 PROGRAM OF “PHYSICS2B” Lecturer: Dr. DO Xuan Hoi Room A1. 413

Slides:



Advertisements
Similar presentations
Lecture 20 Relativistic Effects Chapter Outline Relativity of Time Time Dilation Length Contraction Relativistic Momentum and Addition of Velocities.
Advertisements

Classical Relativity Galilean Transformations
Physics Lecture Resources
Caroline Chisholm College
relativity Quantum Classic physics Modern physics.
Theory of Special Relativity
Cutnell/Johnson Physics 7th edition
Relativity Theories. The Principle of Relativity Although motion often appears relative, it’s logical to identify a “background” reference frame from.
 PROGRAM OF “PHYSICS” Lecturer: Dr. DO Xuan Hoi Room 413
Special Relativity Lecture 24 F2013 The Postulates Phenomenology The proper frame Time Length Mass energy Measuring events Lorentz transformations 1.
 PROGRAM OF “PHYSICS” Lecturer: Dr. DO Xuan Hoi Room 413
1 Special Relativity (Ch 37) Modern physics special relativity quantum mechanics Both were developed to explain the “few remaining puzzles” of classical.
SPECIAL RELATIVITY -Postulates of Special Relativity -Relativity of time –> time dilation -Relativity of length –> length contraction © 2005.
Inflation, vacua and the end of the Universe.
Principle of special relativity Their is inconsistency between EM and Newtonian mechanics, as discussed earlier Einstein proposed SR to restore the inconsistency.
Relativity Chapter 26. Introduction Major Physics accomplishments by the end of the 19 th century –Newton’s laws –Universal gravitation –Kinetic-molecular.
Special Relativity & General Relativity
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 29 Physics, 4 th Edition James S. Walker.
Chapter 29 Relativity.
Why does the mud fly off the tires of a pickup traveling down the interstate? Copernicus had difficulty convincing his peers of the validity of his heliocentric.
Physics 213 General Physics Lectures 20 & Last Meeting: Optical Instruments Today: Optics Practice Problems, Relativity (over two lectures)
Chapter 26 Relativity. General Physics Relativity II Sections 5–7.
 PROGRAM OF “PHYSICS2B” Lecturer: Dr. DO Xuan Hoi Room A1.413
Introduction to special relativity
Special Theory of Relativity
S-164 Countdown G minus 15 and counting. Relativity AP Physics Supplemental.
Page 1 Phys Baski Relativity I Topic #9: Special Relativity I Transformation of Variables between Reference Frames –Non-relativistic Galilean Transformation.
Special relativity.
The Special Theory of Relativity. Galilean-Newtonian Relativity Definition of an inertial reference frame: One in which Newton’s first law is valid Earth.
NS 1300 Dr. Hoge.  Can we slow light down?  Can we make things invisible?  Is it possible to travel faster than the speed of light?  Is faster than.
Chapter 26 Relativity © 2006, B.J. Lieb
Special Relativity Contents: The End of Physics Michelson Morley Postulates of Special Relativity Time Dilation.
 Newtonian relativity  Michelson-Morley Experiment  Einstein ’ s principle of relativity  Special relativity  Lorentz transformation  Relativistic.
Relativity Introduction 14.1 Introduction Electrons can be accelerated to 0.99c using a potential difference of 3.1 MV According to Newtonian Mechanics,
Chapter 9 Relativity Basic Problems The formulation of Newtonian mechanics is based on our daily experience and observation. But, Newtonian mechanics.
USC2001 Energy Lecture 4 Special Relativity Wayne M. Lawton Department of Mathematics National University of Singapore 2 Science Drive 2 Singapore
PHYS 221 Recitation Kevin Ralphs Week 12. Overview HW Questions Chapter 27: Relativity – History of Special Relativity (SR) – Postulates of SR – Time.
The Theory of Special Relativity Ch 26. Two Theories of Relativity Special Relativity (1905) –Inertial Reference frames only –Time dilation –Length Contraction.
Chapter 28 Special Relativity Events and Inertial Reference Frames An event is a physical “happening” that occurs at a certain place and time. To.
Modern Physics Relativity 1 Space is defined by measurements of length and depends on what “ruler” is used to measure the length. Time is defined by measurements.
Relativity Jennifer Keehn. “I want to know how God created this world. I am not interested in this or that phenomena, in the spectrum of this or that.
Astronomy 1143 – Spring 2014 Lecture 18: Special Relativity.
Phy 107 Fall From Last Time Physics changed drastically in the early 1900’s Relativity one of the new discoveries –Changed the way we think about.
Chapter 7 Relativity n Special Theory of Relativity – Einstein 1905 – space contraction and time dilation n General Theory of Relativity – Einstein 1916.
My Chapter 26 Lecture.
Introduction Classical Physics Laws: Mechanics (Newton), Electromagnetism (Maxwell), Optics, Fluids,.. Etc. Modern Physics: What do we mean? Are the laws.
Special Relativity 1. Quiz 1.22 (10 minutes) and a few comments on quiz So far we know that Special Relativity is valid for all speeds. But it is.
Chapter 26 Relativity. General Physics Relative Motion (Galilean Relativity) Chapter 3 Section 5
Physics 1202: Lecture 19 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Unit 13 Relativity.
Consequences of Special Relativity Simultaneity: Newton’s mechanics ”a universal time scale exists that is the same for all observers” Einstein: “No universal.
Chapter 39 Relativity. A Brief Overview of Modern Physics 20 th Century revolution 1900 Max Planck Basic ideas leading to Quantum theory 1905 Einstein.
11.1 – Frames of Reference and Relativity
Chapter 1 Relativity 1.
Visual Guide to Special and General Relativity. This is about to get weird…
PHY 102: Lecture History 12.2 Events and Inertial Reference Frames 12.3 Postulates of Special Relativity 12.4 Relativity of Time: Time Dilation.
Relativity. Historical Development 1600s Newton discovered his laws of mechanics Applied to a wide variety of problems over the next two decades Worked.
By: Jennifer Doran. What was Known in 1900 Newton’s laws of motion Maxwell’s laws of electromagnetism.
Space and Time © 2014 Pearson Education, Inc..
11.1 – Frames of Reference and Relativity. Inertial Frame of Reference (IFOR) a frame of reference in which the law of inertia holds The FOR must be at.
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Chapter 28 Special Relativity Events and Inertial Reference Frames An event is a physical “happening” that occurs at a certain place and time. To.
Special Relativity I Today: Quiz Special Relativity
Chapter S2 Space and Time
Physics: Principles with Applications, 6th edition
Special Theory of Relativity (STR)
An Introduction To ‘High Speed’ Physics
PHYS 3700 Modern Physics Prerequisites: PHYS 1212, MATH Useful to have PHYS 3900 or MATH 2700 (ordinary differential equations) as co-requisite,
Physics 1161: PreLecture 26 Special Relativity 1.
Presentation transcript:

 PROGRAM OF “PHYSICS2B” Lecturer: Dr. DO Xuan Hoi Room A

ANALYTICAL PHYSICS 2B 03 credits (45 periods) Chapter 1 Geometric Optics Chapter 2 Wave Optics Chapter 3 Relativity Chapter 4 Quantum Physics Chapter 5 Nuclear Physics Chapter 6 The Standard Model of Particle Physics

References : Young and Freedman, University Physics, Volume 2, 12th Edition, Pearson/Addison Wesley, San Francisco, 2007 Halliday D., Resnick R. and Merrill, J. (1988), Fundamentals of Physics, Extended third edition. John Willey and Sons, Inc. Alonso M. and Finn E.J. (1992), Physics, Addison-Wesley Publishing Company Hecht, E. (2000), Physics. Calculus, Second Edition. Brooks/Cole. Faughn/Serway (2006), Serway’s College Physics, Brooks/Cole. Roger Muncaster (1994), A-Level Physics, Stanley Thornes.

astr.gsu.edu/hbase/HFrame.html ml

PHYSICS 2B Chapter 3 Relativity Einstein's Postulates Relativity of Time Intervals and of Length Relativistic Dynamics SPECIAL THEORY OF RELATIVITY GENERAL THEORY OF RELATIVITY Relativity of Simultaneity The Michelson-Morley experiment

Before the electromagnetic theory of light and Einstein's special theory of relativity became established, most physicists believed that the propagation of light waves occurred in a medium called the ether. A. SPECIAL THEORY OF RELATIVITY 1 The Michelson-Morley experiment The Michelson interferometer : to detect the motion of the earth through the ether: "negative-result" The ether has never been detected, and the concept has been abandoned; the speed of light is the same relative to all observers. This is part of the foundation of the special theory of relativity.

A Thought Experiment in Simultaneity 2 Relativity of Simultaneity CONCLUSION: Simultaneity is not an absolute concept; events that are simultaneous in one frame are not necessarily simultaneous in a second frame moving relative to the first.

3.1 Einstein's First Postulate (the principle of relativity) “The laws of physics are the same in every inertial frame of reference” (inertial frame of reference : no acceleration) 3 Einstein's Postulates

3.2 Einstein's Second Postulate “The speed of light in vacuum is the same in all inertial frames of reference and is independent of the motion of the source. ”

4 Relativity of Time Intervals A frame of reference S' moves along the common x-x' -axis with constant speed u relative to a frame S For S’ : Event 1 is when a flash of light from a light source leaves 0'. Event 2 is when the flash returns to 0' For S’ : The time interval :

For S : the round-trip distance is the longer distance 2l For S’ : The time interval : For S : The time interval

For S’ : The time interval : For S : The time interval :

For S’ : The time interval : For S : The time interval : In a particular frame of reference, suppose that two events occur at the same point in space. The time interval between these events, as measured by an observer at rest in this same frame is t0 t0. Then an observer in a second frame moving with constant speed u relative to the rest frame will measure the time interval to be  t, where  t > t0 t0 : time dilation Observers measure any clock to run slow if it moves relative to them t0 t0 : Proper time

PROBLEM 1 SOLUTION A muon decays with a mean lifetime of 2.20  s as measured in a frame of reference in which it is at rest. If a muon is moving at 0.990c (about 2.97  10 8 m/s) relative to the earth, what will you (an observer on earth) measure its mean lifetime to be? The mean lifetime of the muon in the earth frame (  t) is about seven times longer than in the muon's frame (  t 0 ).

PROBLEM 2 SOLUTION An airplane flies from San Francisco to New York (about 4800 km) at a steady speed of 300 m/s. How much time does the trip take, as measured by an observer on the ground ? By an observer in the plane ? The time interval measured by ground observers : The time interval in the airplane (proper time) :

5 Relativity of Length A frame of reference S' moves along the common x-x' -axis with constant speed u relative to a frame S For S’ : A light source to one end of a ruler and a mirror to the other end. The ruler is at rest in reference frame S', and its length in this frame is L0 L0. Then the time required for a light pulse to make the round trip from source to mirror and back is

For S : the ruler is moving to the right with speed u during this travel of the light pulse The length of the ruler in S is L, and the time of travel from source to mirror, as measured in S, is t1.t1. The total length of path d from source to mirror is The light pulse travels with speed c, so :

In the same way we can show that the time t2 t2 for the return trip from mirror to source : The total time for the round trip, as measured in S : The length of the ruler in S is l, and the time of travel from source to mirror, as measured in S, is  t 1 :

(Length contraction) Because : ( L < L 0 ) The length L measured in S, in which the ruler is moving, is shorter than the length L0 L0 measured in its rest frame S'. (A length measured in the frame in which the body is at rest is called a proper length; thus L0 L0 is a proper length in S')

PROBLEM 3 SOLUTION A spaceship flies past earth at a speed of 0.990c. A crew member on board the spaceship measures its length, obtaining the value 400 m. What length do observers measure on earth?

PROBLEM 4 SOLUTION A spacecraft flies past a planet A at a speed of 0.600c. A scientist on this planet measures the length of the moving spacecraft to be 74.0 m. The spacecraft later lands on A, and the same scientist measures the length of the now stationary spacecraft. What value does she get? The moving spacecraft appears to an observer on the planet to be shortened along the direction of motion.

6 Relativistic Dynamics 6.1 Relativistic Momentum and Relativistic Mass Classical momentum : Relativistic Momentum : (t0 (t0 : time required to travel the distance  x measured by an observer moving with the particle ) With m : rest mass Relativistic mass m rel : Relativistic Momentum :

6.2 Relativistic Energy Rest energy :  The relativistic generalization of Newton's second law  Relativistic Kinetic Energy Total energy :

 Total Energy and Relativistic Momentum (1) and (2) 

PROBLEM 5 SOLUTION A 60.0-kg person is standing at rest on level ground. How fast would she have to run to (a) double her total energy and (b) increase her total energy by a factor of 10?

PROBLEM 6 SOLUTION A proton (rest mass 1.67  kg) has total energy that is 4.00 times its rest energy. What are (a) the kinetic energy of the proton ; (b) the magnitude of the momentum of the proton ; (c) the speed of the proton?

PROBLEM 7 SOLUTION What is the speed of a particle whose kinetic energy is equal to (a) its rest energy and (b) five times its rest energy?

B General theory of relativity Gravitational property: Inertial property: Postulates of Einstein’s general theory of relativity:  All the laws of nature have the same form for observers in any frame of reference, whether accelerated or not.  Principle of equivalence: In the vicinity of any point, a gravitational field is equivalent to an accelerated frame of reference in the absence of gravitational effects.

The curvature of space–time: the presence of a mass causes a curvature of space–time in the vicinity of the mass, and this curvature dictates the space–time path that all freely moving objects must follow The curvature of space–time is so extreme that, within a certain distance from the center of the black hole, all matter and light become trapped. If the concentration of mass becomes very great (when a large star exhausts its nuclear fuel and collapses to a very small volume): a black hole.