22
ACCESS– Summer 2014 Elastic and Inelastic Collisions - Numerical Integration Gernot Laicher University of Utah - Department of Physics & Astronomy

ACCESS– Summer 2014 Elastic and Inelastic Collisions - Numerical Integration

  • Upload
    jenski

  • View
    29

  • Download
    0

Embed Size (px)

DESCRIPTION

ACCESS– Summer 2014 Elastic and Inelastic Collisions - Numerical Integration. Gernot Laicher University of Utah - Department of Physics & Astronomy. - PowerPoint PPT Presentation

Citation preview

Page 1: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

ACCESS– Summer 2014

Elastic and Inelastic Collisions - Numerical Integration

Gernot LaicherUniversity of Utah - Department of Physics & Astronomy

Page 2: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Newton’s second law

…..or in a more general form

Momentum

m=constant “original” form of Newton’s second law.

Page 3: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Re-arrange Newton’s second law

“A net Force Fnet applied for an infinitesimally small time interval dt results in a change of momentum dp.”

Page 4: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Net force applied over a time interval (tf-ti)

“Impulse” or “Impulse Integral” I

Newton’s second law :

“Impulse = Change of Momentum”.

Page 5: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Example:

A golf ball (m=46g) is struck by a club which applies a constant force of 200N for a time period of 1/100 of a second. What is the impulse on the golf ball? If the ball is at rest initially, how fast will it be after it has been hit?

Page 6: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Change in momentum equals impulse

Page 7: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Conservation of Momentum:

For a “closed system” (no external forces applied to the system) the total linear momentum of the system is conserved. (The sum of all the individual momenta of the pieces that make up the “system” remains constant.)

To approach a system with no applied external force, we can consider two gliders on an air track and just look at the linear momentum in the horizontal direction.

Page 8: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Demo: One glider is initially at rest; both gliders have equal mass.

Page 9: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Before the collision:

Total momentum:

V1i V2i = 0

Page 10: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

After the collision:

Total momentum:

V2f = V1i V1f = 0

Page 11: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Mechanical energy of the system before and after the collision:

Mechanical energy was conserved

” Totally elastic collision”

Page 12: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Before the collision:

After the collision:

V2i = 0 V1i

Vf = ½ V1i

Page 13: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Mechanical energy of the system:

Half the mechanical energy “lost” in collision (converted to heat) Inelastic collision

Page 14: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Numerical Integration

In general, applied forces are not constant during collision:

Impulse = “Area” under the force-time curve (the integral).

Page 15: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

In lab activity: Force sensors Computer

Measurement not continuous - taken in discrete time intervals.

Estimate time integral with “numerical integration”.

Page 16: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Assume force remains constant over each time interval. Then calculate the sum of the rectangular areas (width ti and height Fi).

(Here, ti = t because we sample in equal time intervals.)

Page 17: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Alternative method: “Trapezoidal Rule”.

Partition area under the function into n intervals (widths δx). Label start of each partition as x0, x1, x2, x3, ... xn.

f(x)

Width of intervals

x xo x1 x2 x3 x4 x5 x6 x7 x8 x9

x

Page 18: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

More partitions smaller time intervals Connect with straight lines f(xi) and f(xi+1) Area approximated by sum of n trapezoid areas.

w=width of trapezoid (= δx)

c = length of the leg1= f(xi)

d = length of leg 2 = f(xi+1)

Page 19: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Area Ai of ith trapezoid

Total area Atotal

Page 20: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Example Using Trapezoidal Rule:

Integrate f(x) = x4 for 1 ≤ x ≤ 3 with n = 8.

The width δx of each partition is:

Page 21: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

x0 = 1.00 f(x0) = (1.00)4 = 1.0000

x1 = 1.25 f(x1) = (1.25)4 = 2.4414 (Rounding to 4 decimal places)

x2 = 1.50 f(x2) = (1.50)4 = 5.0625

x3 = 1.75 f(x3) = (1.75)4 = 9.3789

x4 = 2.00 f(x4) = (2.00)4 = 16.0000

x5 = 2.25 f(x5) = (2.25)4 = 25.6289

x6 = 2.50 f(x5) = (2.50)4 = 39.0625

x7 = 2.75 f(x7) = (2.75)4 = 57.1914

x8 = 3.00 f(x8) = (3.00)4 = 81.0000

Page 22: ACCESS–  Summer  2014 Elastic and Inelastic Collisions - Numerical Integration

Compared to exact result:

(Numerical integration within 1% of exact result)