Lecture 2: Relativistic Space-Time Invariant Intervals & Proper Time Lorentz Transformations Electromagnetic Unification Equivalence of Mass and Energy.

Slides:



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

Classical Relativity Galilean Transformations
Physics Lecture Resources
BH Astrophys Ch6.4~6.5. The need to rethink space and time Any such beam of any kind of particles generated at the speed of light by a moving observer.
Lecture 13 Space Time Diagrams ASTR 340 Fall 2006 Dennis Papadopoulos.
Theory of Special Relativity
P1X*Dynamics & Relativity : Newton & Einstein Chris Parkes October 2005 Special Relativity Postulates Time Dilation Length Contraction Lorentz Transformation.
Extragalactic Astronomy & Cosmology First-Half Review [4246] Physics 316.
Phy107 Fall 2006 From last time… Einstein’s Relativity ◦ All laws of physics identical in inertial ref. frames ◦ Speed of light=c in all inertial ref.
Relativistic Momentum Classical physics: Definition of momentum: p = mv Conservation of momentum:p 1 + p 2 = p 3 + p 4 Coordinate transformation (Galilei;
Physics 3 for Electrical Engineering Ben Gurion University of the Negev
Derivation of Lorentz Transformations
Special Relativity Lecture 24 F2013 The Postulates Phenomenology The proper frame Time Length Mass energy Measuring events Lorentz transformations 1.
Relativity Pierre-Hugues Beauchemin PHY 006 –Talloire, May 2013.
Static equilibrium : the two conditions for a body in static equilibrium are: (1)The vector sum of all the external forces acting on the body is zero.
The Lorentz transformation equations Once again Ś is our frame moving at a speed v relative to S.
Inflation, vacua and the end of the Universe.
Life in the fast lane: the kinematics of Star Trek.
Chapter 37 Special Relativity. 37.2: The postulates: The Michelson-Morley experiment Validity of Maxwell’s equations.
NJIT Physics 320: Astronomy and Astrophysics – Lecture IV Carsten Denker Physics Department Center for Solar–Terrestrial Research.
Life in the fast lane: the kinematics of Star Trek.
Lecture 14 Space-time diagrams (cont) ASTR 340 Fall 2006 Dennis Papadopoulos.
The Lorentz transformations Covariant representation of electromagnetism.
PH300 Modern Physics SP11 “The only reason for time is so that everything doesn’t happen at once.” - Albert Einstein 2/1 Day 6: Questions? Spacetime Addition.
1 PH300 Modern Physics SP11 1/27 Day 5: Questions? Time Dilation Length Contraction Next Week: Spacetime Relativistic Momentum & Energy “I sometimes ask.
Further Logistical Consequences of Einstein’s Postulates
Special Relativity.
M H Maps of space Space: N & E or M & H Electromagnetism: E & B or E & B.
2.1The Apparent Need for Ether 2.2The Michelson-Morley Experiment 2.3Einstein’s Postulates 2.4The Lorentz Transformation 2.5Time Dilation and Length Contraction.
Introduction to special relativity
Special Theory of Relativity
Page 1 Phys Baski Relativity I Topic #9: Special Relativity I Transformation of Variables between Reference Frames –Non-relativistic Galilean Transformation.
Modern Physics (PC300) Class #2 Review Einstein and Newton The Ether question How to draw Events on a Spacetime diagram.
1 1.Einstein’s special relativity 2.Events and space-time in Relativity 3. Proper time and the invariant interval 4. Lorentz transformation 5. Consequences.
1 PH604 Special Relativity (8 lectures) Books: “Special Relativity, a first encounter”, Domenico Giulini, Oxford “Introduction to the Relativity Principle”,
Announcements Exam 3 is Monday April 13. Will cover the rest of Chapter 4, all of Chapters 5, 6, 7 & 8. New Sample Questions that include Chapter 8 are.
Little drops of water, little grains of sand, make the mighty ocean and the pleasant land. Little minutes, small though they may be, make the mighty ages.
25 September 2001Astronomy 102, Fall The world’s most famous patent clerk, c Today in Astronomy 102: relativity, continued  Einstein’s procedures.
Special Relativity The Failure of Galilean Transformations
1 1.Einstein’s special relativity 2.Events and space-time in Relativity 3. Proper time and the invariant interval 4.Lorentz transformation Einstein’s special.
Special Relativity & Radiative Processes. Special Relativity Special Relativity is a theory describing the motion of particles and fields at any speed.
Physics 3 for Electrical Engineering Ben Gurion University of the Negev
Introduction to special relativity
The Theory of Special Relativity. Learning Objectives  Einstein’s two postulates in his theory of special relativity: The principle of relativity. (Same.
Physics 12 MODERN PHYSICS: AN INTRODUCTION.  QUOTE AND CLIP OF.
Introduction Classical Physics Laws: Mechanics (Newton), Electromagnetism (Maxwell), Optics, Fluids,.. Etc. Modern Physics: What do we mean? Are the laws.
Special Relativity 1. Quiz 1.22 (10 minutes) and a few comments on quiz So far we know that Special Relativity is valid for all speeds. But it is.
PART TWO: RELATIVISTIC MECHANICS PHYS 141: Principles of Mechanics.
Consequences of Special Relativity Simultaneity: Newton’s mechanics ”a universal time scale exists that is the same for all observers” Einstein: “No universal.
1 PH604 Special Relativity (8 lectures) Books: “Special Relativity, a first encounter”, Domenico Giulini, Oxford “Introduction to the Relativity Principle”,
Wed., Sept. 5, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #3 Wednesday, Sept. 5, 2012 Dr. Jaehoon Yu Galilean Transformation.
Chapter 1 Relativity 1.
SPECIAL THEORY OF RELATIVITY. Inertial frame Fig1. Frame S’ moves in the +x direction with the speed v relative to frame S.
Galileo’s Relativity: Text: The laws of mechanics are the same in all inertial reference frames. More general: The laws of mechanics are the same in all.
1 Review: Special Relativity – Chapter 1 Postulates of relativity: 1. All physical laws are the same in all inertial reference frames 2. The speed of light.
Physics 141Mechanics Lecture 5 Reference Frames With or without conscience, we always choose a reference frame, and describe motion with respect to the.
Course Business: PHYS344 Lecture 7 3 rd problem set due next Wednesday, Sept. 17 th in class From Krane Chapter 2: 39, 40, 41, 42, 47, 48, 49, 50, 53,
PHYS 342: More info The TA is Meng-Lin Wu: His is His office hour is 10:30am to 12pm on Mondays His office is Physics.
Administrative Details: PHYS 344
UNIT-III RIGID BODY DYNAMICS
PHYS 3313 – Section 001 Lecture #5
Lecture 4: PHYS 344 Homework #1 Due in class Wednesday, Sept 9th Read Chapters 1 and 2 of Krane, Modern Physics Problems: Chapter 2: 3, 5, 7, 8, 10, 14,
Units The work done in accelerating an electron across a potential difference of 1V is W = charge x potential W = (1.602x10-19C)(1V) = 1.602x10-19 J W.
An Introduction To ‘High Speed’ Physics
Special relativity Physics 123 1/16/2019 Lecture VIII.
RELATIVITY III SPECIAL THEORY OF RELATIVITY
The Galilean Transformation
Spacetime Structure.
PHYS 3313 – Section 001 Lecture #5
Chapter 37 Special Relativity
Presentation transcript:

Lecture 2: Relativistic Space-Time Invariant Intervals & Proper Time Lorentz Transformations Electromagnetic Unification Equivalence of Mass and Energy Space-Time Diagrams Relativistic Optics Section 6-7, 19-21, Useful Sections in Rindler:

Einstein’s Two Postulates of Special Relativity: I. The laws of physics are identical in all inertial frames II. Light propagates in vacuum rectilinearly, with the same speed at all times, in all directions and in all inertial frames Einstein’s postulates

vv vv v d d tt c = d tt -v tt  c /  t ) 2 + v 2 tt tt tt  1 - (v/c) 2 =  d/  t ) 2 +v 2  x = v  t c =  d 2 +v 2  t 2 tt Time Dilation: Time dilation

c =  d 2 +(  x ) 2 tt Recall: Thus, (c  t ) 2 = d 2 + (  x ) 2 d 2 = (c  t ) 2 - (  x ) 2 invariant or, more generally, S 2 = (c  t ) 2 - [(  x ) 2 + (  y ) 2 + (  z ) 2 ] ''Invariant Interval” choose frame ''at rest” = (c   “Proper Time” Invariant interval & proper time

Consider light beam moving along positive x-axis: x = ct or x - ct = 0 Similarly, in the moving frame, we want to have x = ct or x - ct = 0 We can insure this is the case if: x - ct = a(x - ct ) Generally, the factor could be different for motion in the opposite direction: x + ct = b(x + ct ) Subtracting t = t  x/c (a+ b) 2 (a-b) 2 = t  x/c (a+ b) 2 (a-b) (a+b) [ ] = A t  x/c [ ] Lorentz Transformations: Lorentz transformations

= A t  x/c [ ] t So, we know that A =   t = A  t (at fixed x) Similarly, x =  [ x - Bct ] x =  [ x - vt ] t =  [ t - (v/c 2 )x ] In non-relativistic limit (   1) : x  [ x - Bct ] Must correspond to Galilean transformation, so Bc = v B = v/c Lorentz transformations (2)

Maxwell’s Equations ''Lorentz-Fitzgerald Contraction” ''Aether Drag” George Francis Fitzgerald Hendrik Antoon Lorentz Lorentz & Fitzgerald

+q +  +  +  +  v I B Lab Frame F (pure magnetic) +    q In Frame of Test Charge Lorentz expanded Lorentz contracted F (pure electrostatic)  Electricity & Magnetism are identically the same force, just viewed from different reference frames UNIFICATION !! (thanks to Lorentz invariance)  Relativity & Electromagnetism Symmetry: The effect of a force looks the same when viewed from reference frames boosted in the perpendicular direction

+q +  +  +  +  v I B Lab Frame +    q In Frame of Test Charge Lorentz expanded Lorentz contracted F (pure magnetic) F (pure electrostatic) Equivalence of EM forces F = qv  B | F | = qv I  o / (2  r) lab + = lab  = q  =  q  =  ´ = q +    E =  / 2  r  o =  v   / (2  r  o c 2 ) =  v    / (2  r) | F ´| = Eq =  v    q / (2  r) v = I | F | = | F ´| /  = qv   / (2  r)   =  | F ´| =  v   q / (2  r)

Einstein’s The 2 Postulates of Special Relativity: I. The laws of physics are identical in all inertial frames II. Light propagates in vacuum rectilinearly, with the same speed at all times, in all directions and in all inertial frames Einstein’s postulates, again

Planck’s recommendation for Einstein’s nomination to the Prussian Academy in 1913: “In summary, one can say that there is hardly one among the great problems in which modern physics is so rich to which Einstein has not made a remarkable contribution. That he may sometimes have missed the target in his speculations, as, for example, in his hypothesis of light quanta, cannot really be held against him, for it is not possible to introduce really new ideas even in the most exact sciences without sometimes taking a risk.”

1905

E = h (Planck) p = h/ (De Broglie) = hc/ E = pc absorber emitter p=E/c recoil p=Mv E/c = Mv motion stops distance travelled d = vt = v (L/c) = EL/(Mc 2 ) But no external forces, so CM cannot change! Must have done the equivalent of shifting some mass m to other side, such that M {EL/(Mc 2 )} = m L Md = mL “Einstein’s Box”: Einstein’s box

+ x- x ct -y + y Space-Time: Space-time diagram

+ x- x ct = c  t/  x = c/v = 1/  object stationary until time t 1 x1x1 ct 1 moves with constant velocity (  ) until t 2 ct 2 x2x2 returns to point of origin slope = (ct 2 - ct 1 )/(x 2 -x 1 ) Space-time trajectory

+ x- x ct  tan  = x/ct = v/c =  tan  max = 1  max = 45° 45° v = c 45° v = c light sent backwards Velocities in space-time

“absolute past” + x- x ct “absolute future” “absolute elsewhere” x1x1 ct 1 no message sent from the origin can be received by observers at x 1 until time t 1 there is no causal contact until they are “inside the light cone” Space-time cones

+ x- x ct “absolute future” “absolute past” “absolute elsewhere” Space-time cones (2)

+ x- x ct  ST light rays & trajectory

+ x- x ct  From other frame?

+ x- x ct  Distort trajectory space axis

+ x- x ct  Distort trajectory space axis (2)

+ x- x ct  Distort trajectory space axis (3)

+ x- x ct   Constant c in both coords

+ x- x ct   Constant c in both frames (2)

+ x- x ct   S S´S´ Coord grid in both frames

+ x- x ct Spacetime Showdown Spacetime showdown

Relativistic Optics Relativistic Optics

v  t =   t f = 1/  t = 1/  t = f/  Transverse Doppler Reddening Transverse Doppler effect

Shadow of stationary cube a

v Shadow of Galilean moving cube

v

v ( a v/c ) 2 + ( a  1 - (v/c) 2 ) 2 = a 2 Shadow of relativistic cube a  1 - (v/c) 2

v ( a v/c ) 2 + ( a  1 - (v/c) 2 ) 2 = a 2 a Terrell Rotation (1959) Equivalent Terrell rotation a  1 - (v/c) 2

Penrose (1959): A Sphere By Any Other Frame Is Just As Round Penrose sphere

v Simultaneous snapshot?  h 2 +d 2 h

v More generally, from somewhat off-axis  hyperbolic curvature Apparent curvature  h 2 +d 2 h

SS 433 If assumed distance to object increases, so must the distance traversed by jet to preserve same angular scale for “peaks” and, hence, jet velocity must increase. History of jet precession (period = 162 days) Jet orientation fixed by relative Doppler shifts Light observed from a given point in the jet was produced  t = (s-d)/c earlier, thus distorting the apparent orientation of the loops d vv  s SS 433

Jet aberation

Can fit distance to the source = 5.5 kpc (K. Blundell & M. Bowler) Can even show evidence of jet speed variations! SS 433 distance fit

Angular compression towards centre of field-of-view Intensity = increases towards centre light received solid angle “Headlight Effect” Angular compression & headlight effect

From “Visualizing Special Relativity”