General Relativity 05/12/2008. Lecture 15 1

Similar documents
Kepler's Three LAWS. Universal Gravitation Chapter 12. Heliocentric Model. Geocentric Model. Other Models. Johannes Kepler

Section 4.8. D v(t j 1 ) t. (4.8.1) j=1

An Introduction to General Relativity

Lecture 5. Today: Motion in many dimensions: Circular motion. Uniform Circular Motion

Physics 201 Lab 3: Measurement of Earth s local gravitational field I Data Acquisition and Preliminary Analysis Dr. Timothy C. Black Summer I, 2018

13.4 Work done by Constant Forces

NOT TO SCALE. We can make use of the small angle approximations: if θ á 1 (and is expressed in RADIANS), then

Dynamics Applying Newton s Laws Accelerated Frames

Math 8 Winter 2015 Applications of Integration

The Properties of Stars

Dynamics: Newton s Laws of Motion

Kinematics equations, some numbers

Section 14.3 Arc Length and Curvature

In-Class Problems 2 and 3: Projectile Motion Solutions. In-Class Problem 2: Throwing a Stone Down a Hill

PHYSICS 211 MIDTERM I 21 April 2004

A5682: Introduction to Cosmology Course Notes. 4. Cosmic Dynamics: The Friedmann Equation. = GM s

Recitation 3: More Applications of the Derivative

Week 10: Line Integrals

4 The dynamical FRW universe

Answers to the Conceptual Questions

The Form of Hanging Slinky

THREE-DIMENSIONAL KINEMATICS OF RIGID BODIES

7.1 Integral as Net Change and 7.2 Areas in the Plane Calculus

Section 6: Area, Volume, and Average Value

Classical Mechanics. From Molecular to Con/nuum Physics I WS 11/12 Emiliano Ippoli/ October, 2011

UNIFORM CONVERGENCE. Contents 1. Uniform Convergence 1 2. Properties of uniform convergence 3

Density of Energy Stored in the Electric Field

( dg. ) 2 dt. + dt. dt j + dh. + dt. r(t) dt. Comparing this equation with the one listed above for the length of see that

Chapter 4 Contravariance, Covariance, and Spacetime Diagrams

Terminal Velocity and Raindrop Growth

4-6 ROTATIONAL MOTION

Mathematics of Motion II Projectiles

The momentum of a body of constant mass m moving with velocity u is, by definition, equal to the product of mass and velocity, that is

+ x 2 dω 2 = c 2 dt 2 +a(t) [ 2 dr 2 + S 1 κx 2 /R0

CHAPTER 5 Newton s Laws of Motion

AP Physics 1. Slide 1 / 71. Slide 2 / 71. Slide 3 / 71. Circular Motion. Topics of Uniform Circular Motion (UCM)

Physics 161: Black Holes: Lecture 6: 14 Jan 2011

p(t) dt + i 1 re it ireit dt =

JURONG JUNIOR COLLEGE

A Vectors and Tensors in General Relativity

Problems for HW X. C. Gwinn. November 30, 2009

Sample Problems for the Final of Math 121, Fall, 2005

Infinite Geometric Series

Today in Astronomy 142: general relativity and the Universe

Prep Session Topic: Particle Motion

(3.2.3) r x x x y y y. 2. Average Velocity and Instantaneous Velocity 2 1, (3.2.2)

Lecture 1: Introduction to integration theory and bounded variation

PHYS 4390: GENERAL RELATIVITY LECTURE 6: TENSOR CALCULUS

KINEMATICS OF RIGID BODIES

Phys101 Lecture 4,5 Dynamics: Newton s Laws of Motion

Motion. Acceleration. Part 2: Constant Acceleration. October Lab Phyiscs. Ms. Levine 1. Acceleration. Acceleration. Units for Acceleration.

Review: Velocity: v( t) r '( t) speed = v( t) Initial speed v, initial height h, launching angle : 1 Projectile motion: r( ) j v r

Model Solutions to Assignment 4

Student Session Topic: Particle Motion

Centre of Mass, Moments, Torque

The area under the graph of f and above the x-axis between a and b is denoted by. f(x) dx. π O

PhysicsAndMathsTutor.com

Abstract. Introduction

Homework # 4 Solution Key

ME 141. Lecture 10: Kinetics of particles: Newton s 2 nd Law

1. A 4.00-kg stone is whirled at the end of a 2.00-m rope in a horizontal circle at a speed of 15.0 m/s. Ignoring the gravitational effects;

1 Probability Density Functions

Line and Surface Integrals: An Intuitive Understanding

Your Thoughts. Mechanics Lecture 16, Slide 1

Math 4310 Solutions to homework 1 Due 9/1/16

Intermediate Math Circles Wednesday, November 14, 2018 Finite Automata II. Nickolas Rollick a b b. a b 4

Physics 319 Classical Mechanics. G. A. Krafft Old Dominion University Jefferson Lab Lecture 2

INTRODUCTION. The three general approaches to the solution of kinetics problems are:

and that at t = 0 the object is at position 5. Find the position of the object at t = 2.

The First Fundamental Theorem of Calculus. If f(x) is continuous on [a, b] and F (x) is any antiderivative. f(x) dx = F (b) F (a).

a < a+ x < a+2 x < < a+n x = b, n A i n f(x i ) x. i=1 i=1

Gravitation (Symon Chapter Six)

Lecture XVII. Vector functions, vector and scalar fields Definition 1 A vector-valued function is a map associating vectors to real numbers, that is

Practive Derivations for MT 1 GSI: Goni Halevi SOLUTIONS

- 5 - TEST 2. This test is on the final sections of this session's syllabus and. should be attempted by all students.

MAT187H1F Lec0101 Burbulla

The Regulated and Riemann Integrals

Simulation of Eclipsing Binary Star Systems. Abstract

A little harder example. A block sits at rest on a flat surface. The block is held down by its weight. What is the interaction pair for the weight?

Improper Integrals, and Differential Equations

State space systems analysis (continued) Stability. A. Definitions A system is said to be Asymptotically Stable (AS) when it satisfies

Conservation Law. Chapter Goal. 5.2 Theory

Answers to selected problems from Essential Physics, Chapter 3

3 x x x 1 3 x a a a 2 7 a Ba 1 NOW TRY EXERCISES 89 AND a 2/ Evaluate each expression.

Chapter E - Problems

HW Solutions # MIT - Prof. Kowalski. Friction, circular dynamics, and Work-Kinetic Energy.

16 Newton s Laws #3: Components, Friction, Ramps, Pulleys, and Strings

Jackson 2.26 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell

_3-----"/- ~StudI_G u_id_e_-..,...-~~_~

Introduction to Mechanics Practice using the Kinematics Equations

PHYS Summer Professor Caillault Homework Solutions. Chapter 2

ES 111 Mathematical Methods in the Earth Sciences Lecture Outline 1 - Thurs 28th Sept 17 Review of trigonometry and basic calculus

Lecture 3. Limits of Functions and Continuity

Math 124A October 04, 2011

Name Solutions to Test 3 November 8, 2017

Physics 105 Exam 2 10/31/2008 Name A

20 MATHEMATICS POLYNOMIALS

We divide the interval [a, b] into subintervals of equal length x = b a n

Chapter 0. What is the Lebesgue integral about?

Equations of Motion. Figure 1.1.1: a differential element under the action of surface and body forces

Transcription:

So Fr, We Hve Generl Reltivity Einstein Upsets the Applecrt Decided tht constnt velocity is the nturl stte of things Devised nturl philosophy in which ccelertion is the result of forces Unified terrestril nd celestil mechnics & brought order to the Universe Spring 2008 2 Frmes of Reference Science is Frught with Assumptions This is ll fine, but ccelerting with respect to wht?? Why the Erth, of course! The Erth is t the center of the universe... The Erth is t the center of the solr system... The world is flt... The geometry of the Universe is flt... The surfce of the Erth is the nturl reference frme... Time nd spce re independent concepts These ssumptions cn hve drmtic impct on our views of Nture Spring 2008 3 Spring 2008 4 Lecture 15 1

Recll the Rotting Drum Exmple An ccelerting frme of reference feels lot like grvity In fct, it feels exctly like grvity The essence of Generl Reltivity is the recognition tht grvittionl force is n rtifct of doing physics in prticulr reference frme! Imgine Being in Cr Windows re pinted blck Move the cr to outer spce Now imgine plcing few objects on the dshbord of this blcked-out cr, still in outer spce. If the cr ccelertes forwrd, wht hppens to these objects on the dshbord? (Why?) If you didn t know the cr ws ccelerting, wht would you infer bout force cting on the objects? How would tht force depend on the msses of the objects? Spring 2008 5 Spring 2008 6 Grvity vs. Accelertion Cn you tell the difference between forwrd ccelertion nd grvity from str being brought up behind the cr? Cn you tell the difference between grvity nd ccelertion? Spring 2008 7 Spring 2008 8 Lecture 15 2

Constnt Velocity Elevtor An Exercise Chnging Your Perspective Close your eyes nd imgine you re being ccelerted upwrds by the room round us Accelerting Elevtor The nturl (i.e. inertil) coordinte systems re flling pst you t 9.8 m/s 2! You re being ccelerted upwrds t 9.8 m/s 2 by the norml force of the set you re in. Spring 2008 9 Spring 2008 10 A Conclusion: Doing Newtonin mechnics in non-inertil frme of reference cn force you to invoke fictitious-forces, relly just unexpected forces, i.e., rtifcts from doing physics in tht frme. Since these fictitious-forces re invoked to explin wht is ctully n ccelertion of the entire reference frme, they re necessrily proportionl to mss. Do you understnd why? Exmples: Centrifugl force in rotting systems Actully n exmple of grvity in the theory of Generl Reltivity Grvity! Spring 2008 11 Einstein in n Elevtor Film clip from Nov/PBS http://www.pbs.org/wgbh/nov/einstein/rel-i.html Spring 2008 12 Lecture 15 3

Wht s left?! If we blme grvity on our doing physics in the wrong reference frme, is ll of grvittionl physics wiped out? No! There is still n interction there, just more subtle thn Newton thought... Newton couldn t explin wht grvity ws Thought of it s instntneous ction t distnce Wht s wrong with ction t distnce? Mttress Exmple Imgine 2 bowling blls on mttress, on erth As they roll round on the mttress, they mke dimples in its surfce If they get close to ech other, they roll into ech other s dimples they re ttrcted to ech other Spring 2008 13 Spring 2008 14 Bowling Blls on Mttress Grvity = Geometricl Distortions Film clip from Nov/PBS http://www.pbs.org/wgbh/nov/einstein/rel-i.html Spring 2008 15 Spring 2008 16 Lecture 15 4

A Geometricl Approch Mss tells spce-time how to curve Spce tells mss how to move This nturlly explins the Universlity of Free Fll Accelertion All objects move long the sme geometricl distortions Grvity is property of the geometry of spcetime How fst re you moving? If time is dimension like spce, then how mny meters long is one second: Answer: 300,000,000 meters: c = 300,000,000 m/s Then in ech second, we re trveling 300,000 km through the time dimension! We re ll going t the speed of light! If we ccelerte ourselves to substntil speed through spce, we give up some of our speed in the time dimension: our clock runs slower compred to sttionry observer our totl speed through spcetime is lwys c Spring 2008 17 Spring 2008 18 Mss Tells Spce-Time How to Curve The illustrtions you ve seen re wht would occur if the world were 2-dimensionl. This llows us to show the curvture in the 3 rd dimension. In relity, grvity cuses 3 sptil nd 1 time dimensions to curve, which is tough to visulize! Spce Tells Mss How to Move Objects trvel long stright lines in curved spcetime. They don t ccelerte due to grvity Spring 2008 19 Curvture in this room! Spce (spcetime for tht mtter) seems flt to us Curvture is smll Strength of reltivity in this room is given by 2GM/(Rc 2 ), roughly 1.4 10-9 Ner sun, this is bout 10-6 Actul rdius of curvture on erth is bout one lightyer Is there some wy to mesure curved spce? Yes! Orbiting stellites with gyroscopes Spring 2008 20 Lecture 15 5

The Curvture of Spce is Rel It hs been mesured: GR is right! How? Curved Spce is Rel (Prt Deux) Orbiting gyroscope (Grvity probe B, nd others) Tips becuse spce is curved, just like the rrow before Northern ltitude line Equtor L gyroscope xis rottes Spring 2008 21 Spring 2008 22 Quntifying curvture Let s tke projectile trveling stright up initil speed v (up) mens hng time is t=2v/g height cquired is h = g( t/2) 2 = v 2 /g in this time, we trvel c t = 2vc/g meters through the time dimension If we drew n rc of height h nd length 2vc/g, we would find tht its rdius ws R = c 2 /g 1 light yer note this is independent of initil velocity (could be bullet or superbll) spce time Spring 2008 23 A Contemporry View Curved Spcetime forms stge on which other physics hppens Generl Reltivity (GR) is very successful description of the interction between spcetime nd objects GPS wouldn t work without it Einstein s Field Eqution: (just for fun ) Einstein Tensor describing how spcetime is curved G = 8 T + Cosmologicl Constnt: Einstein s Biggest Blunder (resurrected s drk energy) Stress-Energy Tensor describing distribution of mss nd energy Spring 2008 24 Lecture 15 6

A Genuine Scientific Revolution The Generl Reltivity view Relegted grvity to the interction between mss nd spcetime Abolished the notion tht the geometry of spcetime is everywhere flt Mixed the concepts of spce nd time GR does not men everything is reltive! The bsic concept is tht the equtions/lws tht describe physicl systems should not depend on your reference frme. Coordinte Invrince would be better term... Einstein wnted to cll it The Theory of Invrints References nd Assignments References dmoz.org/science/physics/reltivity/overviews/ especilly links titled Generl Reltivity Reltivity Visulized, by L. C. Epstein gret intuitive development, low mth (low PC lso) Assignments Red Hewitt Chpters 35 nd 36 HW5: 9.R.13, 9.E.9, 9.E.14, 9.E.43, 9.P.7, 10.E.16, 35.R.27, 35.E.6, 35.E.19, 35.E.20, 35.E.37, 35.P.3, 35.P.10, 36.R.7, 36.E.2, 36.E.6 Spring 2008 25 Spring 2008 26 Lecture 15 7