Top Banner
Lecture Two
49

Lecture Two. Historical Background of Special Relativity.

Dec 21, 2015

Download

Documents

Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: Lecture Two. Historical Background of Special Relativity.

Lecture Two

Page 2: Lecture Two. Historical Background of Special Relativity.

Historical Background

ofSpecial Relativity

Page 3: Lecture Two. Historical Background of Special Relativity.

Principle of Relativity in Classical Mechanics

•Galilean transformation

•Newtonian Relativity

Page 4: Lecture Two. Historical Background of Special Relativity.
Page 5: Lecture Two. Historical Background of Special Relativity.

Galilean transformation

x' = x – v ty' = yz' = zt' = t

Page 6: Lecture Two. Historical Background of Special Relativity.
Page 7: Lecture Two. Historical Background of Special Relativity.

Measurement of length

EA = (tA, xA, yA, zA) marking of the left end A

EB = (tB, xB, yB, zB) marking of the right end B

Page 8: Lecture Two. Historical Background of Special Relativity.

Measurement of length

simultaneous measurement

tA = tB

length = xB - xA

Page 9: Lecture Two. Historical Background of Special Relativity.

tA = tB

Simultaneity is crucial in length measurement of

a moving rod.

Otherwise …

Page 10: Lecture Two. Historical Background of Special Relativity.
Page 11: Lecture Two. Historical Background of Special Relativity.

Under Galilean transformation

t'A = tA

t'B = tB

x'A = xA – v tA

x'B = xB – v tB

time is absolute

Page 12: Lecture Two. Historical Background of Special Relativity.

x'B - x'A= (xB – v tB) – (xA – v tA)

= xB - xA - v (tB – tA)

= 0

= xB - xA

Page 13: Lecture Two. Historical Background of Special Relativity.

Measurement of length

length = xB - xA

= x'B - x'ALength is invariant.

Page 14: Lecture Two. Historical Background of Special Relativity.

So much about measurement process

Now physics:

• kinematics

• dynamics

Page 15: Lecture Two. Historical Background of Special Relativity.

Notationv : relative velocity between inertial frames of reference

u : velocity of object

Page 16: Lecture Two. Historical Background of Special Relativity.

kinematics

u' = u - v(classical velocity addition theorem)

Page 17: Lecture Two. Historical Background of Special Relativity.
Page 18: Lecture Two. Historical Background of Special Relativity.

kinematics

a' = a

Page 19: Lecture Two. Historical Background of Special Relativity.

dynamics•mass is unaffected by the motion of the reference frame

F = m a = m a ' = F '

Page 20: Lecture Two. Historical Background of Special Relativity.

Principle of Relativity

• Laws of mechanics are the same in all inertial frames of reference.

namely

• Laws of mechanics are invariant under a certain transformation.

Page 21: Lecture Two. Historical Background of Special Relativity.

samemeans:

invariant under a certain transformation

Page 22: Lecture Two. Historical Background of Special Relativity.

Newtonian Relativity

• Laws of mechanics are the same in all inertial frames of reference.

namely

• Laws of mechanics are invariant under the Galilean transformation.

Page 23: Lecture Two. Historical Background of Special Relativity.

Eisteinian Relativity

• Laws of mechanics are the same in all inertial frames of reference.

namely

• Laws of mechanics are invariant under the Lorentz transformation.

Page 24: Lecture Two. Historical Background of Special Relativity.

Consequences of Relativity

• No mechanical experiments carried out entirely in one inertial frame can tell the observer what the motion of that frame is with respect to any other inertial frame.

• There is no way at all of determining the absolute velocity of an inertial frame.

• No inertial frame is preferred over any other.

whether Newtonian or Einsteinian

Page 25: Lecture Two. Historical Background of Special Relativity.

Example 3 Invariance of Momentum Conservation

• In S:

P = m1u1 + m2u2 = m1U1 + m2U2

• In S':

P ' = m1u1 ' + m2u2 ' = m1U1 ' + m2U2 '

Page 26: Lecture Two. Historical Background of Special Relativity.

Example 4Invariance of Equation of Motion

Page 27: Lecture Two. Historical Background of Special Relativity.

Electromagnetismand

Newtonian Relativity

Page 28: Lecture Two. Historical Background of Special Relativity.

Maxwell’s Equationsare not invariant

underGalilean transformation.

Page 29: Lecture Two. Historical Background of Special Relativity.

Maxwell’s Electrodynamical Laws are not the same in all inertial frames of reference.

Page 30: Lecture Two. Historical Background of Special Relativity.

“Ether” frame the inertial frame of reference in

which the measured speed of light is exactly

c = (00)-½ = 299792458 m/sec

Page 31: Lecture Two. Historical Background of Special Relativity.

In a frame of reference moving at a constant speed v with respect to the “ether” frame, the measured speed of light would range from c- v to c+ v.

Page 32: Lecture Two. Historical Background of Special Relativity.

Newtonian relativity holds for Newtonian mechanics but not for Maxwell’s laws of electromagnetism.

Page 33: Lecture Two. Historical Background of Special Relativity.

Three possibilities or alternatives

Page 34: Lecture Two. Historical Background of Special Relativity.

Arguments following Panofsky and Phillips

• Insisting the existence of Relativity Principle

• Fact: Incompatibility of Maxwell electrodynamics and Newtonian relativity

• Two choices of Relativity: Newtonian or new one

• Then there are only three alternatives:

Page 35: Lecture Two. Historical Background of Special Relativity.

Diagrammatic

N: Newtonian mechanics

N' : new mechanics

M: Maxwell electrodynamics

M' : new electrodynamics

G: relativity under Galilean transformation

G' : new relativity principle

: compatible

: incompatible, preferred frame

Page 36: Lecture Two. Historical Background of Special Relativity.

G N M

G N M '

G ' N ' M

preferred ether frame

No other alternatives

Page 37: Lecture Two. Historical Background of Special Relativity.

• First alternative: without any modification and sacrifice the relativity of electrodynamics.

• Second alternative: maintain Newtonian mechanics and insist Newtonian relativity of electrodynamics but give up Maxwell theory.

• Third alternative: maintain Maxwell electrodynamics and relativity but give up Newtonian mechanics and relativity.

Page 38: Lecture Two. Historical Background of Special Relativity.

Alternative 1Both Newtonian mechanics and Maxwell’s electrodynamics are correct.

Page 39: Lecture Two. Historical Background of Special Relativity.

Alternative 1

Then since Newtonian relativity holds for

Newtonian mechanics but not for Maxwell’s electromagnetism ,

Page 40: Lecture Two. Historical Background of Special Relativity.

Alternative 1

there must be a preferred absolute “ether” frame for electrodynamics.

Page 41: Lecture Two. Historical Background of Special Relativity.

Alternative 2

Newtonian relativity holds for both mechanics and electrodynamics.

Page 42: Lecture Two. Historical Background of Special Relativity.

Alternative 2

But then electromagnetism is not correct in the Maxwell formulation.

Page 43: Lecture Two. Historical Background of Special Relativity.

Alternative 3

Relativity Principle holds for both mechanics and Maxwell’s electrodynamics.

Page 44: Lecture Two. Historical Background of Special Relativity.

Alternative 3

But then the Relativity Principle is not Newtonian, the transformation is not Galilean,

Page 45: Lecture Two. Historical Background of Special Relativity.

Alternative 3

and the mechanics in the Newtonian form needs modification.

Page 46: Lecture Two. Historical Background of Special Relativity.

Alternatives 1 and 2 was ruled out by experiments of Michelson and Morley. (Next lecture)

Page 47: Lecture Two. Historical Background of Special Relativity.

Alternative 3 was realized by Einstein’s Special Relativity. (Fourth lecture)

Page 48: Lecture Two. Historical Background of Special Relativity.

The End

Page 49: Lecture Two. Historical Background of Special Relativity.

http://www.scu.edu.tw/physics/teacher/rency/