Energy and momentum: Collisions and conservation laws.

Slides:



Advertisements
Similar presentations
Chapter 7 Collisions. If the sum of the external forces is zero, then PRINCIPLE OF CONSERVATION OF LINEAR MOMENTUM The total linear momentum of an isolated.
Advertisements

Mass energy equivalence
Section 2: Mass Defect and E=mc 2.  Since an atom is made of protons, neutrons, and electrons, you might expect the mass of the atom to be the same as.
7: Atomic and Nuclear Physics 7.3 Nuclear reactions, fission and fusion.
Conservation of Momentum
1 Chapter Six: Momentum and Collisions. 2 Momentum is the product of the mass of a body and its velocity. A body may be an assembly of particles. Such.
Momentum and Energy in Collisions. A 2kg car moving at 10m/s strikes a 2kg car at rest. They stick together and move to the right at ___________m/s.
Chapter 6 Momentum and Collisions. Momentum The linear momentum of an object of mass m moving with a velocity is defined as the product of the mass and.
Momentum Impulse, Linear Momentum, Collisions Linear Momentum Product of mass and linear velocity Symbol is p; units are kgm/s p = mv Vector whose direction.
LECTURE 6 RELATIVISTIC MOMENTUM AND ENERGY PHYS 420-SPRING 2006 Dennis Papadopoulos.
Announcements 12/5/11 Prayer Office hours: a. a.Today: Colton regular; Chris regular b. b.Wed: Colton none; Chris 5-7 pm Wednesday: Project Show & Tell.
PHY 1371Dr. Jie Zou1 Chapter 39 Relativity (Cont.)
Momentum is Conserved in an isolated system.
Be 8 Decay Mass Be 8 = u Mass He 4 = u Excess mass = 9.9x10 -5 u E released = D mc2 = (9.9x10 -5 u) c 2 (931.5 MeV/c 2 / u) =.0922 MeV.
Nuclear Physics E = mc 2. Outline Theory of Special Relativity Postulates E = mc 2 The Atom What makes up the atom? What holds the atom together? Quantum.
Aim: How can we explain Einstein’s energy-mass relationship? Do Now: In the nucleus of any atom, there exists protons that are tightly packed together.
Conservation of momentum is one of the most fundamental and most useful concepts of elementary physis Does it apply in special relativity? Consider the.
Physics Nuclear Physics: Binding Energy Science and Mathematics Education Research Group Supported by UBC Teaching and Learning Enhancement Fund
Chapter 7 Linear Momentum. Chapter Momentum Linear Momentum- product of mass times velocity p=mvp=momentum units=kg.m/sec Restate Newton’s second.
Physics Momentum: Collisions
Physics 2170 – Spring Special relativity Homework solutions are on CULearn Homework set 3 is on the website.
Science Starter A 2 kg object moving east at 12 m/s collides with a stationary 6 kg object. After the collision, the 2 kg object bounces west at 6 m/s.
Example 1 Conservation of Momentum Examples If the system includes both the man and the boy it is then an isolated, closed system and momentum is conserved.
Two small spheres of putty, A and B, of equal mass m, hang from the ceiling on massless strings of equal length. Sphere A is raised to a height h 0 as.
Monday, Feb. 16, 2015PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #8 Monday, Feb. 16, 2015 Dr. Jaehoon Yu Relativistic Energy.
Collisions.
4.3 Elastic and Inelastic collisions. Consider this… Think very carefully about a system composed of two objects that are on a collision course.
Chapter 9 - Collisions Momentum and force Conservation of momentum
Chapter 8 Conservation of Linear Momentum Linear momentum; Momentum conservation Impulse Total kinetic energy of a system March 9, 2010.
Physics 6.5.
Physics Lecture Andrew Brandt Monday February 1, 2010 Dr. Andrew Brandt HW1 Assigned due Weds 2/3/10 (you can turn it in on Feb.8, but.
Elastic and Inelastic Collisions. Elastic Collision If 2 colliding objects are very hard and no heat is produced in the collision, KE is conserved as.
Inelastic Collision An elastic collision is an encounter between two bodies in which the total kinetic energy of the two bodies after the encounter is.
Consequences of Special Relativity Simultaneity: Newton’s mechanics ”a universal time scale exists that is the same for all observers” Einstein: “No universal.
Chapter 7 Linear Momentum. Objectives: Students will be able to: Explain that a conserved quantity is a quantity that remains numerically constant. Define.
2D Collisions Physics 12 Adv.
 car crashes car crashes 
1. What is the difference in elastic and inelastic collisions?
Motion 3.2 Solving Collision & Explosion Problems
Essential idea: The relativity of space and time requires new definitions for energy and momentum in order to preserve the conserved nature of these laws.
1 Relativity H6: Relativistic momentum and energy.
Relativistic Mechanics Momentum and energy. Momentum p =  mv Momentum is conserved in all interactions.
PHYS344 Lecture 7 Problem set 2 due on Wednesday the 16 th in class. Krane, Chapter 2: Problems 25, 26, 32, 33, 37, 39, 40, 41, 42 We will cover relativistic.
Relativistic Momentum p  mu/[(1 – (u/c) 2 ] 1/2 =  mu   1     
Elastic and Inelastic Collisions
Momentum Mo or . What is Momentum? A quantity of motion Tells that an object is on the move and hard to stop Mass in motion.
1. What is the difference in elastic and inelastic collisions?
Course Business: PHYS344 Lecture 6
Relativity of Mass According to Newtonian mechanics the mass of a body is unaffected with change in velocity. But space and time change…….. Therefore “mass”
Elastic Collisions.
Aim: How do we Analyze elastic collisions?
9.8 Momentum and Kinetic Energy in Collisions
Purpose: Definition of oblique collison.
Day Topic: Conservation of Momentum
Linear Momentum and Collisions
PHYSICS 103: Lecture 13 Review of HW Momentum Agenda for Today:
Mass and relativity mass measures resistance to changing the velocity
Momentum.
Energy and momentum units in particle physics
Momentum and Impulse HMH Physics Chapter 6 pages
Momentum Conservation: Review
Relativistic Momentum
MOMENTUM (p) is defined as the product of the mass and velocity -is based on Newton’s 2nd Law F = m a F = m Δv t F t = m Δv IMPULSE MOMENTUM.
Linear Momentum.
Conservation Laws Conservation of Momentum I
Momentum, Mass, and Velocity
Collisions Chapter 7.5.
Special Relativity Chapter 1-Class6.
Collisions Ms. Jeffrey- Physics.
Mass and Energy Suppose your internship is to ship a jack-in-the box to every person on earth. Should you ship them open or closed? You find that.
Presentation transcript:

Energy and momentum: Collisions and conservation laws

Rest Energy is real: Nuclear fission Initial mass of a neutron and a 235 U nucleus. Final products have less mass, but much more kinetic energy. Conversion of mass to kinetic energy. Oh yes, and more neutrons, so the reaction can run wild (chain reaction!). Protons: U=92, Ba = 56, Kr=36

Suppose that isolated object A has rest mass = 9m 0 and speed v A =0.8c (  A =5/3). Object B has mass 12m 0 and speed v B =−0.6c (  B =5/4). The objects collide and stick together (completely inelastic collision) From Physics 1110 we know all collisions conserve momentum A relativistic inelastic collision How about energy conservation? A)The above collision will conserve total kinetic energy B)The above collision will conserve total rest energy E rest =m A c 2 + m B c 2 C)The above collision will conserve total energy E total =  A m A c 2 +  B m B c 2 D)It is an inelastic collision so heat will be generated. None of the above will hold.

Classically, what is the total initial momentum? Let’s start with momentum conservation. What is the total relativistic momentum? So it does not end at rest as predicted classically! Suppose that object A has rest mass = 9m 0 and speed v A =0.8c (  A =5/3). Object B has mass 12m 0 and speed v B =−0.6c (  B =5/4). A relativistic inelastic collision Momentum conservation gives us: Remember that m f may not be m A +m B as it would be classically.

Now let’s look at the total energy. The initial energy is So conservation of energy gives us: Dividing these two equations: or so Furthermore: conservation of energy equation for m f : so we can solve the Object A has rest mass = 9m 0 and speed v A =0.8c (  A =5/3). Object B has mass 12m 0 and speed v B =−0.6c (  B =5/4). A relativistic inelastic collision

Classically, total momentum is 0 but in reality it is Classically, but in reality, so 8.85m 0 of mass is gained! So the change in KE is The initial and final kinetic energies are: The “lost” kinetic energy appears as gained mass in the total energy A relativistic inelastic collision

Really, mass gets created! CERN in Geneva, Switzerland Before the LHC (Large Hadron Collider) CERN operated LEP, the Large Electron-Positron collider in the same underground tunnel. Electron and positrons have a mass of 9x kg. They were accelerated to very high energies so when they annihilate, they create a Z 0 particle with a mass of 1.6x kg.

8 A proton has a mass of 938 MeV/c 2. What is this in kg? An important unit of energy is the electron-volt (eV). It’s the energy obtained by an electron moving through 1 V. It is not an SI unit but is very common. ΔE = qΔV = 1 eV = C 1 V = J Also use eV/c or MeV/c units for momentum Since mc 2 is a unit of energy, dividing energy by c 2 gives a unit of mass. Also, dividing energy by c gives a unit of momentum.

At what speed is the total energy of a particle equal to twice its rest mass energy? A. 0 B. 0.7c C. 0.87c D. 0.94c E. c To have total energy equal to twice the rest mass energy, need  =2 Solve for . so you need to be moving pretty fast to get your kinetic energy close to your rest mass energy!