Conservation of Energy for the n-Body Problem, Exercises of Classical and Relativistic Mechanics

This lecture handout is part of Advanced Classical and Relativistic Mechanics course. Prof. Manasi Singh provided this handout at Punjab Engineering College. It includes: Conservation, Eenrgy, Body, Problem, Kinetic, Potential, Angular, Momentum, Newton, Law

Typology: Exercises

2011/2012

Uploaded on 07/19/2012

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Conservation of Energy for the n-Body Problem
If Newton’s Second Law holds, then energy is conserved.
Solution: The energy is given by E=T+V, where Tis the kinetic energy and Vis the potential
energy. If there are nbodies in a system, then T=
n
X
i=1
1
2mi˙q2
i(t) and so ˙
T=
n
X
i=1
mi¨qi·˙qi=
n
X
i=1
Fi·˙qi,
by Newton’s Second Law. Since Fi=X
j6=i
Fij =X
j6=i
fij(|qiqj|)qiqj
|qiqj|we have
˙
T=
n
X
i=1 X
j6=i
fij(|qiqj|)qiqj
|qiqj|·˙qi=
n
X
i=1
X
j>i
fij(|qiqj|)qiqj
|qiqj|·˙qi+X
j<i
fij (|qiqj|)qiqj
|qiqj|·˙qi
=
n
X
i=1 X
j>i
qiqj
|qiqj|·(fij(|qiqj|) ˙qifji (|qiqj|) ˙qj) =
n
X
i=1 X
j>i
fij(|qiqj|)qiqj
|qiqj|·( ˙qi˙qj), since
fij =fji by Newton’s Third Law. Also V=
n
X
i=1
Vi=
n
X
i=1 X
j>i
Vij (|qiqj|) so
˙
V=
n
X
i=1 X
j>i
˙
Vij(|qiqj|)d
dt (|qiqj|)) =
n
X
i=1 X
j>i
fij(|qiqj|)qiqj
|qiqj|·( ˙qi˙qj), since V0
ij =fij.
So ˙
E=˙
T+˙
V= 0 and energy is conserved.
Conservation of Energy for the n-Body Problem
If Newton’s Third Law holds, then angular momentum is conserved.
Solution: If there are nbodies in a system, the angular momentum is J(t) =
n
X
i=1
Ji(t) =
n
X
i=1
miqi×˙qi, so ˙
J(t) =
n
X
i=1
mi˙qi×˙qi+qi×m¨qi=
n
X
i=1
qi×Fi=
n
X
i=1
qi×
X
j6=i
fij(|qiqj|)qiqj
|qiqj|
=
n
X
i=1 X
j6=i
fij (|qiqj|)
|qiqj|qi×(qiqj) =
n
X
i=1 X
j6=i
fij(|qiqj|)
|qiqj|qj×qi= 0 since qi×qj=qj×qi,fij =fji
and all the terms will cancel.
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Conservation of Energy for the n-Body Problem

If Newton’s Second Law holds, then energy is conserved.

Solution: The energy is given by E = T + V , where T is the kinetic energy and V is the potential

energy. If there are n bodies in a system, then T =

n ∑

i=

m i q˙

2

i

(t) and so

T =

n ∑

i=

m i q¨ i · q˙ i

n ∑

i=

F

i · q˙ i

by Newton’s Second Law. Since F i

j 6 =i

F

ij

j 6 =i

f ij

(|q i

− q j

q i

− q j

|q i − q j

we have

T =

n ∑

i=

j 6 =i

f ij (|q i −q j

q i

− q j

|q i − q j

· q˙ i

n ∑

i=

j>i

f ij (|q i − q j

q i

− q j

|q i − q j

· q˙ i

j<i

f ij (|q i − q j

q i

− q j

|q i − q j

· q˙ i

n ∑

i=

j>i

q i

− q j

|q i − q j

· (f ij (|q i − q j |) ˙q i − f ji (|q i − q j |) ˙q j

n ∑

i=

j>i

f ij (|q i − q j

q i

− q j

|q i − q j

· ( ˙q i − q˙ j ), since

f ij

= f ji

by Newton’s Third Law. Also V =

n ∑

i=

V

i

n ∑

i=

j>i

V

ij

(|q i

− q j

|) so

V =

n ∑

i=

j>i

V

ij (|q i − q j

d

dt

(|q i − q j

n ∑

i=

j>i

−f ij (|q i − q j

q i

− q j

|q i − q j

· ( ˙q i − q˙ j ), since V

ij

= −f ij

So

E =

T +

V = 0 and energy is conserved.

Conservation of Energy for the n-Body Problem

If Newton’s Third Law holds, then angular momentum is conserved.

Solution: If there are n bodies in a system, the angular momentum is J(t) =

n ∑

i=

J

i

(t) =

n ∑

i=

m i q i × q˙ i , so

J(t) =

n ∑

i=

m i q˙ i × q˙ i +q i ×m q¨ i

n ∑

i=

q i

×F

i

n ∑

i=

q i

×

j 6 =i

f ij (|q i − q j

q i − q j

|q i

− q j

n ∑

i=

j 6 =i

f ij (|q i − q j

|q i

− q j

q i

× (q i

− q j

n ∑

i=

j 6 =i

f ij (|q i − q j

|q i

− q j

q j

× q i

= 0 since q i

× q j

= −q j

× q i

, f ij

= f ji

and all the terms will cancel.

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