Galilean Symmetry, Conserved Quantities, and Hamilton's Equations, Exercises of Classical and Relativistic Mechanics

Galilean symmetry and its corresponding conserved quantity for a system of particles in three-dimensional space interacting via central forces. It also introduces hamilton's equations and poisson brackets, explaining how they relate to the conservation of energy and momentum.

Typology: Exercises

2011/2012

Uploaded on 07/19/2012

davdas900
davdas900 🇮🇳

4.6

(5)

110 documents

1 / 3

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
1Galilean Symmetry and its Conserved Quantity
Last time we discovered there was a symmetry called Galilean symmetry, but we did not know a
corresponding conserved quantity. Given nparticles in R3interacting via central forces, if qi:RR3
is a solution of Newton’s 2nd law, we get a new solution
˜qi(t) = qi(t) + tv
where vR3. This is called Galilean symmetry; Galilean symmetries form a group, R3. What
are the conserved quantities?
Our system of particles has a total mass:
m=
n
X
i=1
mi
and a center of mass
q(t) = Pmiqi(t)
m.
We have also discussed the total momentum
p(t) =
n
X
i=1
pi(t)
which is also conserved. Note:
p(t) = m˙q(t)
so the center of mass moves at a constant velocity, so:
q(t) + q(0) + tv
for some vR3. So
q(t)tv R3
is a conserved quantity! This is “center of mass at time zero” - this is the conserved quantity
corresponding to Galilean symmetry.
q(t)tv =Pmiqi(t)
mtPmi˙qi(t)
m.
Compare this to total momentum:
p(t) = Xmi˙qi(t).
Note: the center of mass at time zero has “explicit time dependence” - not just a function of qi(t)
and ˙qi(t).
1
docsity.com
pf3

Partial preview of the text

Download Galilean Symmetry, Conserved Quantities, and Hamilton's Equations and more Exercises Classical and Relativistic Mechanics in PDF only on Docsity!

1 Galilean Symmetry and its Conserved Quantity

Last time we discovered there was a symmetry called Galilean symmetry, but we did not know a corresponding conserved quantity. Given n particles in R^3 interacting via central forces, if qi: R → R^3 is a solution of Newton’s 2nd^ law, we get a new solution

q˜i(t) = qi(t) + tv

where v ∈ R^3. This is called Galilean symmetry; Galilean symmetries form a group, R^3. What are the conserved quantities? Our system of particles has a total mass:

m =

∑^ n

i=

mi

and a center of mass

q(t) =

miqi(t) m

We have also discussed the total momentum

p(t) =

∑^ n

i=

pi(t)

which is also conserved. Note: p(t) = m q˙(t)

so the center of mass moves at a constant velocity, so:

q(t) + q(0) + tv

for some v ∈ R^3. So q(t) − tv ∈ R^3

is a conserved quantity! This is “center of mass at time zero” - this is the conserved quantity corresponding to Galilean symmetry.

q(t) − tv =

miqi(t) m

t

mi q˙i(t) m

Compare this to total momentum: p(t) =

mi q˙i(t).

Note: the center of mass at time zero has “explicit time dependence” - not just a function of qi(t) and ˙qi(t).

2 Hamilton’s Equations

Let’s just consider a single particle in Rn, with position

q: R → Rn

satisfying newton’s 2nd^ law:

m q¨i(t) =

∂V

∂qi

(q(t))

for some potential V : Rn^ → R. This equation is 2nd-order, so you an rewrite it as a pair of 1st-order equations:

q˙i(t) =

m pi(t) (∗∗)

p˙i(t) =

∂V

∂qi

(q(t))

describing the rate of position and momentum - these are “equal partners” in the Hamiltonian approach. The right-hand side is related to energy

E =

m q˙^2 + V (q)

p^2 2 m

  • V (q)

The Hamiltonian H: Rn^ × Rn^ → R is the energy as a function of p ∈ Rn, q ∈ Rn:

H(q, p) =

p^2 2 m

  • V (q)

Note: ∂H ∂pi

(q, p) = pi m ∂H ∂qi

(q, p) =

∂V

∂qi

So, (**) are equivalent to Hamilton’s equations:

d dt

qi(t) =

∂H

∂pi

(q(t), p(t))

d dt

pi(t) = −

∂H

∂qi

(q(t), p(t))

This pattern reminds of us rotating by 90 degrees in the plane or multiplying by i. This is the secret expanation of what is going on!

3 Poisson Brackets

We call Rn^ the phase space of a particle in n-dimensions - a point in it specifies the particles position and momentum (q, p) ∈ Rn^ × Rn.