PNAS-1935-Stratton-316-21
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Journal article from Proc. Natl. Acad. Sci. 21 (1935), read April 22, 1935, by J.A. Stratton of MIT. It builds on his earlier note on solutions of the spheroidal wave equation, defines a second solution near z=0 using Legendre functions of the second kind, and derives its connection to the Bessel-type expansions via Laplace-type contour integrals. Special cases a=0, a=1 and Mathieu functions are discussed. The scan also includes the opening of Tolman's paper on thermal equilibrium in a gravitational field.
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PHYSICS: J.A.STRATTON
SPHEROIDAL FUNCTIONS OFTHESECOND KIND
ByJ.A.STRATTON
DEPARTMENT OFPHYSICS, MASSACHUSETTS INSTITUTE OFTECHNOLOGY
ReadbeforetheAcademy, Monday, April22,1935
InarecentnoteinthesePROCEEDINGS,I henceforth tobereferred toas
I,certainsolutions oftheequation
(1-z2)w'-2(a +1)zw'+(b-c2z2)w=° (1)
weredefined. Corresponding toadiscrete setofcharacteristic valuesof
theparameter b1thereexistsolutions ofthetype
Re,(c,z)=(CZ)-a-1/2EalJx+a+1/2(CZ)t (I-10)n
convergent throughout theentirez-plane andbehaving as(cz)-a-i sin
cz-+arasz-*co.Intheneighborhood ofz=0aformalsolution
maybeobtained intermsofanexpansion inhypergeometric functions,
54,(c,z)-'d,Tx(), (I-8)
whichforthecharacteristic valuesb1isalsobounded atthesingularities
z=k1.Withtheaidoftheintegralrepresentation (I-18)itwasshown
that(I-8)and(I-10)areproportional,
Sea1(c,z)=XlklRe1,z(c,z), (I-26)
andthattheexpansion coefficients arerelatedbythesimpleexpression
(I-22).
Anindependent particular solutionof(1)behaving atinfinityas(cz)-l
coscz-+ar)maybedefinedformally by
R21(c,z)=(cz)-a'/sEj'axNx+a+,12(cz). (I-ll)n
Thisexpansion, however, diverges ingeneralatthebranchpointsz=
=k1andconsequently isusableonlyforlargevaluesoftheindependent
variable. Itistheobjectofthepresent notetodefineasecondsolution
validintheneighborhood ofz=0,andtodetermine itsanalytic connection
withthefunctions (I-10),(I-ll).
Byanalogy withthedefinition (I4)ofthefunctions T,let
T"(S) =(1-Z2)-a/Qa( (2)316 PROC.N.A.S.
(2)
VL215PHYSICS: J.A.STRATTON
wheretheQn+.areAssociated Legendre functions ofthesecondkindas
definedbyHobson.2 IfR(n+a+1)>0,
eahiri(n +2-a+1)PTae;"r(n+a+1)(1-t2)X+a(z-t)-X2a1 dt.(3)
SinceboththeTx'andtheT"thusdefinedsatisfythesamerecursion
formulas, asecondformalsolution of(1)maybedefined,
Se2,&(c,z)=E',Txa(z), (4)U
whichmaybeexpected toconverge intheneighborhood ofz=0,since
E'dxisbounded whenbassumes oneofthecharacteristic valuesb1.
Itisknownthat(1)issatisfiedbytheLaplacetransform
w(z)=fe(l-t2)au(t)dt, (I-18)C
whereu(t)itselfsatisfies(1)andthecontourCistobedetermined bythe
bilinearconcomitant
eis(1-t2)a+l[icu -du 0. (I-19)
AsinIletu(t)=Sea,1(t)=Xgk1Re1j(ct). Ift-*oXandIargctI<7r,
Se,,a(t)-Xikl(ct)-'-1 sin(ct- +a)
Letitbeassumed thatI[c(z+1)]>0,I[c(z-1)]>0.Thisisinaccord
withtheconditions ofmostphysicalproblems wherein zisrealandI(c)>0.
Thecontour maynowstartandterminate att=+co.Inparticular a
solution mayberepresented by
*r~~(-I+J+,C' t)e.w(z)=J e'0'(1t2)Se1,(t)dt. (5)
r(-1+,1+)
LetIn,=Jf(~l+.i+)eis'(1-t2)Ta(t)dt
Thenonreplacing Tabythedifferential expression
Tx(t)=2 -1)r(n+1)na+1)(1-f2)-1x(1-t2)X+a,(6)()2x+,r(n+1)r(n+a+1) dtx( ),(6
andintegrating partially onefinds
r(n+2a+1) seU+G)Vi(cz)U f'(-4x=2ior(n+1)r(n+a+1) Ji'(t2 -1)x+adt.
(7)VOL.21,1935 317
PHYSICS: J.-A.STRATTON
IthasbeenshownbyWatson' that
r(-n -aJa)(-i+i+)J-ts-a_l/2(CZ)=2"a+.4 sl(t2_1)x+adt2 -2x+a+1irv"2ir e"~t
(8)
andhence
IK=5r(X+2±1(-_)'+'2A/fir5sinair(cz)-a-'/2J X.a-/2(Cz).r(n+1)
(9)
Multiply bothsidesof(9)byd4,replace4ontherightsidebya.according
to(I-22),andsumoveroddorevenvaluesofnasIisoddoreven.There
results
f(-1+l
w(z)=Je"'I(lt2)aSel4(t)dt=
2k,(-1)l+l sinar(cz) /2 --a-/(cz) (10)
Theintegralthusevaluated maybereadilyexpressed intermsofthe
functionsRe',,andRe'j,.Invirtueofthedefinition oftheNeumann
functionNx+,a+i,2 whennisaninteger,
Nx+a+l=/ -tanawrJx++a +,-((1)'J-n.a-1/2, (11)
cosair
itfollowsthat
(-l1)'+(cz) -a/ -t'agJ- x-a(cz)=cosar[tanarRela,I+Rea,j.(12)
Inthedomain 1<zcoonehastherefore
J e"(1-t2jSa,(t)dt=k1sin2air[tanairRea5,+Re,a].(13)
Thecontourintegral mustnow-beevaluated forvaluesofzlyingin
domain .-1<z<1.Toaccomplish this,letSe,j(t)bereplaced by
X1kgR4,g(ct) intheintegrand of(13)andconsiderintegrals ofthetype
Kx e -)a(Ctf4T/I J+a+q/m(d)dt. (14)-
TheBesselfunction maybereplacedby-''itsrepresentation asa-defihite
integral,
(C+a+ +a$t) (15)=2x"a/2-Ir(n +a+1)-1ied1 s+d, (5PROC.N.A.S. 318
PHYSICS: J.A.STRATTON
andonreversing theorderofintegration thereresultsfor(14),
2x+aV21Frr(n +a+1)fds(-s S
eict(s-5)(t2 l)a(ct)ndt. (16)
Letthecontour ofintegration betakenaroundthepoints(-1,+1)such
thatt>1overtheentirepath.Then(t2-1)"maybeexpanded ina
convergent seriesofinversepowersoft,anditmaybeshown4that
l+yl+)eict s(s-S)(t2 --)a(Ct)Xdt =
2,r+ mi2r(-a)Lr(m -a)C2M(z)2m-2a-x+. (17)
C2+ m=Om!r(-a)r(2m -n-2a)
K=12e'2(1)1+'sin2a
2n+aVwr(n +a+1) c9a+i
1(-1),r(m-a)r(n+ 2a+1-2m)mft(1-S2)n+am-o m2t(-2it)(18)
(Z-S)2m-2a-X-ldS
Nowby(3)itappears thatII
(1_-S)+a(Z_)2m2a ds=2+a+r(n+a+1) -avTa-"
FP(n+2a 2m+1)
(1nM
andonsubstituting in(18)andreducing, oneobtains
sn2a- "(-1)mr(m a)ma-2m
Knm=2*- --ea+1e-2me (+20) 1rcr~~~~~m=o m!r(-a) .(20)
(21)
(22)Finally, invirtueof(14)and(13),thereresults
-a"(-+,I+)
E'a,KI =e +eic (1a2)GS41(t)dt,
n olklJ
or
tanawrRe',a+Re,l =
e-a2ie -61)+112 .Ema=, O 2(-1)mr(m a)C2YTa'2m
m!1'-a) .+5
Theright-hand sideof(22)isnexttobeexpressed asamultiple ofthe
function Sr,edefined in(4).Inthesimple casea=0corresponding to
axiallysymmetric spheroidal functions, thesummation overmbreaksIl1VOL.21,1935 319
32YICYSICS: J.A.STRATTON
offwiththefirstterm.Replacing a.byd.,according to(I-22)yieldsat
once
Re=-e2Set,l. (23)C
Inordertodetermine theproportionality factor,letuswrite
'axe (-2)"x(m -)2"Tj+ =;q(c),'dxTx,(24)n m-om!r(-a) n
andevaluate attheordinary pointz=0.Byanobviousmodification of
Hobson's expressions forthefunctionsQx+.onthecrosscutbetween
16wehave
rn+2a +1)
Ta(o) =2a-1sn+2a 2 ' (25)
r(n22}
andacorresponding expression forTx,J+(o).Introducing thesevalues
into(24)oneobtains anexpression forthejoiningfactor,ulintermsof
theknownexpansion coefficients.
r(n+2a+1)
PI(C)E'dlxe2_ , =
n~~~~~rn+2a2+1
r(n+2)n+ a-m+
m.om!r(-a)2'm n+2m+2)rU2)
Theanalytic connection between thefunctions ofthesecondkindis
therefore
tanarRea,l+Rei,a=2(-1g4 X,p,S4g. (27)
Incaseaisaninteger,asinthespheroidal wavefunctions,Sea,,represents
theanalytic continuation ofReajintotheorigin. Inparticular
te-2;(a=0), (28)
and
b(bc+1)(a=1). (29)320 PROC.N.A.S.
PHYSICS: R.C.TOLMAN
Ifaishalfanoddinteger, asinthecaseoftheMathieu functions
(a=-1/2),tanawrin(27)becomes infinite. Thefunction (CZ)-a.-1/2
alJ-.-a-11,(cz),however, isthennolongerindependent ofRe4,'and,as
mightbeexpected, itiseasytoshowthatSe2,jisnowproportional to
Sea,'.Anindependent expression forSe!,1applicable inthiscasemaybe
obtained byalimitingprocess, thedetailsofwhichwillbepublished later.
IJ.A.Stratton, "Spheroidal Functions," Proc.Nat.Acad.Sci.,21,51-56(1935).
2E.W.Hobson, TheoryofSpherical andEllipsoidal Harmonics, p.193.
3G.N.Watson, TheoryofBesselFunctions, p.164.
4Whittaker andWatson, ModernAnalysis, 4thEd.,p.245.
6Hobson, loc.cit.,p.229.
THERMAL EQUILIBRIUM INAGENERAL GRAVITATIONAL
FIELD
ByRIcHARD C.TOLMAN
NORMAN BRIDGE LABORATORY OFPHYSICS, CALIFORNIA INSTJTUTE OFTECHNOLOGY
Communicated May9,1935
1.Introduction.-In theabsenceofanyappreciable gravitational field
theconditions satisfiedbythetemperature ofamediumhavingnothermal
flowfromoneportion toanother, arewellknowntobethoseofuniformity
throughout thesystem. Inthepresence ofagravitational field,however,
theconditions imposed atthermalequilibrium onthepropertemperature-
asmeasured atdifferent pointsofthemediumbylocalobservers-are
considerably morecomplicated, owingtotheassociation ofinertiaand
weightwithallformsofenergyandtheconsequent tendency forheatto
flowfromregionsofhighertothoseoflowergravitational potential.
Nevertheless, forthespecialcaseofstaticgravitational fields,thesemore
complicated conditions havealreadybeenobtained, ",2anditisthepurpose
ofthepresentarticletoinvestigate theconditions forthermalequilibrium
inthegeneralcaseofanykindofgravitational field.
Theinvestigation showsthatareasonably straightforward treatment
canbefoundwhichleadstoanapparently satisfactory, covariant expression
ofthegeneralconditions forthermalequilibrium. Thepossible valueof
sucharesultcanbetwo-fold. Inthefirstplaceitsatisfies ourdesirefor
coherent theory,sinceourpreviousexpression oftheconditions forthermal
equilibrium, whichappliedonlytostaticsystems andwasmadeinthenon-
covariant language ofakindofcoordinate systemthenappropriate, can
nowberegarded asaspecial caseofthegenerally covariant expression
applying toanykindofsystem. Inthesecondplace,theexpression ob-VOL.21,1935 321