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Einstein’sHappiestThought
DavidHodgsonCarolian AstronomySociety
8th Nov2017
QuizWeightlessnessisexperiencedbyaperson:
1. anywhereinspaceregardlessofmotion2. inspacebutoutsidetheearth’satmosphere3. infreefallinagravitationalfield4. ontheMoon5. onlyinanorbitingsatellite
...ledEinsteintoGeneralRelativity
...whichisEinstein’stheoryofgravity
..butwhyshouldwecare?What’swrongwithNewton’stheoryofgravity?
NewtoniangravityOKaslongas:
b)speedsmuchlessthanspeedoflighta)gravityisweakasinsolarsystem
Hencenogoodfor:neutronstars,blackholes,supernovae,gammaraybursts,gravitationalwaves,theoriesoftheuniverse
Conclusion:AstronomersneedGeneralRelativity
Firstthebadnews...
...andnowthegoodnews
OnecanunderstandthefundamentalsofGeneralRelativitythroughsimplephysicalargumentsandalittlemaths
Butfirstletustakeabrieftourthroughthehistoryofgravity
Aristotle350B.C.Heavyobjectsfallfasterthanlightones
Galileo’sDiscorsi 1638Heavyobjectsfallatthesamespeedaslightones
...and
• GalileostatedNewton’sFirstLawbeforeNewton:i.e.Abodywillcontinueinitsstateofrestoruniformmotioninastraightlineunlesssloweddownbyfriction.
...moreaccurately:withthesameacceleration
g=10(m/s)/stime dist0 01 5
2
3
20
45
speed010
20
30
Newton1670
What’swrongwiththispicture?
2dMmGF =
M
m
Newtonhimselfwrotein1692:“Thatonebodymayactuponanotheratadistancethroughavacuum,withoutthemediationofanythingelse,byandthroughwhichtheiractionandforcemaybeconveyedfromonetoanother,istomesogreatanabsurditythatIbelievenoman,whohasinphilosophicalmattersacompetentfacultyofthinking,caneverfallintoit.”
What’swrongwithNewton’stheoryofgravity?
FixedbyEinsteinin1915withhisGeneralTheoryofRelativity
• Actionatadistance• Forcetransmittedinstantaneously• i.e.ifSunsuddenlyceasedtoexistEarthwouldinstantlyshootoffatatangent• Timeisabsolute
FieldfromAcceleratedMass
SomethingelsewrongwithNewton’stheory
OK,Newtonwasn’tquiterightbuthowdidEinsteincorrecthis
theory?
Answer:HishappiestthoughtplussomefancygeometryduetoGaussandRiemann
CarlFriedrichGauss1777-1855Inventeddifferentialgeometrywhichdealswithcurvedspacese.g.thehyperboloid
Gaussaged8Addnumbersfrom1to100
51495248
964973982991
!!
5050490010050 =++=Sum
Sphere(2Dspace)withGeodesic(shortestdistancebetweentwopoints)
Whentwoinitiallyparallelgeodesicsmeet,itindicatesintrinsiccurvature
Locallyflat
Cylinderwithsimplegeodesics
Geodesicsstayparallelas“curved”surfaceisanintrinsicallyflatspace
Howtocharacteriseaspace
OrusePythagorastotestflatness
4 5
3
25169..543 222
=+=+
ei
Pythagorasin3D
a
c
b
d
d2= a2+b2+c2
Iftrianglesmallenoughthena2+b2=c2i.e.locallyflat
a
b
c
AnotherformofPythagoras
y
x
dx
dyds ds2 =dx2 +dy2 (METRIC)
dx =asmalldistanceinthex-direction
Characteristicofflatspace
Minkowski andSpace-Time
Space-TimeDiagramt(hours)
x(miles)
1.00
0.75
0.50
0.25
1 2 3 4
Space-time
x
y
tworldliney
x
SuttonParkRd
InSpecialRelativity
ds2 =dx2 +dy2 – c2 dt2
x
y
ct
cdtdx
dyworldline
Flatspace-time
PropertiesofCurvedSpaces(andspace-times)
1. Ageodesicistheshortest“distance”betweentwopointsandisthereforethenearestthingtoastraightline.
2. Ifinitiallyparallelgeodesicsintersect,thenthespaceiscurved.
3. Locallygeometryisflat.
FramesofReference
y
x
O
Time(s)
0
1
2
3
(x,y)(x’,y’)
y’ v
x’
O’
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
ViewedfromPlatform
ViewedfromPlatform
dx=1.2,dt=2 ds2 =dx2 –dt2 =1.22 -22 =-2.56
Einstein’sHappiestThought
IwassittinginachairinthepatentofficeinBernewhensuddenlyathoughtoccurredtome:“Ifapersonfallsfreelyhewillnotfeelhisownweight.“Iwasstartled.Thissimplethoughtmadeadeepimpressiononme.Itimpelledmetowardatheoryofgravitation.
A.Einstein1907
Einstein’sHappiestThought1907
Infreefallalleffectsofgravitydisappear.Canaccelerationcancelgravity?
Thyssen-KruppTowerRottweil
28July1945BettyLouOliversurvives75floorfall
FallingLiftandWeightlessness
Orbitingsatellitealsoinfreefall
FallenthisfartowardsEarth
Gravity
Fallingobjectinspace-time
Infallingliftgeodesicsbecomestraightlines
t
Distancefromground,y
Ingravity
geodesict
Distancefromfloor
Inlift
LimitedsizeofEinstein’sLift
LimitedsizeofEinstein’sLift
ExplainsTides
StarinellipticgalaxyRXJ1242-11tornapartbytidalforcesduetoblackhole
(artist’simpression)
NASA’sChandraX-rayandESA’sOpticalObservatories
Earth-MoonTides
Lifeinafreelyfallingframe
Foranygravitationalfieldtheeffectsofgravityarenullifiedinafreely-fallingframeoflimitedextent.Howeverthetidalforcesarenoteliminated.
Insuchaframethespace-timegeometryisflat.
Howtotellaspace-timeiscurved
x
y
Intersectionofinitiallyparallelgeodesicsmeanscurvature
y
x
t
Earth’scentre
Einsteindevelopshishappiestthought
Einstein’sEquivalencePrinciple
Itisimpossibletodistinguishbetweenastationaryframeofreferenceinagravitationalfieldgandaframeacceleratingwithaccelerationgbyanyphysicalexperiment.
Let’sapplyittoabeamoflight
FirstuseEinstein’shappiestthought
...thentheEquivalencePrinciple
Gravitydeflectsabeamoflight
GravitationalRedShift
E
R
h
R v
Accelg
InthistimeRacquiresanextravelocityv=gt =gh/c
EERcgh
cv lll )1()1( 2+=+=
Timetforphotontotravelheighth=h/c
HenceRisrecedingfromthesourcewithvelocitygh/cwhenitreceivesthephoton.Henceredshift.
ApplyPrincipleofEquivalence
MustalsobeagravitationalredshiftonEarth’ssurface h
...whichinturnimplies
ACLOCKPLACEDHIGHINAGRAVITATIONALFIELDRUNSFASTERTHANANIDENTICALCLOCKLOWERDOWN
Whathappensnearablackhole?
ERcgh tt )1( 2+=
Space-timedistortedbygravity
x
t
PoundandRebka,Harvard1959
mhsmg 5.22,/8.9 2 ==
152 105.2 -= xcgh
15105.2 -=D xll
Gravitymodifiesspace-timemetric
222
222 )21( dtcrc
GMdydxds --+=
x
ct
y
Newtonianorbit
Einsteinconfirmed
222
222 )21( dtcrc
GMdydxds --+=
Largemassmodifiesthesetermstogivecorrectiontonewtonian orbite.g.CorrectpredictionoftheprecessionofMercury’sorbit.