Elements of Physics II
|
|
- Evelyn Martin
- 5 years ago
- Views:
Transcription
1 Physics 132: Lecture 23 Elements of Physics II Agenda for Today Special Theory of relativity Inertial vs. non-inertial reference frames Postulates of SR Consequences of SR Time dilation Length contraction Physics 201: Lecture 1, Pg 1
2 Postulates of Special Relativity 1) The laws of Physics have the same form in all inertial reference frames. (Moving with constant velocity) Student: Why does all this weird stuff happen? 1B) The speed of light (in a vacuum) is always c, independent of the observer. Student: how is velocity of light constant irrespective of the position or relative velocity of the observer? Physics 201: Lecture 1, Pg 2
3 Example Event A occurs at spacetime coordinates x = 300 m, t = 2 s. Event B occurs at spacetime coordinates x = 1200 m, t =6 s s. Could A possibly be the cause of B? x tt 1200m -300m m/s 6μs 2μs Event C occurs at spacetime coordinates x = 2400 m, t = 8 s. Could A possibly be the cause of fc? x x t 2400m -300m m/s 8μs 2μs Physics 201: Lecture 1, Pg 3
4 Clicker Question 1: At t = 0 an alien spaceship passes by the earth: let this be event A. At t = 13 min (according to synchronized clocks on Earth and Mars) the spaceship passes by Mars, let this be event B. Who measures the proper length between event A and event B? (a) The alien spaceship Student: If the proper time is measured in the frame in which (b) People on Earth the two events happen in the (c) Nobody same place and the proper (d) People on Mars length is measured in the frame (e) Both (b) and (d) in which h the object is at rest, therefore it means that these quantities are measured always in different frames? Physics 201: Lecture 1, Pg 4
5 Alpha Centauri An astronaut is in a spaceship travelling towards the star Alpha Centauri at a speed of.95 c. Alpha Centauri is 4.3 light years away. t D v 4.3lightyears.95c v =.95 c 4.5years E AC On earth we measure a time of 4.5 years to pass Physics 201: Lecture 1, Pg 5
6 Length Contraction Let s imagine you are in a spaceship heading to Alpha Centauri, moving at a speed of 0.95c. An observer on the earth measures a time of 4.5 years to make the trip. v =.95 c E AC x =.95c(4.5 years) = 4.3 light years Physics 201: Lecture 1, Pg 6
7 Length Contraction Now let s look at the frame of the spaceship. In the spaceship you seem to be at rest and the earth and Alpha Centauri moves relative to you with speed 0.95c. You at rest in the ship measure the time of your trip to be 1.4 years. t v 1- c The ships measures the distance between E and AC to be less than observer at rest!!! V =.95c V =.95c 2 2 E v = 0 AC Physics 201: Lecture 1, Pg 7
8 Length of Position Vector ŷ r xˆ y ˆ x ˆ r Physics 201: Lecture 1, Pg 8
9 The Spacetime Interval Consider two events that are separated in time by an interval t, and are separated in space by an interval x. Let us define the spacetime interval between the two events to be: The spacetime interval has the same value in all inertial reference frames. 9 Physics 201: Lecture 1, Pg 9
10 Momentum Other things will change as well. As you can imagine if length and time change so will other quantities. p m 0 v 1 v c 2 2 p is momentum m 0 is rest mass v is relative velocity of objects c is speed of light 10 Physics 201: Lecture 1, Pg 10
11 Clicker Question 2: A particle is moving at a speed of 0.40 c has a momentum p 0. If the particle s velocity doubles what will happen to it s momentum? (a) It s less than 2 p 0 (b) It s greater than 2 p 0 (c) It s 2 p 0 Physics 201: Lecture 1, Pg 11
12 Cosmic Speed Limit No causal influence, particle or wave, can travel faster than the speed of light Tachyon t t 0 1- p m0v 0 2 v 2 1 v 2 c 2 c 12 Physics 201: Lecture 1, Pg 12
13 Mass is equivalent to energy!!! Energy and mass E E = m 2 0 c Energy when at rest (rest energy) tot m 0 c 1 2 v c 2 2 Student: Is there a practical way to get rid of all our trash to power up the city with E=mc^2 equation? 13 Physics 201: Lecture 1, Pg 13
14 Nuclear Fission Probably the most well-known application of the conservation of total energy is nuclear fission. i A 235 U nucleus absorbs a neutron and then quickly fragments into two smaller nuclei and several extra neutrons. Mass has been lost and converted to an equivalent amount of kinetic energy in the fission products. This generates heat. 14 Physics 201: Lecture 1, Pg 14
15 Pre-Class Quiz: A quarter-pound hamburger with all the fixings has a mass m = kg. The food energy of the hamburger is E = 1.50 MJ. (a) What is the energy equivalent of the mass of the hamburger? (b) By what factor does the energy equivalent exceed the food energy? (a) J (b) Physics 201: Lecture 1, Pg 15
16 Clicker Question 3: You are in a spaceship with no windows, radios, or other means to check outside. How would you determine if the spaceship is at rest or moving at constant velocity? a) By determining the apparent velocity of light in the spaceship. b) By checking your precision watch. If it s running slow, then the ship is moving. c) By measuring the lengths of objects. in the spaceship. If they are shorter, then the ship is moving. d) You should give up because you ve taken on a impossible task. Physics 201: Lecture 1, Pg 16
17 Einstein s theories of relativity Theory of special relativity 1905 Deals with reference frames that are not accelerating (IRF) Predicts that strange things happen when objects move very fast Theory of general relativity 1915 More complete theory Deals with reference frames that are accelerating Explains gravity (Newton gave magnitude of gravity) Predicts that strange things happen when masses get very large One of the first times theory proceeded observations Physics 201: Lecture 1, Pg 17
18 Principle of Equivalence Suppose you are in an elevator with no windows Near surface of earth, not moving a = 9.81 m/s 2 Accelerating upwards a=981m/s
19 Principle of Equivalence You can do no experiment to figure which is happening The two cases are equivalent Starting from here Einstein formulated general relativity
20 Principle of Equivalence Pretend we are in the accelerating elevator and light comes by In the elevator you should see
21 Principle of Equivalence If the two cases are equivalent, gravity should bend light Pretty bold prediction, especially since he just thought it up!
22 Distant Star Apparent position of Star Light is bent more the closer to the sun you get, must be during eclipse Deflection is greatly exaggerated
23 General Relativity Einstein s s theory of gravity Gravity is actually the result of curved spacetime Spacetime: Space and time are no longer separate but can be considered part of the same thing g( (4-dimensional) Time and space are no longer absolute Mass curves spacetime Objects simply move in a straight line, however since spacetime is curved the objects might move in a curve Demo Physics 201: Lecture 1, Pg 23
24 Clicker Question 4: Which of the following statements related to Einstein's general theory of relativity is FALSE? A. It applies to accelerated frames of reference. B. A ray of light can bend in a gravitational field. C. Its predictions agree with Newton's theory of gravity in regions of very strong gravitational fields. Physics 201: Lecture 1, Pg 24
25 The Relativistic Universe It may seem as though relativity has nothing to do with our daily lives. However, medicine makes use of radioactive materials for imaging and treatment; satellites must take relativistic effects into account in order to function properly; and space exploration would be a disaster if relativistic effects were not handled properly. Physics 201: Lecture 1, Pg 25
26 General Relativity If the gravitational field is strong enough, light may be bent so much that it cannot escape. An object that is this dense is called a black hole. Calculations show that the radius of a black hole of a given mass will be: Plugging in the numbers shows us that the Earth would have to have a radius of about 0.9 cm in order to be a black hole. Physics 201: Lecture 1, Pg 26
Lecture Outline Chapter 29. Physics, 4 th Edition James S. Walker. Copyright 2010 Pearson Education, Inc.
Lecture Outline Chapter 29 Physics, 4 th Edition James S. Walker Chapter 29 Relativity Units of Chapter 29 The Postulates of Special Relativity The Relativity of Time and Time Dilation The Relativity of
More informationChapter 26. Relativity
Chapter 26 Relativity Time Dilation The vehicle is moving to the right with speed v A mirror is fixed to the ceiling of the vehicle An observer, O, at rest in this system holds a laser a distance d below
More informationE = mc 2. Inertial Reference Frames. Inertial Reference Frames. The Special Theory of Relativity. Slide 1 / 63. Slide 2 / 63.
Slide 1 / 63 The Special Theory of Relativity E = mc 2 Inertial Reference Frames Slide 2 / 63 Newton's laws are only valid in inertial reference frames: n inertial reference frame is one which is not accelerating
More informationCollege Physics B - PHY2054C. Special & General Relativity 11/12/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.
Special College - PHY2054C Special & 11/12/2014 My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building Outline Special 1 Special 2 3 4 Special Galilean and Light Galilean and electromagnetism do predict
More informationLecture 10: General Relativity I
Lecture 10: General Relativity I Einstein Tower Experiment Gravitational redshifting Strong Equivalence Principal Sidney Harris 10/2/13 1 O: RECAP OF SPECIAL RELATIVITY Einstein s postulates Laws of physics
More informationBlack Holes -Chapter 21
Black Holes -Chapter 21 The most massive stellar cores If the core is massive enough (~3 M ; total initial mass of star > 25 M or so), even neutron degeneracy pressure can be overwhelmed by gravity. A
More informationChapter 37. Relativity. PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow
Chapter 37 Relativity PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow Learning Goals for Chapter 37 Looking forward at why different
More informationClass 6 : General Relativity. ASTR398B Black Holes (Fall 2015) Prof. Chris Reynolds
Class 6 : General Relativity ASTR398B Black Holes (Fall 2015) Prof. Chris Reynolds RECAP! Einstein s postulates " Laws of physics look the same in any inertial frame of reference. " The speed of light
More informationRELATIVITY. The End of Physics? A. Special Relativity. 3. Einstein. 2. Michelson-Morley Experiment 5
1 The End of Physics? RELATIVITY Updated 01Aug30 Dr. Bill Pezzaglia The following statement made by a Nobel prize winning physicist: The most important fundamental laws and facts of physical science have
More informationAnnouncements. Lecture 6. General Relativity. From before. Space/Time - Energy/Momentum
Announcements 2402 Lab will be started next week Lab manual will be posted on the course web today Lab Scheduling is almost done!! HW: Chapter.2 70, 75, 76, 87, 92, 97*, 99, 104, 111 1 st Quiz: 9/18 (Ch.2)
More information(ii) Determine, according to an observer in one of the spaceships, the speed of the other spaceship.
TA [87 marks] This question is about relativistic kinematics. 1a. An observer at rest relative to Earth observes two spaceships. Each spaceship is moving with a speed of 0.85c but[5 marks] in opposite
More informationExperimental Values of Lorentz Transformations of Mass and Time
Experimental Values of Lorentz Transformations of Mass and Time Lorentz Transformation Thought Experiment GPS Clock Calculations Pound-Rebka Experiment Triplet Paradox Experiment The Lorentz transformation
More informationLecture Outlines. Chapter 22. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 22 Astronomy Today 8th Edition Chaisson/McMillan Chapter 22 Neutron Stars and Black Holes Units of Chapter 22 22.1 Neutron Stars 22.2 Pulsars 22.3 Neutron-Star Binaries 22.4 Gamma-Ray
More informationPHYSICS - CLUTCH CH 34: SPECIAL RELATIVITY.
!! www.clutchprep.com CONCEPT: INERTIAL REFERENCE FRAMES A reference frame is a coordinate system that you make measurements in, and there are two types: - Inertial reference frames, which move at velocity
More informationLorentz Transformations and the Twin Paradox By James Carter
Lorentz Transformations and the Twin Paradox By James Carter The Lorentz transformation m = M/ 1-v 2 /c 2 is a principle of measurement that can be classed as one of the laws of physics. (A moving body
More informationPHSC 1053: Astronomy Relativity
PHSC 1053: Astronomy Relativity Postulates of Special Relativity The speed of light is constant in a vacuum and will be the same for ALL observers, independent of their motion relative to the each other
More informationChapter S3 Spacetime and Gravity. Agenda. Distinguishing Crackpots
Chapter S3 Spacetime and Gravity Agenda Announce: Online Quizzes Observations Extra Credit Lecture Distinguishing Crackpot/Genuine Science Review of Special Relativity General Relativity Distinguishing
More informationModern Physics notes Paul Fendley Lecture 34. Born, chapter III (most of which should be review for you), chapter VII
Modern Physics notes Paul Fendley fendley@virginia.edu Lecture 34 General Relativity Born, chapter III (most of which should be review for you), chapter VII Fowler, Remarks on General Relativity Ashby
More informationMr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path.
Mr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path. In an accelerated frame, time runs slow compared to a non-accelerated frame. The Equivalence Principle tells
More informationEPGY Special and General Relativity. Lecture 4B
Lecture 4B In the previous lecture we found that the proper description of the universe is one consisting of a four-dimensional manifold (space) endowed with a Lorentzian metric, (of course we are restricting
More informationClass 16. Prof J. Kenney October 31, Relativity
Class 16 Prof J. Kenney October 31, 2016 Relativity Length contraction (moving sticks are shorter) A measuring stick at rest has a length Lo. When it is propelled at velocity v, it has a shorter length
More informationThe interpretation is that gravity bends spacetime and that light follows the curvature of space.
7/8 General Theory of Relativity GR Two Postulates of the General Theory of Relativity: 1. The laws of physics are the same in all frames of reference. 2. The principle of equivalence. Three statements
More informationFriday, November 29, The challenge of interstellar travel
The challenge of interstellar travel The challenge of interstellar travel Interstellar travel - travel between star systems - presents one overarching challenge: The distances between stars are enormous
More informationGeneral Relativity. on the frame of reference!
General Relativity Problems with special relativity What makes inertial frames special? How do you determine whether a frame is inertial? Inertial to what? Problems with gravity: In equation F = GM 1M
More informationRelativity. Physics April 2002 Lecture 8. Einstein at 112 Mercer St. 11 Apr 02 Physics 102 Lecture 8 1
Relativity Physics 102 11 April 2002 Lecture 8 Einstein at 112 Mercer St. 11 Apr 02 Physics 102 Lecture 8 1 Physics around 1900 Newtonian Mechanics Kinetic theory and thermodynamics Maxwell s equations
More information0 : Einstein s postulates of Special Relativity
Class 2 : The Special Theory of Relativity Recap of Einstein s postulates Time dilation Length contraction Energy and momentum Causality 0 : Einstein s postulates of Special Relativity Consider a group
More informationAstronomy 122 Outline
Astronomy 122 Outline This Class (Lecture 19): Black Holes Next Class: The Milkyway Last Nightlab tonight! HW7 due on Friday. Mar Lecture report due in discussion class on April 5 th th. Nightlab report
More informationReview Special Relativity. February 3, Absolutes of Relativity. Key Ideas of Special Relativity. Path of Ball in a Moving Train
February 3, 2009 Review Special Relativity General Relativity Key Ideas of Special Relativity No material object can travel faster than light If you observe something moving near light speed: Its time
More informationChapter 36 The Special Theory of Relativity. Copyright 2009 Pearson Education, Inc.
Chapter 36 The Special Theory of Relativity Units of Chapter 36 Galilean Newtonian Relativity The Michelson Morley Experiment Postulates of the Special Theory of Relativity Simultaneity Time Dilation and
More informationChapter 37. PowerPoint Lectures for University Physics, Twelfth Edition Hugh D. Young and Roger A. Freedman. Lectures by James Pazun
Chapter 37 Relativity PowerPoint Lectures for University Physics, Twelfth Edition Hugh D. Young and Roger A. Freedman Lectures by James Pazun 37. Relativity 1. Maxwell s equations (and especially the wave
More informationBasic Physics. Remaining Topics. Gravitational Potential Energy. PHYS 1403 Introduction to Astronomy. Can We Create Artificial Gravity?
PHYS 1403 Introduction to Astronomy Basic Physics Chapter 5 Remaining Topics Gravitational Potential Energy Escape Velocity Artificial Gravity Gravity Assist An Alternate Theory of Gravity Gravitational
More informationPhysics. Special Relativity
Physics Special Relativity 1 Albert Einstein, the high school dropout and patent office clerk published his ideas on Special Relativity in 1905. 2 Special vs. General Relativity Special Relativity deals
More informationRelativity. Class 16 Prof J. Kenney June 18, boss
Relativity Class 16 Prof J. Kenney June 18, 2018 boss Length contraction (moving sticks are shorter) A measuring stick at rest has a length Lo. When it is propelled at velocity v, it has a shorter length
More informationToday HW#4 pushed back to 8:00 am Thursday Exam #1 is on Thursday Feb. 11
Today HW#4 pushed back to 8:00 am Thursday Exam #1 is on Thursday Feb. 11 Bring a calculator and a #2 pencil Allowed 1 page notes (front and back) E=mc 2, General Relativity, and exam review ISP209s10
More informationLecture 10: General Relativity I
Lecture 10: General Relativity I! Recap: Special Relativity and the need for a more general theory! The strong equivalence principle! Gravitational time dilation! Curved space-time & Einstein s theory
More informationModern Physics Part 2: Special Relativity
Modern Physics Part 2: Special Relativity Last modified: 23/08/2018 Links Relative Velocity Fluffy and the Tennis Ball Fluffy and the Car Headlights Special Relativity Relative Velocity Example 1 Example
More informationTest 3 results B A. Grades posted in Learn
Test 3 results Grades posted in Learn D C B A End of the Semester approaches - make sure that your test, clicker and homework grades are what you think they should be on Learn F Clicker Question: What
More informationAstronomy 421. Lecture 24: Black Holes
Astronomy 421 Lecture 24: Black Holes 1 Outline General Relativity Equivalence Principle and its Consequences The Schwarzschild Metric The Kerr Metric for rotating black holes Black holes Black hole candidates
More informationCenters of Galaxies. = Black Holes and Quasars
Centers of Galaxies = Black Holes and Quasars Models of Nature: Kepler Newton Einstein (Special Relativity) Einstein (General Relativity) Motions under influence of gravity [23] Kepler The planets move
More informationBasic Physics. What We Covered Last Class. Remaining Topics. Center of Gravity and Mass. Sun Earth System. PHYS 1411 Introduction to Astronomy
PHYS 1411 Introduction to Astronomy Basic Physics Chapter 5 What We Covered Last Class Recap of Newton s Laws Mass and Weight Work, Energy and Conservation of Energy Rotation, Angular velocity and acceleration
More informationToday in Astronomy 102: Einstein studies gravity
Today in Astronomy 102: Einstein studies gravity The principle of equivalence Gravitational time dilation, specialrelativistic time dilation, and the Doppler effect Curved spacetime and the nature of tides
More informationSpecial Relativity 05/09/2008. Lecture 14 1
How Fast Are You Moving Right Now? Special Relativity Einstein messes with space and time 0 m/s relative to your chair 400 m/s relative to earth center (rotation) 30,000 m/s relative to the sun (orbit)
More informationLecture 21: General Relativity Readings: Section 24-2
Lecture 21: General Relativity Readings: Section 24-2 Key Ideas: Postulates: Gravitational mass=inertial mass (aka Galileo was right) Laws of physics are the same for all observers Consequences: Matter
More informationTest #3 Next Tuesday, Nov. 8 Bring your UNM ID! Bring two number 2 pencils. Announcements. Review for test on Monday, Nov 7 at 3:25pm
Test #3 Next Tuesday, Nov. 8 Bring your UNM ID! Bring two number 2 pencils Announcements Review for test on Monday, Nov 7 at 3:25pm Neutron Star - Black Hole merger Review for Test #3 Nov 8 Topics: Stars
More informationAstronomy 1 Fall 2016
Astronomy 1 Fall 2016 Lecture 14; November 10, 2016 Previously on Astro 1 Late evolution and death of intermediate-mass stars (about 0.4 M to about 4 M ): red giant when shell hydrogen fusion begins, a
More informationManifestations of General Relativity. Relativity and Astrophysics Lecture 32 Terry Herter
Manifestations of General elativity elativity and Astrophysics Lecture 32 Terry Herter Outline Consequences of General elativity Tests of G Escape Velocity => Black holes Black holes Size, Event Horizon,
More informationASTR Midterm 2 Phil Armitage, Bruce Ferguson
ASTR 1120-001 Midterm 2 Phil Armitage, Bruce Ferguson SECOND MID-TERM EXAM MARCH 21 st 2006: Closed books and notes, 1 hour. Please PRINT your name and student ID on the places provided on the scan sheet.
More informationGeneral Relativity and Gravity. Exam 2 Results. Equivalence principle. The Equivalence Principle. Experiment: throw a ball. Now throw some light
General Relativity and Gravity Special Relativity deals with inertial reference frames, frames moving with a constant relative velocity. It has some rather unusual predictions Time dilation Length contraction
More informationExperimental Values of Lorentz Transformations of Mass and Time
Experimental Values of Lorentz Transformations of Mass and Time Measuring the Fitzgerald Contraction Lorentz Transformation Thought Experiment GPS Clock Calculations Pound-Rebka Experiment Triplet Paradox
More informationSimultaneity And Time Dilation
OpenStax-CNX module: m42531 1 Simultaneity And Time Dilation OpenStax College This work is produced by OpenStax-CNX and licensed under the Creative Commons Attribution License 3.0 Abstract Describe simultaneity.
More informationSurvey of Astrophysics A110
Black Holes Goals: Understand Special Relativity General Relativity How do we observe black holes. Black Holes A consequence of gravity Massive neutron (>3M ) cannot be supported by degenerate neutron
More informationOutline. General Relativity. Black Holes as a consequence of GR. Gravitational redshift/blueshift and time dilation Curvature Gravitational Lensing
Outline General Relativity Gravitational redshift/blueshift and time dilation Curvature Gravitational Lensing Black Holes as a consequence of GR Waste Disposal It is decided that Earth will get rid of
More informationSpecial Relativity. Principles of Special Relativity: 1. The laws of physics are the same for all inertial observers.
Black Holes Special Relativity Principles of Special Relativity: 1. The laws of physics are the same for all inertial observers. 2. The speed of light is the same for all inertial observers regardless
More informationEinstein s Relativity and Black Holes
Einstein s Relativity and Black Holes Guiding Questions 1. What are the two central ideas behind Einstein s special theory of relativity? 2. How do astronomers search for black holes? 3. In what sense
More informationA100H Exploring the Universe: Black holes. Martin D. Weinberg UMass Astronomy
A100H Exploring the Universe: Black holes Martin D. Weinberg UMass Astronomy astron100h-mdw@courses.umass.edu March 22, 2016 Read: S2, S3, Chap 18 03/22/16 slide 1 Exam #2: March 29 One week from today!
More informationSpace and Time Before Einstein. The Problem with Light. Admin. 11/2/17. Key Concepts: Lecture 28: Relativity
Admin. 11/2/17 1. Class website http://www.astro.ufl.edu/~jt/teaching/ast1002/ 2. Optional Discussion sections: Tue. ~11.30am (period 5), Bryant 3; Thur. ~12.30pm (end of period 5 and period 6), start
More informationGeneral Relativity. PHYS-3301 Lecture 6. Chapter 2. Announcement. Sep. 14, Special Relativity
Announcement Course webpage http://www.phys.ttu.edu/~slee/3301/ Textbook PHYS-3301 Lecture 6 HW2 (due 9/21) Chapter 2 63, 65, 70, 75, 76, 87, 92, 97 Sep. 14, 2017 General Relativity Chapter 2 Special Relativity
More informationGeneral relativity, 3
General relativity, 3 Gravity as geometry: part II Even in a region of space-time that is so small that tidal effects cannot be detected, gravity still seems to produce curvature. he argument for this
More informationChapter 26 Special Theory of Relativity
Chapter 26 Special Theory of Relativity Classical Physics: At the end of the 19 th century, classical physics was well established. It seems that the natural world was very well explained. Newtonian mechanics
More information7/5. Consequences of the principle of equivalence (#3) 1. Gravity is a manifestation of the curvature of space.
7/5 Consequences of the principle of equivalence (#3) 1. Gravity is a manifestation of the curvature of space. Follow the path of a light pulse in an elevator accelerating in gravityfree space. The dashed
More informationTheory of Relativity Final Quiz July 11, VERY short answers. Each worth 1 point.
Theory of Relativity Final Quiz July 11, 2012 Name: Below are short questions and problems. Answer to the best of your ability. All equations and constants you need are on a separate sheet. VERY short
More informationSpecial theory of relativity
Announcements l CAPA #9 due Tuesday April 1 l Mastering Physics Chapter 35 due April 1 l Average on exam #2 is 26/40 l For the sum of the first two exams (80 points); l >=67 4.0 l 61-66 3.5 l 50-60 3.0
More informationTransformation of velocities
Announcements l Help room hours (1248 BPS) Ian La Valley(TA) Mon 4-6 PM Tues 12-3 PM Wed 6-9 PM Fri 10 AM-noon l LON-CAPA #9 due on Thurs Nov 15 l Third hour exam Thursday Dec 6 l Final Exam Tuesday Dec
More informationYour student ID 1 page notes, written double sided Calculator Pencil for marking answer sheet
Hour Exam 2: Wednesday, Oct. 27 In-class (1300 Sterling Hall) Twenty multiple-choice questions Will cover: 8.1-8.6 (Light and E&M) 9.1-9.5 (E&M waves and color) 10, 11 (Relativity) You should bring Your
More informationWallace Hall Academy
Wallace Hall Academy CfE Higher Physics Unit 1 - Universe Notes Name 1 Newton and Gravity Newton s Thought Experiment Satellite s orbit as an Application of Projectiles Isaac Newton, as well as giving
More informationGR and Spacetime 3/20/14. Joys of Black Holes. Compact Companions in Binary Systems. What do we mean by the event horizon of a black hole?
ASTR 1040: Stars & Galaxies Prof. Juri Toomre TA: Ryan Orvedahl Lecture 20 Thur 20 Mar 2014 zeus.colorado.edu/astr1040-toomre Tycho Brahe SNR (1572) Joys of Black Holes Black holes, their general properties,
More informationNeutron Stars. are as small as a city (~10 km) But as massive as the Sun!
Neutron Stars are as small as a city (~10 km) But as massive as the Sun! Extra-Terrestrial Mystery...! In 1967, graduate student Jocelyn Bell helped build a radio telescope in England.! She found a source
More informationRELATIVITY. Special Relativity
RELATIVITY Special Relativity FROM WARMUP How does special relativity differ from general? Special relativity deals with inertial reference frames. General relativity deals with gravity and acceleration
More informationModern Physics notes Spring 2005 Paul Fendley Lecture 35
Modern Physics notes Spring 2005 Paul Fendley fendley@virginia.edu Lecture 35 Gravity and clocks Curved spacetime Born, chapter III (most of which should be review for you), chapter VII Fowler, Remarks
More informationPhysics 107: Ideas of Modern Physics
Physics 107: Ideas of Modern Physics Exam 2 March 14, 2007 Name SOLUTIONS ID # Section # On the Scantron sheet, 1) Fill in your name 2) Fill in your student ID # (not your social security #) 3) Fill in
More informationPhysics 131: Lecture 22. Today s Agenda
Physics 131: Lecture 22 Today s Agenda Rotational dynamics Torque = I Angular Momentum Physics 201: Lecture 10, Pg 1 An Unfair Race A frictionless block and a rolling (without slipping) disk are released
More informationThe result is; distances are contracted in the direction of motion.
The result is; distances are contracted in the direction of motion. t = t/(1 v 2 /c 2 ) 0.5 d = d(1- v 2 /c 2 ) 0.5 These are the Lorentz equations. The Twin-Paradox. A woman astronaut is going to fly
More informationThe Problem of Slowing Clocks in Relativity Theory
The Problem of Slowing Clocks in Relativity Theory The basic premise of Relativity Theory is that the speed of light ( c ) is a universal constant. Einstein evolved the Special Theory on the assumption
More informationName Final Exam December 7, 2015
Name Final Exam December 7, 015 This test consists of five parts. Please note that in parts II through V, you can skip one question of those offered. Part I: Multiple Choice (mixed new and review questions)
More informationAnnouncement. Einstein s Postulates of Relativity: PHYS-3301 Lecture 3. Chapter 2. Sep. 5, Special Relativity
Announcement PHYS-3301 Lecture 3 Sep. 5, 2017 2 Einstein s Postulates of Relativity: Chapter 2 Special Relativity 1. Basic Ideas 6. Velocity Transformation 2. Consequences of Einstein s Postulates 7. Momentum
More informationBlack Holes, or the Monster at the Center of the Galaxy
Black Holes, or the Monster at the Center of the Galaxy Learning Objectives! How do black holes with masses a few times that of our Sun form? How can we observe such black holes?! Where and how might you
More informationCollege Physics B - PHY2054C. Special Relativity 11/10/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.
College - PHY2054C 11/10/2014 My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building Outline 1 2 3 1 The speed of light is the maximum possible speed, and it is always measured to have the same value
More informationElements of Physics II
Physics 132: Lecture 23 Elements of Physics II Agenda for Today Special Theory of relativity Inertial vs. non-inertial reference frames Postulates of SR Consequences of SR Time dilation Length contraction
More informationPage 1. ConcepTest Clicker Questions Chapter 32. Physics, 4 th Edition James S. Walker
ConcepTest Clicker Questions Chapter 32 Physics, 4 th Edition James S. Walker There are 82 protons in a lead nucleus. Why doesn t the lead nucleus burst apart? Question 32.1 The Nucleus a) Coulomb repulsive
More informationA100 Exploring the Universe: Black holes. Martin D. Weinberg UMass Astronomy
A100 Exploring the Universe: Black holes Martin D. Weinberg UMass Astronomy weinberg@astro.umass.edu October 30, 2014 Read: S2, S3, Chap 18 10/30/14 slide 1 Sizes of s The solar neighborhood visualized!
More informationLecture 10: General Relativity I
Lecture 10: General Relativity I! Einstein Tower Experiment! Gravitational redshifting! Strong Equivalence Principal! Read Chapter 8! Due to snow and confusion the mid-term is delayed to Thursday March
More informationToday in Astronomy 102: Einstein studies gravity
Today in Astronomy 102: Einstein studies gravity q The principle of equivalence q Gravitational time dilation, specialrelativistic time dilation, and the Doppler effect q Curved spacetime and the nature
More informationSyllabus and Schedule for ASTRO 210 (Black Holes)
Black Holes Syllabus and Schedule for ASTRO 210 (Black Holes) The syllabus and schedule for this class are located at: http://chartasg.people.cofc.edu/chartas/teaching.html Gravity is Universal Gravity
More informationSpecial Theory of Relativity. The Newtonian Electron. Newton vs. Einstein. So if Newtonian Physics is wrong. It is all Relative.
Special Theory of Relativity Chapter 26 The Newtonian Electron Newtonian Theory (everything we have done so far in class) can be tested at high speeds by accelerating electrons or other charged particles
More informationMichael Fowler, UVa Physics, 12/1/07. Momentum has Direction
Michael Fowler, UVa Physics, //07 Momentum has Direction As we discussed in the last lecture, even before Newton formulated his laws, Descartes, with a little help from Huygens, had discovered a deep dynamical
More informationPostulates of Special Relativity
Relativity Relativity - Seen as an intricate theory that is necessary when dealing with really high speeds - Two charged initially stationary particles: Electrostatic force - In another, moving reference
More informationPhysics 131: Lecture 22. Today s Agenda
Physics 131: Lecture Today s Agenda Rotational dynamics Torque = I Angular Momentum Physics 01: Lecture 10, Pg 1 An Unfair Race A frictionless block and a rolling (without slipping) disk are released at
More informationPhysics 120 Quantum Physics and Beyond Today!
Physics 120 Quantum Physics and Beyond Today! General Relativity Accelerated Frames General Relativity Light in General Relativity Motion and Time in General Relativity Back to Quantum Entanglement? More
More informationLecture 13 Notes: 07 / 20. Invariance of the speed of light
Lecture 13 Notes: 07 / 20 Invariance of the speed of light The Michelson-Morley experiment, among other experiments, showed that the speed of light in vacuum is a universal constant, as predicted by Maxwell's
More informationRelativity. Overview & Postulates Events Relativity of Simultaneity. Relativity of Time. Relativity of Length Relativistic momentum and energy
Relativity Overview & Postulates Events Relativity of Simultaneity Simultaneity is not absolute Relativity of Time Time is not absolute Relativity of Length Relativistic momentum and energy Relativity
More informationExam. Topics covered in Exam 2. Wave properties. Types of wave motion. Waves Questions. Interference of sound waves
Exam Hour Exam 2: Wednesday, October 25th In-class, covering waves, electromagnetism, and relativity Twenty multiple-choice questions Will cover: Chapters 8, 9 10 and 11 Lecture material You should bring
More informationRelativity and Black Holes
Relativity and Black Holes Post-MS Evolution of Very High Mass (>15 M Θ ) Stars similar to high mass except more rapid lives end in Type II supernova explosions main difference: mass of iron core at end
More informationEinstein and his theory of Special Relativity (1905) General relativity came later and deals more with gravity (1915) 07 relativity.
Einstein and his theory of Special Relativity (1905) General relativity came later and deals more with gravity (1915) Groundwork for Einstein's theory was laid out my Michelson and Morley with their interferometer
More informationBell s spaceship paradox
Bell s spaceship paradox If the two ships start accelerating at the same time, I always see them travelling at the same velocity, and keeping a constant distance... But I said the objects get shorter when
More informationPHY152H1S Practical 10: Special Relativity
PHY152H1S Practical 10: Special Relativity Don t forget: List the NAMES of all participants on the first page of each day s write-up. Note if any participants arrived late or left early. Put the DATE (including
More informationIntroduction. Classical vs Modern Physics. Classical Physics: High speeds Small (or very large) distances
Introduction Classical vs Modern Physics High speeds Small (or very large) distances Classical Physics: Conservation laws: energy, momentum (linear & angular), charge Mechanics Newton s laws Electromagnetism
More informationCorrect Resolution of the Twin Paradox
Correct Resolution of the Twin Paradox Michael Huemer In the following, I explain the Twin Paradox, which is supposed to be a paradoxical consequence of the Special Theory of Relativity (STR). I give the
More informationChapter 13 2/19/2014. Lecture Outline Neutron Stars. Neutron Stars and Black Holes Neutron Stars. Units of Chapter
13.1 Neutron Stars Lecture Outline Chapter 13 Neutron Stars and After a Type I supernova, little or nothing remains of the original star. After a Type II supernova, part of the core may survive. It is
More informationGeneral Relativity and Black Holes
General Relativity and Black Holes Lecture 19 1 Lecture Topics General Relativity The Principal of Equivalence Consequences of General Relativity slowing of clocks curvature of space-time Tests of GR Escape
More informationBig Bang, Black Holes, No Math
ASTR/PHYS 109 Dr. David Toback Lectures 8 & 9 1 Prep For Today (is now due) L9 Reading: BBBHNM Unit 2 (already due) Pre-Lecture Reading Questions (PLRQ) Unit 2 Revision (if desired), Stage 2: Was due today
More information