Symmetries and Conserved Quantities in Newton's Second Law, Exercises of Classical and Relativistic Mechanics

The symmetries and conserved quantities in newton's second law, including time reversal symmetry, spatial rotation symmetry, spatial translation symmetry, and galilean symmetry. How these symmetries imply that the forces acting on a body satisfy certain properties, and introduces the concepts of isometries and orthogonal linear transformations. The document also mentions the conserved quantities of energy, angular momentum, momentum, and galilean symmetry.

Typology: Exercises

2011/2012

Uploaded on 07/19/2012

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2. Time reversal symmetry:
˜qi(t) = qi(t)
Again: qisatisfying Newton’s 2nd law implies ˜qialso satisfies Newton’s 2nd law.
3. Spatial rotation symmetry:
˜qi(t) = Rqi(t)
where R:R3R3is a rotation. Again: qisatisfying Newton’s 2nd law implies ˜qialso does.
Then JB breaks the table because he’s not strong enough to move the Earth.
4. Spatial translation symmetry:
˜qi(t) = qi(t) + k, k R3
Again, same thing. 3) and 4) are isometries of R3, that is, functions T:R3R3such that
||T x T y || =||xy||,x, y R3.
Theorem 1 Every isometry T:R3]R3is the composite of:
1. a rotation
2. a translation
and possibly
3. parity (total spacial inversion):
x7→ x, (xR3)
Let’s show that if T:R3R3is an isometry and
˜qi(t) = T qi(t)
then qisatisfies Newton’s 2nd law implies ˜qidoes.
m¨
˜qi(t) = md2
dt2T qi(t)
=md
dt ddtT qi(t)
Now use the theorem:
T x =Sx +k x R3
where kR3and Sis an orthogonal linear transformation (i.e. 3 ×3 matrix with S S= 1, or a
linear transformation with ||Sx|| =||x||,xR3).
Then d
dt T qi(t) = S˙qi(t)
and d2
dt2T qi(t) = S¨qi(t)
2
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  1. Time reversal symmetry: q˜i(t) = qi(−t) Again: qi satisfying Newton’s 2nd^ law implies ˜qi also satisfies Newton’s 2nd^ law.
  2. Spatial rotation symmetry: q˜i(t) = Rqi(t) where R: R^3 → R^3 is a rotation. Again: qi satisfying Newton’s 2nd^ law implies ˜qi also does. Then JB breaks the table because he’s not strong enough to move the Earth.
  3. Spatial translation symmetry:

q˜i(t) = qi(t) + k, k ∈ R^3

Again, same thing. 3) and 4) are isometries of R^3 , that is, functions T : R^3 → R^3 such that

||T x − T y|| = ||x − y||, ∀x, y ∈ R^3.

Theorem 1 Every isometry T : R^3 →]R^3 is the composite of:

  1. a rotation
  2. a translation and possibly
  3. parity (total spacial inversion): x 7 → −x, (x ∈ R^3 )

Let’s show that if T : R^3 → R^3 is an isometry and

q˜i(t) = T qi(t)

then qi satisfies Newton’s 2nd^ law implies ˜qi does.

m q¨˜i(t) = m

d^2 dt^2

T qi(t)

= m d dt

ddtT qi(t)

Now use the theorem: T x = Sx + k x ∈ R^3

where k ∈ R^3 and S is an orthogonal linear transformation (i.e. 3 × 3 matrix with SS†^ = 1, or a linear transformation with ||Sx|| = ||x||, ∀x ∈ R^3 ). Then d dt

T qi(t) = S q˙i(t)

and d^2 dt^2

T qi(t) = S q¨i(t)

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so

mi q¨˜i(t) = miS q¨i(t)

= S

j 6 =i

f (||qi(t) − qj (t)||)

qi(t) − qj (t) ||qi(t) − qj (t)||

j 6 =i

f (||T qi(t) − T qj (t)||)

T qi(t) − T qj (t) ||T qi(t) − T qj (t)||

using T x = Sx + k and that T is an isometry.

There is also a fifth symmetry, Galilean symmetry

q ˜i(t) = qi(t) + tv, v ∈ R^3

If qi is a solution of Newton’s 2nd^ law, then so is ˜qi.

m q¨˜i(t) = m q¨i(t)

=

j 6 =i

fi(||qi(t) − qj (t)||)

qi(t) − qj (t) ||qi (t) − qj (t)||

j 6 =i

fi(|| q˜i(t) − q˜j (t)||)

q˜i(t) − q˜j (t) || q˜i (t) − q˜j (t)||

Conserved quantities Symmetries Energy E ∈ R Time translation symmetry (a 1d group, R) Angular momentum J ∈ R^3 Rotation symmetry (a 3d group, SO(3)) Momentum p ∈ R^3 Translation symmetry (a 3d group, R^3 ) ? Galilean symmetry (a 3d group, R^3 )

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