Physics 2130: General Physics 3

Similar documents
Everything should be made as simple as possible, but not simpler -A. Einstein

Special relativity. Announcements:

Announcements. Today s class. The Lorentz transformation. Lorentz transformation (Relativistic version of Galileo transformation)

Einstein s theory of special relativity

General Physics I. Lecture 20: Lorentz Transformation. Prof. WAN, Xin ( 万歆 )

Lecture 4 Fields, Relativity

Chapter 36 Relativistic Mechanics

General Physics I. Lecture 17: Moving Clocks and Sticks. Prof. WAN, Xin ( 万歆 )

General Physics I. Lecture 18: Lorentz Transformation. Prof. WAN, Xin ( 万歆 )

SPH4U UNIVERSITY PHYSICS

Frames of Reference, Energy and Momentum, with

Lecture 13 Birth of Relativity

Relativity II. The laws of physics are identical in all inertial frames of reference. equivalently

Physics 280 Lecture 2

Reversal in time order of interactive events: Collision of inclined rods

The Magnetic Force. x x x x x x. x x x x x x. x x x x x x q. q F = 0. q F. Phys 122 Lecture 17. Comment: What just happened...?

Einstein s theory of special relativity

General Lorentz Boost Transformations, Acting on Some Important Physical Quantities

Special Theory of Relativity (I) Newtonian (Classical) Relativity. Newtonian Principle of Relativity. Inertial Reference Frame.

Special relativity. x' = x vt y' = y z' = z t' = t Galilean transformation. = dx' dt. = dx. u' = dx' dt'

10520EE Modern Physics Instructor: 陳明彰 LAs:??

Physics 1501 Lecture 28

Relativity III. Review: Kinetic Energy. Example: He beam from THIA K = 300keV v =? Exact vs non-relativistic calculations Q.37-3.

Transformation of Surface Charge Density in Mixed Number Lorentz Transformation

8.022 (E&M) Lecture 11

Dynamics ( 동역학 ) Ch.2 Motion of Translating Bodies (2.1 & 2.2)

UNDERSTAND MOTION IN ONE AND TWO DIMENSIONS

Electricity and Magnetism Relativity and the Magnetic Field

Modern Physics Part 2: Special Relativity

Problem Set 1: Solutions

So now that we ve mentioned these terms : kinetic, potential, work we should try to explain them more. Let s develop a model:

Physics 2A Chapter 3 - Motion in Two Dimensions Fall 2017

Kinematics of special relativity

Chapter 35. Special Theory of Relativity (1905)

4-vectors. Chapter Definition of 4-vectors

Fluid Physics 8.292J/12.330J

Relativistic Boats: an explanation of special relativity. Brianna Thorpe, Dr. Michael Dugger

Kinematic Physics for Simulation and Game Programming

Chapter 11 Collision Theory

Welcome back to PHY 3305

Class 1: Special Relativity

PH-101:Relativity and Quantum Mechanics

12:40-2:40 3:00-4:00 PM

2.1 The Ether and the Michelson-Morley Experiment

In special relativity, it is customary to introduce the dimensionless parameters 1

The Foundations of Special Relativity

Physics 2D Lecture Slides Lecture 2. March 31, 2009

Relativity. Overview & Postulates Events Relativity of Simultaneity. Relativity of Time. Relativity of Length Relativistic momentum and energy

Final Exam. conflicts with the regular time. Two students have confirmed conflicts with me and will take the

RELATIVISTIC DOPPLER EFFECT AND VELOCITY TRANSFORMATIONS

Therefore F = ma = ma = F So both observers will not only agree on Newton s Laws, but will agree on the value of F.

Would you risk your live driving drunk? Intro

8.20 MIT Introduction to Special Relativity IAP 2005 Tentative Outline

Physics 2D Lecture Slides Sept 29. Vivek Sharma UCSD Physics

CHAPTER 2 Special Theory of Relativity-part 1

) 2 = Square of rest energy. E = "m o. c 2, or E = mc 2. Homework & Exam

4/13/2015. Outlines CHAPTER 12 ELECTRODYNAMICS & RELATIVITY. 1. The special theory of relativity. 2. Relativistic Mechanics

Vector Basics. Lecture 1 Vector Basics

Physics 139 Relativity. Thomas Precession February 1998 G. F. SMOOT. Department ofphysics, University of California, Berkeley, USA 94720

Bell s spaceship paradox

Introduction to Special Relativity

Announcement. Einstein s Postulates of Relativity: PHYS-3301 Lecture 3. Chapter 2. Sep. 5, Special Relativity

Line Integrals and Path Independence

SPECIAL RELATIVITY. Chapter 28

PY1008 / PY1009 Physics Rotational motion

Modern Physics notes Paul Fendley Lecture 35. Born, chapter III (most of which should be review for you), chapter VII

Physics 2D Lecture Slides Lecture 1: Jan

Today: Review of SR. Einstein s Postulates of Relativity (Abbreviated versions) Let's start with a few important concepts

Module 2: Special Theory of Relativity - Basics

Modern Physics notes Spring 2006 Paul Fendley Lecture 35

THE FIFTH DIMENSION EQUATIONS

Purpose of the experiment

Special Relativity-General Discussion

Modern Physics notes Spring 2005 Paul Fendley Lecture 35

DO PHYSICS ONLINE. WEB activity: Use the web to find out more about: Aristotle, Copernicus, Kepler, Galileo and Newton.

PHY100S. PHY100S (K. Strong) - Lecture 15 - Slide 1.

The Dot Product Pg. 377 # 6ace, 7bdf, 9, 11, 14 Pg. 385 # 2, 3, 4, 6bd, 7, 9b, 10, 14 Sept. 25

Physics 1A. Lecture 3B

PHYS 100: Lecture 7. FRICTION and UNIFORM CIRCULAR MOTION. θ Mg. v R. R a. Static: Kinetic: Physics 100 Lecture 7, Slide 1

Lesson 7: Slopes and Functions: Speed and Velocity

Physics 225 Relativity and Math Applications. Fall Unit 7 The 4-vectors of Dynamics

Sept. 3, 2013 Math 3312 sec 003 Fall 2013

Introduction to Relativity & Time Dilation

What is allowed? relativity: physics is the same for all observers so light travels at the same speed for everyone. so what? THE UNIVERSITY OF ALABAMA

Your Comments. I don't understand how to find current given the velocity and magnetic field. I only understand how to find external force

Welcome back to PHY101: Major Concepts in Physics I. Photo: J. M. Schwarz

Chapter-1 Relativity Part I RADIATION

Consequences of special relativity.

a by a factor of = 294 requires 1/T, so to increase 1.4 h 294 = h

Einstein s theory of special relativity

General Physics I. Lecture 6: Conservation of Momentum. Prof. WAN, Xin 万歆.

E = mc 2. Inertial Reference Frames. Inertial Reference Frames. The Special Theory of Relativity. Slide 1 / 63. Slide 2 / 63.

Motion In Two Dimensions. Vectors in Physics

Accelerated Observers

Relativity. An explanation of Brownian motion in terms of atoms. An explanation of the photoelectric effect ==> Quantum Theory

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS AP PHYSICS

Physics 2D Lecture Slides Lecture 2. Jan. 5, 2010

Two postulates Relativity of simultaneity Time dilation; length contraction Lorentz transformations Doppler effect Relativistic kinematics

MA 1125 Lecture 15 - The Standard Normal Distribution. Friday, October 6, Objectives: Introduce the standard normal distribution and table.

Physics 2D Lecture Slides Sep 26. Vivek Sharma UCSD Physics

Transcription:

Phsics 2130: General Phsics 3 Lecture 8 Length contraction and Lorent Transformations. Reading for Monda: Sec. 1.13, start Chap. 2 Homework: HWK3 due Wednesda at 5PM.

Last Time: Time Dilation Who measures the Proper Time, Dt 0? One obserer with one clock who sees local eents at their location. That s Proper Time Obserers in other frames DON T measure Proper Time. More obserers are required. The see more time Dt pass: Dt Dt 0 1 1 c 2 2

Length of an object... -3-2 -1 0 1 2 3... This length, measured in the stick s rest frame, is its proper length. This stick is 3m long. I measure both ends at the same time in m frame of reference. Or not. It doesn t matter, because the stick isn t going anwhere. But as we know, at the same time is relatie it depends on how ou re moing.

Length of an object S... -3-2 -1 0 1 2 3... S 0 Another obserer comes whiing b at uniform elocit,. This obserer can measure the length of the stick, b measuring time. Eent 1 Origin of S passes left end of stick.

Length of an object S... -3-2 -1 0 1 2 3... S 0 Eent 1 Origin of S passes left end of stick. Eent 2 Origin of S passes right end of stick.

Length of an object S... -3-2 -1 0 1 2 3... S 0 Eent 1 Origin of S passes left end of stick. Eent 2 Origin of S passes right end of stick. How man obserers are needed in S to measure the time between eents? A) 0 B) 1 C) 2 D) 57

Length of an object S... -3-2 -1 0 1 2 3... S 0 Eent 1 Origin of S passes left end of stick. Eent 2 Origin of S passes right end of stick. Which frame measures the Proper Time between the eents? A) S B) S C) neither

The frames agree on relatie speed In frame S: length of stick = L (this is the proper length) time between measurments = Dt Relatie speed of frame S is = L/Dt In frame S : length of stick = L (this is what we re looking for) time between measurements = Dt Relatie speed of frame S is = L /Dt Q: a) Dt = Dt or b) Dt = Dt Follow the proper time!

A little math Speeds are the same (both refer to the relatie speed). And so L L L Dt Dt Dt L L Length measured in frame moing rel. stick Length in stick s rest frame (proper length) Length contraction is a consequence of time dilation (and ice-ersa).

Curl measures L C Larr measures L L Moe measures L M Curl runs b real fast with a stick he knows to be of length L C. Larr and Moe are both standing on the ground and each measures the stick as it goes b. How are the three measurements related? a) L C < L L < L M b) L C > L L > L M c) L C = L L = L M d) L C < L L = L M e) L C > L L = L M

Space-time ct A useful wa to isualie things in relatiit. Think of eents as four (x,,, ct) coordinates. x Suppose something is moing to the right in frame S. It starts at x=0 at t=0. It moes to positie x at positie time. Connect the dots this is the world line.

The Lorent transformation S S 0 A stick is at rest in S. Its endpoints are the eents (position, c*time) = (0,0) and (x,0) in S. S is moing to the right with respect to frame S. x Eent 1 left of stick passes origin of S. Its coordinates are (0,0) in S and (0,0) in S.

The Lorent transformation S x As iewed from S, the stick s length is x /. Then, time t passes. According to S, where is the right end of the stick? a) x = t b) x = -t c) x = t + x / d) x = -t + x / e) x = t x /

The Lorent transformation S x = t + x /. This relates the coordinates of an eent in one frame to its coordinates in the other. Algebra x = (x-t)

Transformations If S is moing with speed in the positie x direction relatie to S, then the coordinates of the same eent in the two frames is related b: In Galilean relatiit x t x t t In Special relatiit x t ( x ( t t) x 2 c ) In a minute Remark: this assumes (0,0) is the same eent in both frames.

The Lorent transformation 2 S S 0 A stick is at rest in S. Its endpoints are the eents (position, c*time) = (0,0) and (x,0) in S. S is moing to the left with respect to frame S. x Eent 1 left of stick passes origin of S. Its coordinates are (0,0) in S and (0,0) in S.

The Lorent transformation 2 0 As iewed from S, the stick s length is x/. Time t passes. According to S, where is the right end of the stick? a) x = t b) x = -t c) x = t + x/ d) x = -t + x/ e) x = t x/

The Lorent transformation 2 t x x x x t 0 x = -t + x/. This relates the coordinates of an eent in one frame to its coordinates in the other. Algebra t t x 2 c

Transformations t t t x x If S is moing with speed in the positie x direction relatie to S, then the coordinates of the same eent in the two frames is related b: In Galilean relatiit In Special relatiit ) ( ) ( 2 x c t t t x x Remark: this assumes (0,0) is the same eent in both frames. 2 ( ) ( ) x x t t t x c

Transformations We now hae the tools to compare positions and times in different inertial reference frames. NOW we can talk about how elocities, etc. compare.: In Galilean relatiit x t t x t Newton s Laws worked with these x t ( x ( t In Special relatiit t) c 2 x ) x ( xt) t ( t x) 2 c Newton s Laws need attention. Momentum and Energ definitions!