q

How can we prove that space is homogeneous?

A
  • Displacement of pos by 𝛿r, so r1’ = r1 + 𝛿r, and v1’ = v1
  • New L’ = L + 𝛿L
  • If space is homogeneous, then action is the same, 𝛿L = 0
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3
Q

How do we express the Lagrangian after it has been displaced by 𝛿r?

A

L(r+𝛿r, v) = L(r, v) + dL/dx 𝛿x + dL/dy 𝛿y + dL/dz 𝛿z, so 𝛿L = L(r+𝛿r, v) - L(r,v) = ∇L.𝛿r

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4
Q

What is ∇L equal to if 𝛿L = 0 for and 𝛿r?

A

∇L = 0, so dL/dqi = 0

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5
Q

What do we find from the E-L equation from dL/dqi = 0?

A

d/dt(dL/dq’i) = dL/dqi = 0, so d/dt(pi) = 0, where pi is the generalised momentum -> pi is constant if space is homogeneous

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6
Q

How can we express 𝛿L for many particles?

A

𝛿L = sum over a of dL/dra . 𝛿r, where a is the index of the particle

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7
Q

If 𝛿L = 0 for any 𝛿r, what do we get the sum of dL/dra is equal to?

A

sum over a of dL/dra = 0

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8
Q

What can we do with the E-L equation for many particles?

A

Sum all E-L equations: sum over a of dL/dra - sum over a of d/dt(dL/dr’a) = 0, so sum over a of d/dt(dL/dr’a) = 0

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9
Q

What do we find from the sum of the E-L equations?

A

p(a) = dL/dr’a, so total momentum P = sum over a of p(a) -> P is conserved if space is homogeneous

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10
Q

What is the one exception for the homogeneity of space with velocity depending on r?

A

Can hold if there are interactions between particles i.e. v(r2-r1)

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11
Q

What is the conservation law for the momenta?

A

Any canonical momenta pi whose conjugate coordinate qi does not appear in L is conserved.

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12
Q

What is meant by the homogeneity of time?

A

If L is not an explicit function of time, it doesn’t matter what time motion occurs.

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13
Q

What can we infer from the Homogeneity of time?

A

If time is homogeneous, L = L(qi, qi’), so dH/dt = 0, H is conserved (E is conserved)

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14
Q

What is meant by the isotropy of space?

A

Mechanical properties don’t change on rotating the system if space is isotropic. Conversely, special direction effects motion.

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15
Q

What do we do to show the isotropy of space?

A
  • Rotate space around z, define rotation as by 𝛿Ф = dФ z(hat), and change in position 𝛿r = r*sinθ 𝛿Ф Ф(hat)
  • 𝛿r = 𝛿Ф X r, and want 𝛿v
  • 𝛿v = d/dt(𝛿r) = 𝛿Ф X r’ = 𝛿Ф X v
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16
Q

What is the change in Lagrangian for a single particle when rotation the space?

A

𝛿L = sum over i of (dL/dqi * 𝛿qi + dL/dqi’ *𝛿qi’) = dL/dr 𝛿r + dL/dv 𝛿v

17
Q

What is another way of writing dL/dqi and how can we write this?

A

Fi = ρi’ = dL/dqi, so 𝛿L = ρi’ . 𝛿r + ρi . 𝛿v

18
Q

What do we then substitute into 𝛿L?

A
  • 𝛿r = 𝛿Ф Xr and 𝛿v = 𝛿Ф X v

- Can then rearrrange using law to 𝛿L = 𝛿Ф.(rXρ’ + vXρ) = d/dt(rXρ)

19
Q

What do we finally find from 𝛿L?

A
  • 𝛿L = 𝛿Ф.d/dt(rXρ) = 0 if space isotropic
  • For all 𝛿Ф, d/dt(rXρ) = 0 or d/dt(L) = 0, where L is angular momentum
  • Isotropy of space means angular momentum is conserved
20
Q

What is the change in Lagrangian for many particles when rotation the space?

A

𝛿L = sum over a of (dL/dr(a) . 𝛿r(a) + dL/dv(a) . 𝛿v(a) = 0, where a is the particle index and 𝛿r(a) = 𝛿ФXr(a), and same of 𝛿v(a)

21
Q

What is the next step after finding the in Lagrangian for multiple particles?

A
  • Use ρ(a) = dL/dv(a) and F(a) = dL/dr(a) = ρ’(a), and sub this into 𝛿L
  • Sub in the values for 𝛿r(a) and 𝛿v(a) aswell
22
Q

What is the final version of 𝛿L for many particles?

A

𝛿L = 𝛿Ф*(sum over a of d/dt(r(a)Xρ(a)) = 0

23
Q

What do we find from the final version of 𝛿L for many particles?

A

sum over a of d/dt(r(a)Xρ(a)) = 0 so total angular momentum of system is conserved if space is isotropic

24
Q

What can we summarise from these Lagrangian rearrangements?

A

With n generlised coordinates, have up to 2n+1 conserved quantities (n linear momenta, n angular momenta and energy)

25
Q

What is Noether’s theorem?

A

If a symmetry in the Lagrangian exists, there is a corresponding constant of the motion.

26
Q

What is a good example to show this theory?

A

-Field is an infinite homogeneous plane, e.g. V constant at height z i.i. V(z), but T(x’, y’, z’)

27
Q

How can we find the conserved quantities in this example?

A
  • Energy conserved as no t in L = t-V
  • Linear momenta ρx and ρy conserved as L invariant to translation in x-y plane, not conserved in ρz
  • angular momenta Lz conserved and L is invariant under rotation about z(hat)
28
Q

How can we find the conserved quantities for a field due to 2 point objects?

A

Since V is symmetric on rotation around x, Lx is conserved, and energy is conserved, but everything else is not. Component of angular momentum along an axis about which V is symmetric, is conserved.