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Einstein’s Happiest Thought David Hodgson Carolian Astronomy Society 8 th Nov 2017

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Page 1: Einsteins Happiest Thought - Carolian Astrocarolianastro.co.uk/wpastro/wp-content/uploads/2017/11/Einsteins... · Thyssen-Krupp Tower Rottweil. 28 July 1945 Betty Lou Oliver survives

Einstein’sHappiestThought

DavidHodgsonCarolian AstronomySociety

8th Nov2017

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QuizWeightlessnessisexperiencedbyaperson:

1. anywhereinspaceregardlessofmotion2. inspacebutoutsidetheearth’satmosphere3. infreefallinagravitationalfield4. ontheMoon5. onlyinanorbitingsatellite

Page 3: Einsteins Happiest Thought - Carolian Astrocarolianastro.co.uk/wpastro/wp-content/uploads/2017/11/Einsteins... · Thyssen-Krupp Tower Rottweil. 28 July 1945 Betty Lou Oliver survives

...ledEinsteintoGeneralRelativity

...whichisEinstein’stheoryofgravity

..butwhyshouldwecare?What’swrongwithNewton’stheoryofgravity?

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NewtoniangravityOKaslongas:

b)speedsmuchlessthanspeedoflighta)gravityisweakasinsolarsystem

Hencenogoodfor:neutronstars,blackholes,supernovae,gammaraybursts,gravitationalwaves,theoriesoftheuniverse

Conclusion:AstronomersneedGeneralRelativity

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Firstthebadnews...

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...andnowthegoodnews

OnecanunderstandthefundamentalsofGeneralRelativitythroughsimplephysicalargumentsandalittlemaths

Butfirstletustakeabrieftourthroughthehistoryofgravity

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Aristotle350B.C.Heavyobjectsfallfasterthanlightones

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Galileo’sDiscorsi 1638Heavyobjectsfallatthesamespeedaslightones

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...and

• GalileostatedNewton’sFirstLawbeforeNewton:i.e.Abodywillcontinueinitsstateofrestoruniformmotioninastraightlineunlesssloweddownbyfriction.

Page 10: Einsteins Happiest Thought - Carolian Astrocarolianastro.co.uk/wpastro/wp-content/uploads/2017/11/Einsteins... · Thyssen-Krupp Tower Rottweil. 28 July 1945 Betty Lou Oliver survives

...moreaccurately:withthesameacceleration

g=10(m/s)/stime dist0 01 5

2

3

20

45

speed010

20

30

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Newton1670

What’swrongwiththispicture?

2dMmGF =

M

m

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Newtonhimselfwrotein1692:“Thatonebodymayactuponanotheratadistancethroughavacuum,withoutthemediationofanythingelse,byandthroughwhichtheiractionandforcemaybeconveyedfromonetoanother,istomesogreatanabsurditythatIbelievenoman,whohasinphilosophicalmattersacompetentfacultyofthinking,caneverfallintoit.”

Page 13: Einsteins Happiest Thought - Carolian Astrocarolianastro.co.uk/wpastro/wp-content/uploads/2017/11/Einsteins... · Thyssen-Krupp Tower Rottweil. 28 July 1945 Betty Lou Oliver survives

What’swrongwithNewton’stheoryofgravity?

FixedbyEinsteinin1915withhisGeneralTheoryofRelativity

• Actionatadistance• Forcetransmittedinstantaneously• i.e.ifSunsuddenlyceasedtoexistEarthwouldinstantlyshootoffatatangent• Timeisabsolute

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FieldfromAcceleratedMass

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SomethingelsewrongwithNewton’stheory

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OK,Newtonwasn’tquiterightbuthowdidEinsteincorrecthis

theory?

Answer:HishappiestthoughtplussomefancygeometryduetoGaussandRiemann

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CarlFriedrichGauss1777-1855Inventeddifferentialgeometrywhichdealswithcurvedspacese.g.thehyperboloid

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Gaussaged8Addnumbersfrom1to100

51495248

964973982991

!!

5050490010050 =++=Sum

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Sphere(2Dspace)withGeodesic(shortestdistancebetweentwopoints)

Whentwoinitiallyparallelgeodesicsmeet,itindicatesintrinsiccurvature

Locallyflat

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Cylinderwithsimplegeodesics

Geodesicsstayparallelas“curved”surfaceisanintrinsicallyflatspace

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Howtocharacteriseaspace

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OrusePythagorastotestflatness

4 5

3

25169..543 222

=+=+

ei

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Pythagorasin3D

a

c

b

d

d2= a2+b2+c2

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Iftrianglesmallenoughthena2+b2=c2i.e.locallyflat

a

b

c

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AnotherformofPythagoras

y

x

dx

dyds ds2 =dx2 +dy2 (METRIC)

dx =asmalldistanceinthex-direction

Characteristicofflatspace

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Minkowski andSpace-Time

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Space-TimeDiagramt(hours)

x(miles)

1.00

0.75

0.50

0.25

1 2 3 4

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Space-time

x

y

tworldliney

x

SuttonParkRd

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InSpecialRelativity

ds2 =dx2 +dy2 – c2 dt2

x

y

ct

cdtdx

dyworldline

Flatspace-time

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PropertiesofCurvedSpaces(andspace-times)

1. Ageodesicistheshortest“distance”betweentwopointsandisthereforethenearestthingtoastraightline.

2. Ifinitiallyparallelgeodesicsintersect,thenthespaceiscurved.

3. Locallygeometryisflat.

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FramesofReference

y

x

O

Time(s)

0

1

2

3

(x,y)(x’,y’)

y’ v

x’

O’

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Viewedfromtrain

sxlightofspeed

xheightTime 6.118.022===

0.8light

seconds

Tickingclock

V=0.6

dx’=0,dt’=1.6 ds2 =dx’2 –dt’2 =02 -1.62 =-2.56

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ViewedfromPlatform

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ViewedfromPlatform

dx=1.2,dt=2 ds2 =dx2 –dt2 =1.22 -22 =-2.56

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Einstein’sHappiestThought

IwassittinginachairinthepatentofficeinBernewhensuddenlyathoughtoccurredtome:“Ifapersonfallsfreelyhewillnotfeelhisownweight.“Iwasstartled.Thissimplethoughtmadeadeepimpressiononme.Itimpelledmetowardatheoryofgravitation.

A.Einstein1907

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Einstein’sHappiestThought1907

Infreefallalleffectsofgravitydisappear.Canaccelerationcancelgravity?

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Thyssen-KruppTowerRottweil

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28July1945BettyLouOliversurvives75floorfall

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FallingLiftandWeightlessness

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Orbitingsatellitealsoinfreefall

FallenthisfartowardsEarth

Gravity

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Fallingobjectinspace-time

Infallingliftgeodesicsbecomestraightlines

t

Distancefromground,y

Ingravity

geodesict

Distancefromfloor

Inlift

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LimitedsizeofEinstein’sLift

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LimitedsizeofEinstein’sLift

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ExplainsTides

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StarinellipticgalaxyRXJ1242-11tornapartbytidalforcesduetoblackhole

(artist’simpression)

NASA’sChandraX-rayandESA’sOpticalObservatories

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Earth-MoonTides

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Lifeinafreelyfallingframe

Foranygravitationalfieldtheeffectsofgravityarenullifiedinafreely-fallingframeoflimitedextent.Howeverthetidalforcesarenoteliminated.

Insuchaframethespace-timegeometryisflat.

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Howtotellaspace-timeiscurved

x

y

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Intersectionofinitiallyparallelgeodesicsmeanscurvature

y

x

t

Earth’scentre

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Einsteindevelopshishappiestthought

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Einstein’sEquivalencePrinciple

Itisimpossibletodistinguishbetweenastationaryframeofreferenceinagravitationalfieldgandaframeacceleratingwithaccelerationgbyanyphysicalexperiment.

Let’sapplyittoabeamoflight

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FirstuseEinstein’shappiestthought

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...thentheEquivalencePrinciple

Gravitydeflectsabeamoflight

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GravitationalRedShift

E

R

h

R v

Accelg

InthistimeRacquiresanextravelocityv=gt =gh/c

EERcgh

cv lll )1()1( 2+=+=

Timetforphotontotravelheighth=h/c

HenceRisrecedingfromthesourcewithvelocitygh/cwhenitreceivesthephoton.Henceredshift.

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ApplyPrincipleofEquivalence

MustalsobeagravitationalredshiftonEarth’ssurface h

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...whichinturnimplies

ACLOCKPLACEDHIGHINAGRAVITATIONALFIELDRUNSFASTERTHANANIDENTICALCLOCKLOWERDOWN

Whathappensnearablackhole?

ERcgh tt )1( 2+=

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Space-timedistortedbygravity

x

t

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PoundandRebka,Harvard1959

mhsmg 5.22,/8.9 2 ==

152 105.2 -= xcgh

15105.2 -=D xll

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Gravitymodifiesspace-timemetric

222

222 )21( dtcrc

GMdydxds --+=

x

ct

y

Newtonianorbit

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Einsteinconfirmed

222

222 )21( dtcrc

GMdydxds --+=

Largemassmodifiesthesetermstogivecorrectiontonewtonian orbite.g.CorrectpredictionoftheprecessionofMercury’sorbit.