- •Preface
- •Contents
- •1 Introduction
- •1.1 Physics
- •1.2 Mechanics
- •1.3 Integrating Numerical Methods
- •1.4 Problems and Exercises
- •1.5 How to Learn Physics
- •1.5.1 Advice for How to Succeed
- •1.6 How to Use This Book
- •2 Getting Started with Programming
- •2.1 A Python Calculator
- •2.2 Scripts and Functions
- •2.3 Plotting Data-Sets
- •2.4 Plotting a Function
- •2.5 Random Numbers
- •2.6 Conditions
- •2.7 Reading Real Data
- •2.7.1 Example: Plot of Function and Derivative
- •3 Units and Measurement
- •3.1 Standardized Units
- •3.2 Changing Units
- •3.4 Numerical Representation
- •4 Motion in One Dimension
- •4.1 Description of Motion
- •4.1.1 Example: Motion of a Falling Tennis Ball
- •4.2 Calculation of Motion
- •4.2.1 Example: Modeling the Motion of a Falling Tennis Ball
- •5 Forces in One Dimension
- •5.1 What Is a Force?
- •5.2 Identifying Forces
- •5.3.1 Example: Acceleration and Forces on a Lunar Lander
- •5.4 Force Models
- •5.5 Force Model: Gravitational Force
- •5.6 Force Model: Viscous Force
- •5.6.1 Example: Falling Raindrops
- •5.7 Force Model: Spring Force
- •5.7.1 Example: Motion of a Hanging Block
- •5.9.1 Example: Weight in an Elevator
- •6 Motion in Two and Three Dimensions
- •6.1 Vectors
- •6.2 Description of Motion
- •6.2.1 Example: Mars Express
- •6.3 Calculation of Motion
- •6.3.1 Example: Feather in the Wind
- •6.4 Frames of Reference
- •6.4.1 Example: Motion of a Boat on a Flowing River
- •7 Forces in Two and Three Dimensions
- •7.1 Identifying Forces
- •7.3.1 Example: Motion of a Ball with Gravity
- •7.4.1 Example: Path Through a Tornado
- •7.5.1 Example: Motion of a Bouncing Ball with Air Resistance
- •7.6.1 Example: Comet Trajectory
- •8 Constrained Motion
- •8.1 Linear Motion
- •8.2 Curved Motion
- •8.2.1 Example: Acceleration of a Matchbox Car
- •8.2.2 Example: Acceleration of a Rotating Rod
- •8.2.3 Example: Normal Acceleration in Circular Motion
- •9 Forces and Constrained Motion
- •9.1 Linear Constraints
- •9.1.1 Example: A Bead in the Wind
- •9.2.1 Example: Static Friction Forces
- •9.2.2 Example: Dynamic Friction of a Block Sliding up a Hill
- •9.2.3 Example: Oscillations During an Earthquake
- •9.3 Circular Motion
- •9.3.1 Example: A Car Driving Through a Curve
- •9.3.2 Example: Pendulum with Air Resistance
- •10 Work
- •10.1 Integration Methods
- •10.2 Work-Energy Theorem
- •10.3 Work Done by One-Dimensional Force Models
- •10.3.1 Example: Jumping from the Roof
- •10.3.2 Example: Stopping in a Cushion
- •10.4.1 Example: Work of Gravity
- •10.4.2 Example: Roller-Coaster Motion
- •10.4.3 Example: Work on a Block Sliding Down a Plane
- •10.5 Power
- •10.5.1 Example: Power Exerted When Climbing the Stairs
- •10.5.2 Example: Power of Small Bacterium
- •11 Energy
- •11.1 Motivating Examples
- •11.2 Potential Energy in One Dimension
- •11.2.1 Example: Falling Faster
- •11.2.2 Example: Roller-Coaster Motion
- •11.2.3 Example: Pendulum
- •11.2.4 Example: Spring Cannon
- •11.3 Energy Diagrams
- •11.3.1 Example: Energy Diagram for the Vertical Bow-Shot
- •11.3.2 Example: Atomic Motion Along a Surface
- •11.4 The Energy Principle
- •11.4.1 Example: Lift and Release
- •11.4.2 Example: Sliding Block
- •11.5 Potential Energy in Three Dimensions
- •11.5.1 Example: Constant Gravity in Three Dimensions
- •11.5.2 Example: Gravity in Three Dimensions
- •11.5.3 Example: Non-conservative Force Field
- •11.6 Energy Conservation as a Test of Numerical Solutions
- •12 Momentum, Impulse, and Collisions
- •12.2 Translational Momentum
- •12.3 Impulse and Change in Momentum
- •12.3.1 Example: Ball Colliding with Wall
- •12.3.2 Example: Hitting a Tennis Ball
- •12.4 Isolated Systems and Conservation of Momentum
- •12.5 Collisions
- •12.5.1 Example: Ballistic Pendulum
- •12.5.2 Example: Super-Ball
- •12.6 Modeling and Visualization of Collisions
- •12.7 Rocket Equation
- •12.7.1 Example: Adding Mass to a Railway Car
- •12.7.2 Example: Rocket with Diminishing Mass
- •13 Multiparticle Systems
- •13.1 Motion of a Multiparticle System
- •13.2 The Center of Mass
- •13.2.1 Example: Points on a Line
- •13.2.2 Example: Center of Mass of Object with Hole
- •13.2.3 Example: Center of Mass by Integration
- •13.2.4 Example: Center of Mass from Image Analysis
- •13.3.1 Example: Ballistic Motion with an Explosion
- •13.4 Motion in the Center of Mass System
- •13.5 Energy Partitioning
- •13.5.1 Example: Bouncing Dumbbell
- •13.6 Energy Principle for Multi-particle Systems
- •14 Rotational Motion
- •14.2 Angular Velocity
- •14.3 Angular Acceleration
- •14.3.1 Example: Oscillating Antenna
- •14.4 Comparing Linear and Rotational Motion
- •14.5 Solving for the Rotational Motion
- •14.5.1 Example: Revolutions of an Accelerating Disc
- •14.5.2 Example: Angular Velocities of Two Objects in Contact
- •14.6 Rotational Motion in Three Dimensions
- •14.6.1 Example: Velocity and Acceleration of a Conical Pendulum
- •15 Rotation of Rigid Bodies
- •15.1 Rigid Bodies
- •15.2 Kinetic Energy of a Rotating Rigid Body
- •15.3 Calculating the Moment of Inertia
- •15.3.1 Example: Moment of Inertia of Two-Particle System
- •15.3.2 Example: Moment of Inertia of a Plate
- •15.4 Conservation of Energy for Rigid Bodies
- •15.4.1 Example: Rotating Rod
- •15.5 Relating Rotational and Translational Motion
- •15.5.1 Example: Weight and Spinning Wheel
- •15.5.2 Example: Rolling Down a Hill
- •16 Dynamics of Rigid Bodies
- •16.2.1 Example: Torque and Vector Decomposition
- •16.2.2 Example: Pulling at a Wheel
- •16.2.3 Example: Blowing at a Pendulum
- •16.3 Rotational Motion Around a Moving Center of Mass
- •16.3.1 Example: Kicking a Ball
- •16.3.2 Example: Rolling down an Inclined Plane
- •16.3.3 Example: Bouncing Rod
- •16.4 Collisions and Conservation Laws
- •16.4.1 Example: Block on a Frictionless Table
- •16.4.2 Example: Changing Your Angular Velocity
- •16.4.3 Example: Conservation of Rotational Momentum
- •16.4.4 Example: Ballistic Pendulum
- •16.4.5 Example: Rotating Rod
- •16.5 General Rotational Motion
- •Index
Chapter 13
Multiparticle Systems
So far we have studied the motion of objects, but we have not been very precise in deÞning an object. What we really have studied is the motion of mass-points, particles, or extended objects that move as a particle. What does it mean to move as a particle? It means that all the points in the object move with the same velocity and the same acceleration, the whole object is translated as a stiff (rigid) body: The various parts of the object are not moving relative to each other.
But this does not seem to be a good description of everyday phenomena around us. If you are running, you are surely not moving both your arms and your legs with the same velocity and acceleration all the time. And if you throw a ball, it may wobble and spin on its path. Even on the microscopic level objects are not only translated: Molecules may vibrate, spin, or wobble as they move. When the world is so complex, can we still use the simple descriptions and models we have developed so far, or do we have to describe the motion of each small part of the object independently?
Fortunately, we are saved by NewtonÕs third law: If we only deÞne the position of the object in a particular way, by deÞning the position of the object as its center of mass, NewtonÕs second law is valid for any system of particles, and therefore for any object. This wonderful consequence of NewtonÕs second and third laws allows us to use the force models and the concepts we have developed so far also to address extended objects. The motion of an object is further simpliÞed if the object is a rigid body: An object where the relative positions of any two points do not change, that is, the object is only translated and rotated, but does not change shape, stretch, or otherwise deform during its motion.
In this chapter, we discuss the motion of systems of particlesÑmultiparticle systems. Before we proceed to describe the motion of rigid bodies in Chaps. 15 and 16, we Þrst introduce a general description of rotational motion in Chap. 14.
13.1 Motion of a Multiparticle System
Let us start describing a system of many particles. For most practical purposes, two particles are many particles, but we are ambitious and start with a system of N particles. We number the particles using the index j running from 1 to N as
© Springer International Publishing Switzerland 2015 |
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A. Malthe-S¿renssen, Elementary Mechanics Using Python,
Undergraduate Lecture Notes in Physics, DOI 10.1007/978-3-319-19596-4_13
402
Fig. 13.1 The motion of a system of particles is described by the position r j of each of the N particles in the system. Here, the system consists of 5 particles
13 Multiparticle Systems
Fiext |
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illustrated in Fig. 13.1. The position of each particle is given in a coordinate system S as illustrated. The position of particle 1 as a function of time is r1(t ), and its mass is m1. Similarly, the position of particle j is r j and its mass is m j .
All the quantities we have deÞned so far are easily extended to each of these particles. For example, the velocity and acceleration of particle j is found from the derivatives of the position vector:
v j |
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and the momentum of particle j is p j = m j v j .
The motion of each particle is determined from the forces acting on it. In our discussion of momentum, we already discussed that the forces acting on particle j may be either from one of the other particles in the system, or from the environment. Forces from other particles in the system are called internal forces, and forces from the environment are called external forces. NewtonÕs second law for particle i is therefore:
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where F j,i is the force from particle j on particle i .
In order to Þnd the motion of one of the particles inside the system, we need to know both the external forces acting on this particle and the forces from the other particles in a system. This may require a complicated force model, for example, consider the forces acting between two parts of a tennis ball as the ball wiggles and rotates. Often, we are not interested in the detailed motion of particles inside a system, but only in the motion of the system as a whole. We can address this by
adding together (13.2) for each particle i , getting: |
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13.1 Motion of a Multiparticle System |
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As we noticed when we discussed the total momentum of a system of particles, the sum of all the internal forces will always contain both the force F j,i and the force Fi, j . Since these two forces are action-reaction pairs, they are equal, but oppositely directed. Therefore, every such pair will cancel. The sum of all the internal forces is therefore zero!
If we introduce P = i pi as the total momentum of the system, we Þnd: |
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This looks a lot like NewtonÕs second law, but now for the system of particles. We can make this similarity even stronger by introducing the velocity V of the system so that:
P = M V = |
pi = mi vi , |
(13.5) |
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i |
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where M = i mi is the total mass of the system.
Notice that this is a definition of the velocity V of the system. We deÞne it this way to be able to write the total momentum, P, of the system in the intuitive way P = M V. From (13.5) we Þnd:
V = |
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mi vi . |
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What is the acceleration of the system? It is natural to deÞne the acceleration, A, of the system as the time derivative of the velocity V of the system:
d1
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Similarly, we deÞne the position of the system, R, as:
Center of mass: The effective position of the system, or the center of mass of the system, is deÞned as
1 |
mi ri , |
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i