problema resuelto de mecanica
DESCRIPTION
problema resuelto de mecanica por medio de la teoria lagrangianaTRANSCRIPT
7/21/2019 problema resuelto de mecanica
http://slidepdf.com/reader/full/problema-resuelto-de-mecanica-56d9ab6e87290 1/3
August 14, 2003
PHYSICS 44 MECHANICS
Homework Assignment VI
SOLUTIONS
Problem 1
(a) Consider the case involving motion on the (x; y)-plane perpendicular to the angularvelocity vector ! = ! bz with the potential energy
U (r) = 1
2 k
³x2 + y2
´:
Using the Euler-Lagrange equations
m Är = ¡ rU (r) ¡ m [ 2!£ _r + !£ (!£ r) ] ;
derive the equations of motion for x and y.
(b) By using the equations of motion derived in Part (a), show that the canonical angularmomentum ` = bz ¢ (r£p) is a constant of the motion.
Solution
(a) Using the vector identity j!£ rj2 = !2 r2 ¡ (! ¢ r)2, we ¯nd
@L
@ _r = m (_r + !£ r) ! d
dt
Ã@L
@ _r
! = m (Är + !£ _r)
@L
@ r = ¡ rU (r) + m
h !2 r ¡ ! (! ¢r)
i + m _r£!
or, using the identity ! 2 r¡! (! ¢ r) = ¡ !£ (!£ r), the Euler-Lagrange equation is
m Är = ¡ rU ¡ !£ (!£ r) ¡ 2m !£ _r: (1.1)
We now consider two-dimensional motion under the in°uence of the e®ective potential
U eff (x;y) = k
2
³x2 + y2
´ ¡ m !2
2
³r2¡ z 2
´ =
K
2
³x2 + y2
´;
where K = k ¡ m !2. The Lagrangian in this case is
L(x; _x; y; _y) = m
2
³_x2 + _y2
´ + m! (x _y ¡ y _x) ¡ K
2
³x2 + y2
´: (1.2)
1
7/21/2019 problema resuelto de mecanica
http://slidepdf.com/reader/full/problema-resuelto-de-mecanica-56d9ab6e87290 2/3
The Euler-Lagrange equations are
m Äx = 2 m! _y ¡ K x; (1.3)
m Äy = ¡ 2 m! _x ¡ K y: (1.4)
(b) The canonical momentum p for this problem is de¯ned as
p = @L
@ _r = m ( _r + !£ r) ;
so that the canonical angular momentum ` = bz ¢ r£p is expressed as
` = bz ¢ r£ (m _r + m!£r) = m (x _y ¡ y _x) + m!³
x2 + y2´
:
Using Eqs. (1.3) and (1.4), we ¯nd
d`
dt = m (x Äy
¡y Äx) + 2 m! (x _x + y _y) = 0:
That the canonical angular momentum ` is a constant of the motion can also be seen bytransforming the Lagrangian (1.2) in Cartesian coordinates (x; y) into the Lagrangian
L(r; _r; _') = m
2
³_r2 + r2 _'2
´ + m! r2 _' ¡ K
2 r2; (1.5)
in polar coordinates (r; '), where x = r cos ' and y = r sin '. Since the Lagrangian (1.5)is independent of the polar angle ' , the canonical angular momentum
p' = @L
@ _' = mr2 ( _' + !) (1.6)
is a constant of the motion. It is easy to verify that ` = p'.
Problem 2
If a particle is projected vertically upward to a height h above a point on the Earth'ssurface at a northern latitude ¸, show that it strikes the ground at a point
4!
3 cos ¸
s 8 h3
g
to the west. (Neglect air resistance, and consider only small vertical heights.)
Solution
The Coriolis acceleration equations are
Äx = 2 ! sin ¸ _yÄy = ¡ 2 ! (sin ¸ _x + cos ¸ _z )Äz = ¡ g + 2 ! cos ¸ _y
9>=>; : (2.1)
2
7/21/2019 problema resuelto de mecanica
http://slidepdf.com/reader/full/problema-resuelto-de-mecanica-56d9ab6e87290 3/3
A ¯rst integration of Eq. (2.1) yields
_x = 2 ! sin ¸ y + C x
_y = ¡ 2 ! (sin ¸ x + cos ¸ z ) + C y_z = ¡ g t + 2 ! cos ¸ y + C z9>=>; ; (2.2)
where (C x; C y; C z) are constants de¯ned from initial conditions (x0; y0; z 0) and (_x0; _y0; _z 0).
Here, the initial conditions are (x0; y0; z 0) = (0; 0; 0) and (_x0; _y0; _z 0) = (0; 0; v0). Thus,the constants are (C x; C y; C z) = (0; 0; v0) and integration of Eqs. (2.2) yields
x(t) = 2 ! sin ¸Z t
0
y(¿ ) d¿; (2.3)
y(t) = ¡ 2 ! sin ¸Z t0
x(¿ ) d¿ ¡ 2 ! cos ¸Z t0
z (¿ ) d¿; (2.4)
z (t) = v0 t ¡ g t2
2 + 2 ! cos ¸
Z t0
y(¿ ) d¿: (2.5)
To ¯rst order in !, the equations (2.3)-(2.5) become
x(t) = 0; (2.6)
y(t) = ¡ 2 ! cos ¸Z t0
µv0 ¿ ¡ g
2 ¿ 2¶
d¿ = ¡ ! cos ¸µ
v0 t2 ¡ g
3 t3¶
; (2.7)
z (t) = v0 t ¡ g t2
2: (2.8)
The projectile reaches its maximum height h after a time T = v0=g and thus v0 = p 2 hg.
After a time 2T =q
8h=g, the projectile is back on the ground and has drifted by
y(2T ) = ¡ ! cos ¸µ
4 v0 T 2 ¡ 8g
3 T 3
¶ = ¡ 4
3 ! cos ¸
v30
g2 = ¡ 4
3 ! cos ¸
s 8 h3
g :
Since y(2T ) < 0, the drift is westward .
3