The Relativistic Quantum World
|
|
- Olivia Cunningham
- 5 years ago
- Views:
Transcription
1 The Relativistic Quantum World A lecture series on Relativity Theory and Quantum Mechanics Marcel Merk University of Maastricht, Sept 14 Oct 12, 2017
2 Relativity Quantum Mechanics The Relativistic Quantum World Sept 14: Lecture 1: The Principle of Relativity and the Speed of Light Lecture 2: Time Dilation and Lorentz Contraction Sept 21: Lecture 3: The Lorentz Transformation and Paradoxes Lecture 4: General Relativity and Gravitational Waves Sept 28: Lecture 5: The Early Quantum Theory Lecture 6: Feynman s Double Slit Experiment Oct 5: Lecture 7: The Delayed Choice and Schrodinger s Cat Lecture 8: Quantum Reality and the EPR Paradox Standard Model Oct 12: Lecture 9: The Standard Model and Antimatter Lecture 10: The Large Hadron Collider Lecture notes, written for this course, are available: Prerequisite for the course: High school level mathematics.
3 Lecture 4 General Relativity and Gravitational Waves Do not worry about your difficulties in mathematics. I can assure you mine are still greater. -Albert Einstein
4 Ehrenfest Paradox Rotating disk with ruler on the edge: Circumference: C = 2 p r 2p r Paul Ehrenfest
5 Ehrenfest Paradox Rotating disk with ruler on the edge: Circumference: C = 2 p r 2p r Alice stands next to the disk and sees rulers on disk Lorentz contracted: C = 2 p r / g è Circumference is smaller! Bob moves on the disk and sees rulers next to disk contracted: C = 2 p r g è Circumference is larger! A rotating object is not an inertial frame: Postulate of relativity only worked for inertial frames Need to adapt the postulates: special relativity à general relativity
6 The Equivalence Principle (Inertial Frame) Einstein happiest thought : There is no way to determine whether you are standing on the earth or accelerating upwards in a rocket in space.
7 The Equivalence Principle (Inertial Frame) There is no difference between acceleration force and gravitation. Gravitational mass = inertial mass
8 The Eötvös Experiment Direction of gravity and Centrifugal force on earth Small (m 1 ) and big (m 2 ) mass on a rod suspended by a thin fiber Loránd Eötvös Gravity force G depends on Newton s law of gravity: gravitational mass Centrifugal force F depends on Newton s law of motion inertial mass: inertial mass The system did not rotate. è F 1 /F 2 = G 1 /G 2 èexperimental proof that indeed gravitational mass is equivalent to inertial mass.
9 Bending of light Consequence if acceleration and gravity are identical: A B Outside view Inside view Gravity view A: Lightbeam in accelerating rocket B: Lightbeam in gravitational field Prediction of Einstein: light beam bends under gravity!
10 Bending of light in gravitation field of the Sun Light wants to go straight but space is curved! Confirmed during solar eclipse on November !
11
12 Einstein s thought experiment Particle with mass m falling from tower: m E = mc 2 ) E = hf From quantum mechanics we know: Energy of light is related to frequency (and wavelength): E = hf = hc/ h hf 0 >hf?? èno! Photon loses energy as it travels up the gravitational field! E 0 = mc mv2 = mc 2 + mgh = mc 2 1+gh/c 2 ) E 0 = hf 0
13 The Harvard Tower Experiment Harvard Tower Experiment (Pound-Rebka) at Jefferson lab in Harvard: Measure red-shift of photons in earth gravitational field. h = 22.5 m Df/f = DE/E = gh/c 2 = 2.5 x as expected!
14 Gravitational Time Dilation The photon loses energy as it climbs the gravitational field. ètime ticks faster at higher altitude.
15 Accelerating Rocket From special relativity we know that space contracts at high velocity velocity : 0 < v 1 < v 2 < v 3 s s s l 1 v 2 1 c 2 l 1 v 2 2 c 2 l 1 v 2 3 c 2 l Space is seen to shrink further and further with increasing velocity! 1/ = s 1 v 2 c 2
16 Falling apple: E pot = G mm R Free falling object Newton s Constant G Compare an to accelerating rocket: 1 E kin = E pot 2 mv2 = G mm R l v 2 =2 GM R s 1 v 2 c 2 = Lorentz factor r 1 2 GM Rc 2 l 0 Space shrinkage ( curvature ): l 0 = r 1 2 GM Rc 2 l
17 Space-Time curvature A falling apple accelerates and units of space get more and more contracted: An apple falls into the gravitational field and time runs slower and slower: l t Space Time l 0 t 0 l 0 =1/ l = r 1 2 GM Rc 2 l t 0 = t = 1 t q1 2 GMRc2 Space contracts near mass and dilates away from it. Time slows near mass and Speeds up away from it. Space-time is curved in the presence of mass
18 Mass causes curvature in space-time
19 Relativity and GPS Two effects: Time speeds up at the satellite in comparison to earth surface due to gravity Time slows down at the satellite due to high velocity compared to person on earth è Clocks in satellite and on earth de-synchronize with ~ 40 msec per day!
20 Black Hole Gravitational time slowdown near a star with mass M: r t 0 2GM = t 1 Rc 2 Schwarzschild radius: R s = 2GM c 2 r t 0 = t 1 R s R R
21 Black Hole Gravitational time slowdown near a star with mass M: r t 0 2GM = t 1 Rc 2 Schwarzschild radius: R s = 2GM c 2 r t 0 = t 1 R s R R s Time stand-still: if R = R s then t 0 =0 (Time stands still at the horizon of a black-hole) Example our Sun: G = 6.67 x m 3 /kg s 2 (Newton s gravitation constant) M sun = 2 x kg è R s = 3 km for a black hole.
22 Black hole requires ~ 3 x Msun
23 What is a black hole? Purely curved space-time!
24 What is a black hole? What happens when black holes meet?
25 Electric vs Gravitational Fields Electric field of positive and negative charged particle: Gravitational field of the earth: F e = qe = 1 qq 4 " 0 r 2 F g = mg = G mm R 2 Einstein spent most of his life looking for a unified theory of electromagnetism and general relativity.
26 Waves and Radiation Electromagnetic waves: Caused by accelerating electric particles electrons, eg.: radio-emission Maxwell µ F µ = 4 c J E and B fields Electric charge and currents Gravitational Waves: Caused by moving masses. Requires very heavy masses àblack holes. (Einstein thought these couldn t be observed) Einstein equations: G µ + g µ = 8 G c 4 T µ Space-time fields Mass and mass-flow
27 Electromagnetic and Gravitational Waves Electromagnetic wave Electromagnetic wave: Changing electric and magnetic field propagating through space. Caused by moving (accelerating!) electric charges. Gravitational wave Gravitational wave: Changing space-time field. Caused by moving (accelerating!) masses. y x
28 Remember the interferometer!
29 Detection of Gravitational Waves
30 Which precision is needed? Seismic proton Laser noise (f,p) atom Laser Beamsplitter Mirror hair Radiation Pressure noise Photodetector Interference
31 Current Facilities
32 Two merging black holes Two massive colliding/merging black holes: B.H.1 = 36 x mass of the sun B.H.2 = 29 x mass of the sun New BH: 62 solar masses Distance: 1.3 billion lightyears Relative change of space (strain) % Rotation speed increasing to half the light speed! More energy emitted in grav waves than the visible light of all stars in the universe!
33 Ligo Hanford and Livingston Consistent signals seen in the Washington and Louisiana detectors! (GW150914) observation observation Expectation GR Expectation GR
34 Numerical relativity simulation for GW Parameters measured by matching millions of trial waveforms in 15-dimensional parameter space
35 The Virgo Experiment in Pisa
36 Ultrahigh Vacuüm Largest vacuüm vessel in Europe Pressure ~ mbar
37 Seismic dampingsystem
38 Seismic Damping Table
39 Input mode cleaner end mirror
40 Beam splitter Example #1: advanced optical systems
41 Example #2: Cavity control
42 Einstein Telescope Possible future facility Een observatorium voor zwaartekrachtsgolven van 2 Hz tot 10 khz
43 Possible future facility Einstein Telescope The next gravitational wave observatory
44 Possible future facility Einstein Telescope The next gravitational wave observatory
45 Fundamental Black hole physics Wat happens at the edge of a black hole (quantum effects)? Is Einstein s theory still valid under these extreme conditions?
46 Looking into the Big Bang What happened the first moments of the Big Bang? Search for gravitational waves originating from the very first moment! Inflatie (Big Bang plus seconden) Neutrino s 1 seconde Big Bang plus jaar zwaartekrachtsgolven Licht Nu Big Bang plus 14 miljard jaar
47 Next Lecture Quantum mechanics developed by Bohr and Heisenberg leads to absurd thought experiments of Feynman and Wheeler. Einstein and Schrödinger did not like it. Even today people are debating its interpretation. Richard Feynman
48 Some extra slides
49 Einstein Quotes Imagination is more important than knowledge Education is what remains after one has forgotten what one has learned at school. I fear the day that technology will surpass our human interaction. The world will have a generation of idiots. A person who never made a mistake never tried anything new.
50 Gravitatie golven Detectie methode (dutch)
51 The Gravitational Wave Spectrum
Lecture 18 Vacuum, General Relativity
The Nature of the Physical World Lecture 18 Vacuum, General Relativity Arán García-Bellido 1 Standard Model recap Fundamental particles Fundamental Forces Quarks (u, d, c, s, t, b) fractional electric
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 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 informationGravitational Waves: From Einstein to a New Science
Gravitational Waves: From Einstein to a New Science LIGO-G1602199 Barry C Barish Caltech - LIGO 1.3 Billion Years Ago 2 Black Holes Regions of space created by super dense matter from where nothing can
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 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 informationLecture 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 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 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 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 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 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 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 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 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 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 informationPostulate 2: Light propagates through empty space with a definite speed (c) independent of the speed of the source or of the observer.
Einstein s Special Theory of Relativity 1 m E = mv E =m*c m* = KE =m*c - m c 1- v p=mv p=m*v c 9-1 Postulate 1: The laws of physics have the same form in all inertial reference frames. Postulate : Light
More informationCracking the Mysteries of the Universe. Dr Janie K. Hoormann University of Queensland
Cracking the Mysteries of the Universe Dr Janie K. Hoormann University of Queensland Timeline of Cosmological Discoveries 16c BCE: flat earth 5-11c CE: Sun at the centre 1837: Bessel et al. measure distance
More informationSPECIAL RELATIVITY! (Einstein 1905)!
SPECIAL RELATIVITY! (Einstein 1905)! Motivations:! Explaining the results of the Michelson-Morley! experiment without invoking a force exerted! on bodies moving through the aether.! Make the equations
More informationGravity Waves and Black Holes
Gravity Waves and Black Holes Mike Whybray Orwell Astronomical Society (Ipswich) 14 th March 2016 Overview Introduction to Special and General Relativity The nature of Black Holes What to expect when Black
More informationUnderstanding and Testing Relativity
Understanding and Testing Relativity From Einstein s formulations to the tests of today www. library.thinkquest.org www.csep10.phys.utk.edu www.arcive.ncsa.uiuc.edu Boston University - April 25, 2006 1
More informationLimitations of Newtonian Physics
Limitations of Newtonian Physics 18 th and 19 th Centuries Newtonian Physics was accepted as an ultimate truth Science is never absolute Hundreds of experiments can t prove my theory right but only one
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 informationBlack Holes. Introduction: Stable stars which balance pressure due to gravity by quantum pressure(qp) are:
Black Holes Introduction: Stable stars which balance pressure due to gravity by quantum pressure(qp) are: 1. White Dwarfs (WD) : QP = electron degeneracy pressure. Mass < 1.4 M_sun This upper limit is
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 informationLIGO s Detection of Gravitational Waves from Two Black Holes
LIGO s Detection of Gravitational Waves from Two Black Holes Gregory Harry Department of Physics, American University February 17,2016 LIGO-G1600274 GW150914 Early History of Gravity Aristotle Kepler Laplace
More information6 General Relativity. Today, we are going to talk about gravity as described by Einstein s general theory of relativity.
6 General Relativity Today, we are going to talk about gravity as described by Einstein s general theory of relativity. We start with a simple question: Why do objects with di erent masses fall at the
More informationSpecial Relativity: The laws of physics must be the same in all inertial reference frames.
Special Relativity: The laws of physics must be the same in all inertial reference frames. Inertial Reference Frame: One in which an object is observed to have zero acceleration when no forces act on it
More informationClass 5: Equivalence Principle
Class 5: Equivalence Principle In this class we will discuss the conceptual foundations of General Relativity, in which gravity may be associated with the reference frames in which perceive events Class
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 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 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 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 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 informationGravitational Wave. Kehan Chen Math 190S. Duke Summer College
Gravitational Wave Kehan Chen 2017.7.29 Math 190S Duke Summer College 1.Introduction Since Albert Einstein released his masterpiece theory of general relativity, there has been prediction of the existence
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 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 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 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 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 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 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 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 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 informationModern Physics notes Paul Fendley Lecture 35. Born, chapter III (most of which should be review for you), chapter VII
Modern Physics notes Paul Fendley fendley@virginia.edu Lecture 35 Curved spacetime black holes Born, chapter III (most of which should be review for you), chapter VII Fowler, Remarks on General Relativity
More informationAstronomy 182: Origin and Evolution of the Universe
Astronomy 182: Origin and Evolution of the Universe Prof. Josh Frieman Lecture 6 Oct. 28, 2015 Today Wrap up of Einstein s General Relativity Curved Spacetime Gravitational Waves Black Holes Relativistic
More informationDynamics of star clusters containing stellar mass black holes: 1. Introduction to Gravitational Waves
Dynamics of star clusters containing stellar mass black holes: 1. Introduction to Gravitational Waves July 25, 2017 Bonn Seoul National University Outline What are the gravitational waves? Generation of
More informationEinstein s Gravity. Understanding space-time and the gravitational effects of mass
Einstein s Gravity Understanding space-time and the gravitational effects of mass Albert Einstein (1879-1955) One of the iconic figures of the 20 th century, Einstein revolutionized our understanding of
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 informationDiscovery of Gravita/onal Waves
Discovery of Gravita/onal Waves Avto Kharchilava QuarkNet Workshop, August 2016 https://www.ligo.caltech.edu/news/ligo20160211 Gravity Einstein s General theory of relativity: Gravity is a manifestation
More informationLecture: Principle of Equivalence
Chapter 6 Lecture: Principle of Equivalence The general theory of relativity rests upon two principles that are in fact related: The principle of equivalence The principle of general covariance 6.1 Inertial
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 informationASTR 200 : Lecture 30. More Gravity: Tides, GR, and Gravitational Waves
ASTR 200 : Lecture 30 More Gravity: Tides, GR, and Gravitational Waves 1 Topic One : Tides Differential tidal forces on the Earth. 2 How do tides work???? Think about 3 billiard balls sitting in space
More informationGravitational Waves and LIGO
Gravitational Waves and LIGO Ray Frey, University of Oregon 1. GW Physics and Astrophysics 2. How to detect GWs The experimental challenge 3. Prospects June 16, 2004 R. Frey QNet 1 General Relativity Some
More informationAPPENDIX C APPENDIX C. The Problem with E = mc
APPENDIX C APPENDIX C The Problem with E = mc 154 THE DEADBEAT UNIVERSE APPENDIX C 155 APPENDIX C THE PROBLEM WITH E = mc In 1905 Einstein envisaged energy of mass m as being equivalent to mass velocity
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 information11/1/17. Important Stuff (Section 001: 9:45 am) Important Stuff (Section 002, 1:00 pm) 14.1 White Dwarfs. Chapter 14: The Bizarre Stellar Graveyard
11/1/17 Important Stuff (Section 001: 9:45 am) The Second Midterm is Thursday, November 9 The Second Midterm will be given in a different room: Willey 175 Bring 2 pencils and a photo-id. In accordance
More information5/7/2018. Black Holes. Type II.
Black Holes Type II https://www.youtube.com/watch?v=ctnkk7tnkq8 1 Scientific American 22, 82 (2013) Scientific American 22, 82 (2013) 2 First detection of gravitational waves Recommended reading Physics
More informationThe Relativistic Quantum World
The Relativistic Quantum World A lecture series on Relativity Theory and Quantum Mechanics Marcel Merk University of Maastricht, Sept 24 Oct 15, 2014 Relativity Quantum Mechanics The Relativistic Quantum
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 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 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 informationStellar remnants II. Neutron Stars 10/18/2010. (progenitor star 1.4 < M< 3 Msun) Stars, Galaxies & the Universe Announcements
Stars, Galaxies & the Universe Announcements Exam #2 on Wednesday Review sheet and study guide posted by Thursday Use office hours and Astronomy Tutorial hours Covers material since Exam #1 (plus background
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 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 informationASTR 200 : Lecture 31. More Gravity: Tides, GR, and Gravitational Waves
ASTR 200 : Lecture 31 More Gravity: Tides, GR, and Gravitational Waves 1 Topic One : Tides Differential tidal forces on the Earth. 2 How do tides work???? Think about 3 billiard balls sitting in space
More informationBlack Holes. Over the top? Black Holes. Gravity s Final Victory. Einstein s Gravity. Near Black holes escape speed is greater than the speed of light
Black Holes Over the top? What if the remnant core is very massive? M core > 2-3 M sun (original star had M > 18 M sun ) Neutron degeneracy pressure fails. Nothing can stop gravitational collapse. Collapses
More informationGravitation. Adrian Ferent. This is a new quantum gravity theory which breaks the wall of Planck scale. Abstract
Gravitation Adrian Ferent This is a new quantum gravity theory which breaks the wall of Planck scale. My Nobel Prize Idea Abstract The Photon Graviton pair (coupled) has the same speed and frequency, and
More informationLight and Relativity
PHY1033C Fall 2017 Lecture W11 Light and Relativity 1. Light, a Special Wave For more than 200 years, Newton s theory of mechanics, condensed into the three laws of motion, have been accepted as the correct
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 informationRelativity. Astronomy 101
Lecture 29: Special & General Relativity Astronomy 101 Common Sense & Relativity Common Sense is the collection of prejudices acquired by the age of 18. Albert Einstein It will seem difficult at first,
More informationLIGO Status and Advanced LIGO Plans. Barry C Barish OSTP 1-Dec-04
LIGO Status and Advanced LIGO Plans Barry C Barish OSTP 1-Dec-04 Science Goals Physics» Direct verification of the most relativistic prediction of general relativity» Detailed tests of properties of gravitational
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 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 informationGravitational Waves Theory - Sources - Detection
Gravitational Waves Theory - Sources - Detection Kostas Glampedakis Contents Part I: Theory of gravitational waves. Properties. Wave generation/the quadrupole formula. Basic estimates. Part II: Gravitational
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 informationENTER RELATIVITY THE HELIOCENTRISM VS GEOCENTRISM DEBATE ARISES FROM MATTER OF CHOOSING THE BEST REFERENCE POINT. GALILEAN TRANSFORMATION 8/19/2016
ENTER RELATIVITY RVBAUTISTA THE HELIOCENTRISM VS GEOCENTRISM DEBATE ARISES FROM MATTER OF CHOOSING THE BEST REFERENCE POINT. GALILEAN TRANSFORMATION The laws of mechanics must be the same in all inertial
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 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 informationTalking about general relativity Important concepts of Einstein s general theory of relativity. Øyvind Grøn Berlin July 21, 2016
Talking about general relativity Important concepts of Einstein s general theory of relativity Øyvind Grøn Berlin July 21, 2016 A consequence of the special theory of relativity is that the rate of a clock
More informationUnit- 1 Theory of Relativity
Unit- 1 Theory of Relativity Frame of Reference The Michelson-Morley Experiment Einstein s Postulates The Lorentz Transformation Time Dilation and Length Contraction Addition of Velocities Experimental
More informationMotivation. The Speed of Light. The Speed of Light. In Water Things Look Like This. Introduction to Special and General Relativity
Introduction to Special and General Relativity Motivation: Michelson-Morley Experiment Induction versus Force Law The Basics Events Principles of Relativity Giving up on absolute space and time What Follows
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 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 informationMidterm Solutions. 1 1 = 0.999c (0.2)
Midterm Solutions 1. (0) The detected muon is seen km away from the beam dump. It carries a kinetic energy of 4 GeV. Here we neglect the energy loss and angular scattering of the muon for simplicity. a.
More informationEinstein s Special Theory of Relativity. Dr. Zdzislaw Musielak UTA Department of Physics
Einstein s Special Theory of Relativity Dr. Zdzislaw Musielak UTA Department of Physics OUTLINE Einstein s Miraculous Year 1905 Time and Space before 1905 Einstein s Paper # 3 Time and Space after 1905
More informationSqueezed Light for Gravitational Wave Interferometers
Squeezed Light for Gravitational Wave Interferometers R. Schnabel, S. Chelkowski, H. Vahlbruch, B. Hage, A. Franzen, and K. Danzmann. Institut für Atom- und Molekülphysik, Universität Hannover Max-Planck-Institut
More informationEinstein in a Nutshell
Einstein in a Nutshell Richard Wolfson Benjamin F. Wissler Professor of Physics Middlebury College Insight Cruises/Scientific American January 15, 2011 Relativity in Recent News http://newscenter.berkeley.edu/2011/12/05/record-black-holes-bigger-than-our-solar-system/,
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 informationIntroduction: Special Relativity
Introduction: Special Relativity Observation: The speed c e.g., the speed of light is the same in all coordinate systems i.e. an object moving with c in S will be moving with c in S Therefore: If " r!
More informationAstronomy 120 Overview
Prof. Jeff Kenney Class 15 June 15, 2018 Astronomy 120 Overview Lec 1-5: intro, physics review (FAST) Lec 6-8: stars (FAST) Lec 9-14: galaxies, clusters & dark matter (SLOW) Lec 15-18: black holes & active
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 informationAstronomy 1143 Quiz 2 Review
Astronomy 1143 Quiz 2 Review Prof. Pradhan October 1, 2018 Light 1. What is light? Light is electromagnetic energy It is both a particle (photon) and a wave 2. How is light created and what can light interact
More informationEinstein did not explain the photoelectric effect. There are not Black Holes at Planck wall
Einstein did not explain the photoelectric effect. There are not Black Holes at Planck wall I discovered a new Gravitation theory which breaks the wall of Planck scale! Abstract My Nobel Prize - Discoveries
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 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 information11/1/16. Important Stuff (Section 001: 9:45 am) Important Stuff (Section 002, 1:00 pm) 14.1 White Dwarfs. Chapter 14: The Bizarre Stellar Graveyard
Important Stuff (Section 001: 9:45 am) The Second Midterm is Thursday, November 10 The Second Midterm will be given in a different room: Willey 175 Bring 2 pencils and a photo-id. In accordance with the
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 informationGeneral Relativity: Einstein s Theory of Gravitation. Arien Crellin-Quick and Tony Miller SPRING 2009 PHYS43, SRJC
General Relativity: Einstein s Theory of Gravitation Presented By Arien Crellin-Quick and Tony Miller SPRING 2009 PHYS43, SRJC The Motivations of General Relativity General Relativity, or GR, was created
More informationThe Quest to Detect Gravitational Waves
The Quest to Detect Gravitational Waves Peter Shawhan California Institute of Technology / LIGO Laboratory What Physicists Do lecture Sonoma State University March 8, 2004 LIGO-G040055-00-E Outline Different
More information