Mechanics Langrange's Equation , Lecture Notes - Physics, Study notes of Mechanics

Mechanics, Physics, Lagrange’s Equations, Hamilton’s Principle, D’Alembert’s Principle, Constraint force, Transformation functions, Kinetic energy, Potential energy, harmonic oscillato,r Velocity-Dependent Potential, EM Force on Particle, Monogenic System, Configuration Space, Action Integral , Infinitesimal Path Difference.

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Mechanics
Physics 151
Lecture 3
Lagrange’s Equations
(Goldstein Chapter 1)
Hamilton’s Principle
(Chapter 2)
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MechanicsPhysics 151

Lecture 3

Lagrange’s Equations(Goldstein Chapter 1)Hamilton’s Principle

(Chapter 2)

What We Did Last Time!^ Discussed multi-particle systems^!^ Internal and external forces

!^ Laws of action and reaction

!^ Introduced constraints^!^ Generalized coordinates!^ Introduced Lagrange’s Equations^!^ ... and didn’t do the derivation "^ Let’s pick it up and start from there

Lagrange’s Equations!^ Express

L = T – V

in terms of generalized coordinates

, their time-derivatives

, and time

t

!^ The potential

V = V

(q,^ t) must exist

!^ i.e. all forces must be conservative

j^

j d^ L

L

dt^ q ^ ∂^ ∂−^ q

^ ^ ∂^

!^  

( ,^ , )L q q t^

!T^ V≡^ −

Kinetic energyPotential energy Lagrangian

Recipe

{^ }q^ j

!{ }qj

Virtual Displacement!^ Consider a system with constraints^!^ Ordinary coordinates

r (i^ = 1...i^

N)

!^ Generalized coordinates

q(j^ = 1...j^

n)

!^ Imagine moving all the particlesslightly^!^ Note that

δ r must satisfy the constraintsi^

1 1

1 2 2 2

(^ ,^ ,...,^1 21

(^ ,^ ,...,

(^ ,^ ,...,

n n , ) N^ N^

n q^ q^

q^ t q^ q^

q^ t q^ q^

q^ t = r r   = r r  ^ "  = r r

i^ i^

δi →^ + r r^

r

Virtual displacement i i^

j j^ j

q q

=^ ∑^ ∂

r r 3 N^ coordinatesnot independent

n^ coordinatesindependent j^ j^

j q^ q

q^ δ→ +

D’Alembert’s Principle^!^ Force of constraints dropped out because^!^ Called D’Alembert’s Principle (1743)!^ Now we switch from

r to^ i^

q^ j

!^ Unit of

Q^ not always [force]j^ !^ Q^ qj^

(^ )( is always [work]j

)^

a i i^

i i

δ− = F^ ∑

! p^ r

(^0) δ =i i f^ r

1st term

i i^

j^

j^ j

i^ j^

j q^ j

Q^ q δ q

δ ∂ =^

∑^ ∑

r F^

i j^

i i j Q^

∂ q ≡^

rF ∑ ∂ Generalized force

“constraint” force is out of the game.

You can forget (a)

D’Alembert’s Principle^!^ A bit of work can show!^ D’Alembert’s Principle becomes

,

2nd term

i^

i

i^ i^

i^

j^

i^ i^

j

i^

i^ j^

i j j^

j q^

m^

q

q^

q

δ

δ

δ

∂^

=^

=^

∂^

∑^

∑^ ∑

r^

r

p^ r^

p^

r

!^

!^

!!^2

2 2

i^

i^

i

i j^

j^

j v^

v

d q^ dt

q^

q ^

^ 

∂^

∂^

→^

^

^ 

∂^

∂^

^

^ 

^

r !! (^) r

! j

j^

j^

j d^ T

T

q dt^ q

q

^

^ ∂^

^

=^

^ 

^ ∂^

^

^ 

∑^

j^ j

j^

j^

j d^ T

T

Q^

q

dt^ q

q

^

^

^ ∂^

^

−^

−^

^

^ 

^ ∂^

^

^

^ 

^

∑^

(^2) mv i (^2) i T^ ≡^ ∑

Lagrange’s Equations!^ Assume that

(^ V^ does not depend on

)^0 j^

T^ V j d^ T dt^ q^

q ^ 

∂^

∂^ −

^ ^ ∂^

!^ q^ j

V ∂^0 =!q∂ j

0 j^

j d^ L

L

dt^ q ^ ∂^ ∂−^ q

^ ^ ∂^

Finally

(^ ,^

, )^

(^ , )

j^ j^

j

L^ T q

q^ t^

V q^ t =^

Done!

Assumptions We Made!^ Constraints are holonomic^!^ We always assume this!^ Constraint forces do no work^!^ Forget frictions!^ Applied forces are conservative^!^ Lagrange’s Eqn. itself is OK if

V^ depends explicitly on

t

!^ Potential

V^ does not depend on

(^ ,^ ,...,^1

i^ i^

n q^ q^

q^ t

= r r^0 δ^ = f r i i V= −∇ F i i

!^ q^ j

V ∂ 0 =!q∂ j

Will review the last assumption later

Example: Time-Dependent^!^ Transformation functions:^!^ Kinetic energy^!^ Potential energy

(^ ) cos x l^ r^ (^ ) sin

t y^ l^

r^ α tα =^ +  =^ + {^

}^ {

}

2 2

2

m^

m T^

x^ y^

r^ l^

r^ α

=^

+^ =

+^ +

!^!^

K^22

V^

r= {^

} 2

2 2

2 (^ ) 2

m^

K

L^

r^ l^

r^

r α =^

+^ +^

2 (^ )

d^ L^

L^ mr

m^

l^ r^

Kr

dt^ r

r

∂^

^ ^ −

=^

−^

+^ +^

^ ∂^

^ ^

Lagrange’s Equation

Example: Time-Dependent^!^ If

K^ >^ m

2 α, a harmonic oscillator with

!^ Center of oscillation is shifted by! If^ K^ <^ m

2 α, moves away exponentially

!^ If^ K

2 = m α

, velocity is constant !^ Centripetal force balances with the spring force

2 (^ )

d^ L^

L^ mr

m^

l^ r^

Kr

dt^ r

r

∂^

^ ^ −

=^

−^

+^ +^

^ ∂^

^ ^

2 2

2

(^

)^

m^ l

mr^ K

m^

r^ K^

α m α^

α ^

+^ −

−^

^

^

2

K^ m^ α m

ω^

Assumptions We Made!^ Constraints are holonomic^!^ We always assume this!^ Constraint forces do no work^!^ Forget frictions!^ Applied forces are conservative^!^ Lagrange’s Eqn. itself is OK if

V^ depends explicitly on

t

!^ Potential

V^ does not depend on

(^ ,^ ,...,^1

i^ i^

n q^ q^

q^ t

= r r^0 δ^ = f r i i V= −∇ F i i

!^ q^ j

V ∂ 0 =!q∂ j

Let’s review the last assumption

Velocity-Dependent Potential!^ We assumed

and^

so that

!^ We could do the same if we had

V ∂^0 =!q∂ j j j^

j d^ T

T

Q

dt^ q ^ ∂^ ∂−^ q

^ ^ ∂^

(^

)^ (

j^

j

d^ T

V^

T^ V

dt^

q^

q ^

∂^ −^

∂^ −−

^

^

∂^

^

This had to be 0

j

j^

j U^ d

U

Q^

q^ dt

^  q ∂^

= −^

+^ ^

∂^

!^ ∂ 

(^ ,^

, )j j U^ U q

! q^ t=

Generalized,or velocity-dependent“potential”

(^ ,^

, )^

(^ ,^

j^ j^

j^ j

L^ T q

q^ t^

U q^ q

t

=^

!^ −

j

V j Q^

∂= − q∂

Monogenic System!^ If all forces in a system are derived from a generalizedpotential,its called a monogenic system^!^ U

is a function of! Lorentz force is monogenic

!^ A monogenic system is conservative only if^!^ Or!^ Lagrange’s Equation works on a monogenic system

j

j^

j U^ d

U

Q^

q^ dt

^  q ∂^

= −^

+^ ^

∂^

! , ,q q t

U^ U q=

U^ U q^

t ∂^

Hamilton’s Principle!^ We derived Lagrange’s Eqn from Newton’s Eqn usinga “differential principle”^!^ D’Alembert’s principle uses infinitesimal displacements!^ It’s possible to do it with an “integral principle”

Hamilton’s Principle