a quantum potential approach to spin superposition in neutron interferometry
TRANSCRIPT
Volume 121, number3 PHYSICSLETTERSA 13 April 1987
A QUANTUM POTENTIAL APPROACH TO SPIN SUPERPOSITIONIN NEUTRON INTERFEROMETRY
C.DEWDNEYDepartmentofAppliedPhysics,PortsmouthPolytechnic,ParkBuilding, KingHenryIStreet,PortsmouthP012DZ, UK
P.R. HOLLAND andA. KYPRIANIDISInstitut HenriPoincaré,LaboratoiredePhysiqueTheorique,11, rue PierreetMarie Curie, 75231Paris Cedex05, France
Received12 January1987; acceptedfor publication6 February1987
Thecausalinterpretationof thePauliequationis shownto provideanunderstandingof spin superpositionin neutroninterfer-ometryin termsofwell-definedindividual particletrajectorieswith continuouslyvariablespin vectors.
In a recentpaper[1] it wasshownthat the causal depictedin fig. I. A beampolarizedin the z-direc-interpretationof quantummechanics[2] canpro- tion (definedby aguidefield B intothepaper)entersvide a clearunderstandingof thespatialinterference thedeviceandissplit into anupper(II) anda lowerobserved in neutron interferometers.The simple (I) component.Theupperbeamis passedthroughamodeusedto facilitate this descriptionconsistedin devicewhich inverts the spin. The two beamswithreplacingthesetsof crystalplaneswith squarepoten- oppositespin convergeon the lastsemi-transparenttial barriers,in orderto simulatetheactionof semi- surfacewhereeachbeamis split oncemore.Conse-transparentsurfaces,andtheuseof numericalmeth- quently the emergingforward anddeviatedbeamsodsto solvethe appropriatetime-dependentSchrö- both contain a coherentsuperpositionof compo-dingerequation. nentsofoppositespin.Representingtheeffectof the
In this contributionthe aim is to show how the semi-transparentsurfaceby a squarepotential V wecausal interpreationcan also account for the spin maywrite theappropriatePaulihamiltonianassuperpositionexperimentscarriedoutwith neutron H— — (h 2/2m)V2+ V+ 0
interferometers[31which haveconfirmedthewell- — I12
knowntheoreticalresultthatthesuperpositionofspin whereB is the uniform guidefield, andp is theneu-up andspindown beams(in thez-direction)results tron magneticmoment.The initial two-componentin a polarizationvectorlying in thexyplane.Wehave spinor (thatis, justbeforethefinal semi-transparentalreadydemonstrated[4] how the causalinterpre- surface)is a superpositionof two wavepacketsasso-tation of the Pauli equation [5] canbe appliedto ciatedwith thespin up anddownbeams:elementaryspinphenomena.Thesecalculationshave / qi
shownhowquantumphenomenaassociatedwithspin q’0 ( lo
maybe explainedin termsof ensemblesof individ- \ e5
ualparticletrajectorieswithwell-definedbutcontin- Herex is the relativephasedifference(introduceduously variable spin vectors subject to the spin by an aluminium sheet)which may be varied bydependentquantumpotentialandquantumtorque. rotatingthe sheetsothat it presentsdifferent thick-
In orderto calculatethetrajectoriesandspin vec- nessesto eachbeamcomponent,andtor orientationsin the contextof the simplemodelreferredto above,we considerthe interferometeras !Pi~=A exp[ — (x— 0.5)2 /4o~+ ik
0x]
0375-960l/87/$03.50© ElsevierSciencePublishersB.V. 105(North-HollandPhysicsPublishingDivision)
Volume 121, number3 PHYSICSLETTERSA i3 April 1987
yFig. I. Neutron interferometermodelwith onespinrotatingcoil andphaseshifter.
qiulo=A exp[—(x—l)2/4c~—i(k0x+~)], ~h(Th~i/at+cos0oØ/at)+~mv
2+Q+H0+ V=0,
whereA is a constant,a0 is the initial half width, where Q= — (h2/2m)V2R/R is the usual quantum
k~/2misthe incident energyandC1 isa constantfac- potentialandtor introducedtosymmetrizethetwo wavefunctions H
0 = (h2/8m)[(V 0)2 + sin20(V 0)2] — (2pI1~)s~B
with respectto thepotential.To determinetheevolutionof the spinvectorand is a spin-dependentaddition.The particleenergyis
positionof a particlewe first note that the internal givenbydegreesof freedommaybe representedby the Euler — ~h(8~/8t+cos 0 aØ/at)angles0(x, t), Ø(x, t), ~t’(x,t) in termsofwhich thespinorfield at time t takestheform which, like thevelocity (2), containsa spindepend-
ent contribution.
aw/2(
cos(0/2)e”~2‘\
~(x, t) =R e sin(0/2) e_~2) (1) A quantumforcemdv/dt=—V(V+Q)—(2pIh)(VBk)sk
whereR(x, t) is a realamplitudefunction.Thespinvectoris given by — (h2/4mp)ö~[p(V 0 0k° +sin2OVO äkØ)]
qit
0qJ
s=~h k=l,2,3,p
thusactswhich introducesa new form of spin—orbit
= ~h(sin 0 sin0, sin0 cos 0, cos 0) couplinggiving riseto trajectorieswhich dependonthe spin even in the absenceof external magnetic
with p= = R2andthe velocity,derivedfrom the fields.The equationof motionof thespinvectormay
Paulicurrent,by bewritten
v=(h/2m)(V~v+cos0 VØ). (2) ds/dt=T+(2p/h)BXs,
In termsof thevariablesp,0, 0, ~ thePauliequation whereimpliesa continuityequation T= (l/mp)sxôk(pôkS)
op/at+div(pv)=0,is an additionalquantummechanicaltorquewhich
anda Hamilton—Jacobiequation: similarly maygive risetonon-stationaryspinvectors
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Volume 121, number3 PHYSICSLETTERSA 13 April 1987
I I I I
1.05 -
0.45
0 40 I I I I I I I I I0 00 2 00 4 00 6.00 8 00 10.00 12 00 14.00 16 00 15 00
1010
NEUTRON TRAJECTORIES SPIN SUPERPOSITIONFig.2. Particletrajectoriesatthelast semi-transparentsurface.
evenin theabsenceof magneticfields. figuresallowsustoseetheway inwhich thespinori-FromthenumericalsolutionofthePauliequation entationchangesin a continuousmannerduringthe
we may calculatethe spin vectororientationsfrom scatteringfrom the final semi-transparentsurface.(1) andthetrajectoriesfrom (2) by writingv= dx/dt Fig. 4 showstheazimuthalangle0 andin this figureandspecifyingthe initial position (which of course we haveneglectedthe purely classicalprecessionofin practiceis unknown). In fig. 2 ~ we displaythe the spin vector about the guide field. Clearly thetrajectoriesfrom thegaussiandistribution of initial averagevalueof the spin isconserved.Changingthepositionsin eachcomponentbeam.The horizontal relativephasedoesnotaffectthepolaranglebutdoes,lines indicatethe position of the squarepotential. asis shown in fig. 5, causethe final directionof theNoticethatall thetrajectoriesoriginatingin theupper spinvectorin the xyplaneto be rotated.How this(lower) beam inside the interferometerenterthe arisescanbeseenif wewriteupper(lower) beamoutside.This leadsasexpected / R ~ ~
to an equalcountratein thetwo detectorsindepen- ~= ( 1S2/h •~
dentof therelativephase. \R2 e eThe spin orientationfields 0(x, I) andØ(x, t) are .andcomparewith (1). Thisgives
shown in figs. 3 and 4. In the emergingbeamsthespinvectorliesin thexy plane(0=x/2) asshown in 0=2tan~(R2/R1),fig. 3. Superposingthetrajectoriesmentally on these
çti=(S1 +S2)/h+it/2+X,
0 Inthefiguresweputh= 1, m=O.5,~~=O.O5,k0=50E.
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Volume 121, number3 PHYSICSLETTERSA 13 April 1987
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Fig. 3. Thepolarorientationangleof thespin vector0(x, t) plottedon a meshof pointsassociatedwith fig. 2.
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2,00 4 00 6 00 6,00 10,00 2,00 14.00 16,00 18,00
,dONEUTRON INTERFEROMETRY SPINSUP PHI
Fig.4. Theazimuthalorientationangleof thespin vectorØ(x, t) associatedwith fig. 2.
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Volume121, number3 PHYSICSLETTERSA 13 April 1987
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NEUTRON INTERFEROMETRY SPINSUP 10 PHI
Fig. 5. Theazimuthalorientationangleof thespin vectorwith anadditionalrelativephasex~introducedby rotatingthephaseplate.
0 (S1 S2)/hit/2~. thetimethewave packetpassed.
However, if the spin rotationon beamII is carried By measuringthespinina directionin thexy planeoutwith a time-dependentradiofrequencyspin flip or, as is in fact done,in the z-directionafter a ~tf2coil [7] the situationis ratherdifferent.Theuseof spin turn coil, anintensityvariationwith respecttosucha deviceintroducesanenergyexchangebetween therelativephasemaybeobserved.Sucha measure-the neutronandthe coil, an effect notpresentwith ment could in principle be carried out using astatic magnetic fields, and this raises interesting Stern—Gerlachapparatus,butweshouldguardagainstproblemsof interpretationdiscussedelsewhere[8]. unwarrantedinferencesfreomsuchresults.If thespinIt also producesa time-dependentrelative phase. is measuredin the z-directionoutsidethe interfero-Eachneutronpassingthroughtheapparatuswill suf- meter,in theabsenceof~t/2spinturncoils, theresultfer a differentphaseshift dependingon the phaseof is not relatedto which beampath the neutrontookthe coil as it passes.Thetotal relativephaseis then insidetheinterferometer,asmaybenaivelyexpected
x — w~t. Thedirectionof the spinvectoroutsidethe from the extensionof classicalideasinto this quan-interferometerthusrotatesin thexyplane,requiring tumphenomenon.Accordingtothecalculationspre-a detectionprocesssynchronizedwith the phaseof sentedhereboth resultsspin up andspin down canthecoil torevealthesuperposition.Thesimplemodel be achievedwith neutronsthathavetravelledalongusedheredescribeseventsafterthespinflip hastaken eitherpath,andthe spin measurementprocesscanplace,thusa time-dependentrelativephasecanonly be accountedfor in a deterministicmanner.Eachbesimulatedin a seriesof “stills” eachwith a differ- emergingneutronhasawell-definedspinvectorlyingent relativephase.Of course,eachindividual neu- in the xy planeand a definite position within thetron,apartfrom theprecessionabouttheguidefield, beamas it entersthe Stern—Gerlachapparatus.Thehasa staticspin vectororientationoutsidetheinter- interactionwith the inhomogeneousfield producesferometerwhich dependson the stateof the coil at two separatingbeams,the neutronenteringoneor
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Volume 121, number3 PHYSICSLETTERSA 13 April 1987
the other depending on its initial position at the the Royal Society, the SERCand the French Gov-entranceslit. As the beamsseparatethe quantum ernmentrespectively for grants which made thistorquerotatesthe spinvectorto lie alongor opposed researchpossible,andthe IHP for its hospitality.to thefield gradient.Thuswemaychooseto measurethe spin in the z-direction or in a perpendiculardirection afterthe neutronhasenteredthe appara- Referencestus.Thequentumpotentialapproachshowsthatthereis no needto concludethat the choiceof what to [1] C. Dewdney,Phys.Lett. A 109 (1985) 377.
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dam, 1960);ified initial conditions. This is important to bear in
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ments[9] which aredesignedto showthat theact of Phys.Lett.A 90(1982)110;
observationcan affect the set of events occurring G. Badurek,H. Rauch,J. Summhammer,U. KischkoandA.
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phenomenaassociatedwith spin superpositionneu- [4] C. Dewdney,P.R.HollandandA. Kyprianidis,Phys.Lett. A
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TheauthorsC.D.,P.R.H.,andA.K. wishto thank
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