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Hwa-Long Gau 

and Pei Yuan Wu 

Abstract

Inthissurveyarticle,wegiveanexpositoryaccountoftherecentdevelopmentson

thePonceletpropertyfornumericalrangesoftheoperatorsS(). Itcanbeconsidered

as an updated and more advanced edition of the recent expository article published

intheAmericanMathematicalMonthlyby the secondauthoronthis topic. The new

informationincludes: (1)asimpli edapproachtothemainresults(generalizationsof

Poncelet, Brianchon{Ceva and Lucas{Siebeck theorems) in this area, (2) the recent

discovery of Mirman refuting a previous conjecture on the coincidence of Poncelet

curves and boundaries of the numerical ranges of nite-dimensional S(), and (3)

some partial generalizations by the present authors of the above-mentioned results

fromthe unitary-dilationcontexttothe normal-dilationone and alsofromthe

nite-dimensional S()to the in nite-dimensional.

||||||||||||||||||||||||

2000 Mathematics Subject Classi cation: Primary 15A60, 47A12; Secondary 14H99.

Key words and phrases: Numerical range, Poncelet property, unitarydilation.



ThisworkwaspartiallysupportedbytheNationalScienceCounciloftheRepublicof

Chinaunder research projects NSC-91-2115-M-008-011and NSC-91-2115-M-009-009

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Inrecentyears,theresearchonthenumericalrangesof nitematricesand

bound-ed operators has been very active, thanks tothe biennialconvening of the WONRA

(Workshop on Numerical Ranges and Numerical Radii). (For more information on

this, check the webpage http://www.resnet.wm.edu/cklixx/wonra02.html.) One

area of investigations concerns the numerical ranges of the nite-dimensional

com-pressions oftheshift. Itwasdiscovered thattheboundariesoftheirnumericalranges

possessthePonceletproperty,meaningthatthereexistin nitelymanypolygonswith

thepropertythateachhas allitsverticesonthe unitcircleand allitssides tangentto

theasserted boundary. Thisyieldsanunexpectedlinkbetweenthe twentieth-century

subject of numerical range and some nineteen-century gems of projective geometry.

Anexpository accountof this developmentwasgiven in[35], whichexplainsthe

per-tinent results in a historical context. The purpose of this survey is to update this

previous account by providinga simpli edapproach and expounding the recent

dis-coveries. ChiefamongthelatteristheonebyMirmanthatnoteveryalgebraicconvex

curveintheopen unitdisc whichhas thePonceletpropertyarisesasthe boundaryof

the numericalrange of the asserted operator, thus refuting aprevious conjecture on

identifying such numerical ranges by the Poncelet property. We will also elaborate

on our recent attempts in generalizing the main results in this area to more general

contextssuchasgeneralconvexpolygonsinsteadofpolygonswithverticesontheunit

circleandgeneralcompressionsoftheshiftinsteadofmerethe nite-dimensionalones.

In Section2 below, we start with abrief review of the de nition and basic

prop-ertiesof numericalranges ofoperatorsonaHilbert space. Wealsodiscuss thenotion

ofdilationand itsconnectionwith numericalranges. Section3 thentreatsnumerical

rangesof nitematrices. Here theextra toolofKippenhahn curve provesveryuseful.

Itinvolvesthe point-linedualityoftheprojectiveplane. Section4considersthe

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presented,eachofwhichhasitsmeritinexposingcertainpropertiesoftheirnumerical

ranges. Section 5 gives the main results on the Poncelet property for the numerical

ranges of the compressions of the shift on nite-dimensional spaces. There are three

of them: generalizations of the Poncelet porism (on the existence of in nitely many

interscribing polygons between twoellipses),Brianchon-Cevatheorem (on the

condi-tion for the tangent points of an inscribing ellipse of a triangle), and Lucas-Siebeck

theorem (on the relationbetween zeros of apolynomial and its derivative). We then

moveon tothe partial generalizationsof these results inSection 6.

2. Numerical Range

Let A be a (bounded linear) operator on a complex Hilbert space H. The

nu-merical range of A is the set W(A)  fhAx;xi : x 2 H;kxk = 1g in the complex

plane,whereh;idenotes theinnerproductinH. Inotherwords,W(A)istheimage

of the unit sphere fx 2 H : kxk = 1g of H under the (bounded) quadratic form

x 7! hAx;xi. Some properties of the numerical range follow easily from the

de ni-tion. Forone thing, the numericalrange isunchanged underthe unitary equivalence

of operators: W(A) = W(U 

AU) for any unitary U. It also behaves nicely under

the operation of taking the adjointof an operator: W(A 

) =fz :z 2W(A)g. More

generally,this is even the case when taking the aÆnetransformation: if

f(x+iy)=(a 1 x+b 1 y+c 1 )+i(a 2 x+b 2 y+c 2 )

is an aÆne transformation of the complex plane C, where x;y and a

j ;b j and c j ;j =

1;2,are all real and the latter satisfy a

1 b 2 6=a 2 b 1

, and if we de ne f(A)to be

(a 1 ReA+b 1 Im A+c 1 I)+i(a 2 ReA+b 2 ImA+c 2 I); where Re A = (A+A  )=2 and Im A = (A A 

)=(2i) are the real and imaginary

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of numericalranges, the reduction through aÆne transformations is a handy toolin

many situations.

The most importantpropertyof the numericalrangeis thatW(A) isalways

con-vex. This is the celebrated Toeplitz{Hausdor Theorem from1918-19 [31, 15]. Over

the years, therearenumerous proofsandgeneralizationsofthisfact. Theusualproof

is to rst reduce it to the case of 2-by-2 matrices (since the de nition of convexity

involves only two points at a time) and show that the numericalrange of the latter

is a closed elliptic disc or one of its degenerate forms (circular disc, line segment or

a single point). Indeed, if A = 

a b

0 c 

, then W(A) is the elliptic disc with foci a

and c and minor axis of length jbj. An easy proof of this is to reduce A to 

0 1

0 0 

viasome aÆnetransformationand check directlythatthe latterhas numericalrange

fz 2C :jzj1=2g (cf. [19]).

The numericalrange is abounded set, but isnot closed ingeneral. Forexample,

if S isthe (simple) unilateral shifton l 2 : S(x 0 ;x 1 ;)=(0;x 0 ;x 1 ;);

then W(S)equals the open unit discD =fz 2C :jzj<1g. However, ifthe operator

A acts on a nite-dimensionalspace, then W(A)is obviously closed and hence

com-pact. For an arbitrary operator A, the closure of its numerical range W(A) always

contains the spectrum (A). Hence the numerical range gives a rough estimate of

the locationof thespectrum. Thisisone of thereasonstostudy the numericalrange

and provides its main applications. If A is normal, then W(A) equals (A) ^

, the

convex hull of (A). Thus, in particular, if A is a normal ( nite) matrix, then

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ty boundedconvexset isthenumericalrangeofsomeoperatoronaseparableHilbert

space. (Note that if nonseparable Hilbert spaces are allowed, then every such set is

the numerical range of some normal operator; compare [26].) Even more intricate

is to determine, for each positive integer n, the numerical ranges of operators on

an n-dimensional space. Although many necessary/suÆcient conditions are known,

a complete characterization is beyond reach at this moment. One condition on the

boundaryofthenumericalrangeisworthnoting. If4isaclosedconvexsubsetofthe

plane, then every nondi erentiable point of the boundary @4 of 4 has two distinct

supporting lines of 4 with angle less then  such that the closed section formed by

them contains 4. Such a point is calleda corner of 4. Accordingto this de nition,

theendpointsofalinesegmentarecorners. AresultofDonoghue[8,Theorem1]says

that a corner  of W(A) which also belongs to W(A) is a reducing eigenvalue of A.

The latter meansthat there isa nonzero vectorx suchthat Ax=x and A 

x=x.

The proof of this makes use of the geometric fact that an elliptic disc which is

con-taining  and contained inW(A) must bereduced toa linesegment. It follows that

ifA isann-dimensionaloperator,thenW(A)can have atmostn corners. This gives

acertainconstraintonthe shapeofthe numericalrange ofa nite-dimensional

oper-ator. Usingthe condition forthe equality case of the Cauchy{Schwarz inequality,we

may prove the analogous result that any point  in W(A) satisfying jj = kAk is a

reducing eigenvalueof A.

Associated with the numerical range W(A) is the quantity w(A), the numerical

radius ofA,de ned by supfjzj:z 2W(A)g. Forexample,ifS isthe unilateralshift,

then w(S)=1, and if A is normal,then w(A)=supfjzj:z2 (A)g.

We say that the operatorA onspace H dilates toB on K or B compressesto A

if there is an isometry V from H to K such that A = V 

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form 

A 

  

. The notion of dilation and compression is closely related to that of

numericalrange. For one thing, the numericalrange itself can be described in terms

of dilation. Namely, for any operatorA, the numericalrange ofA is the same as the

set of complex numbers  forwhich the 1-by-1matrix [] dilatesto A. On the other

hand,ifAisanoperatorwhichdilatestoB,thenW(A)iscontainedinW(B). Hence

ajudiciouschoiceofanicelybehavedB canyieldusefulinformationonthenumerical

range of A. One type of dilation which will be fully exploited in our derivations in

Sections 5 and 6 is the unitary dilation of contractions. The classical result in this

respect is Halmos's dilation: every contraction A (kAk  1) can be dilated to the

unitary operator 2 4 A (I AA  ) 1=2 (I A  A) 1=2 A  3 5

(cf. [14, Problem 222 (a)). With more care, the unitary dilation can be achieved

in a most economical way: if A is a contraction on H, then A can be dilated to

a unitary operator U from H  K

1 to H  K 2 with K 1 and K 2 of dimension-s d A   dimran (I AA  ) 1=2 and d A  dimran (I A  A) 1=2 , respectively, and,

moreover, in this case d

A 

and d

A

are thesmallest dimensionsof such spaces K

1 and K 2 . Here d A and d A 

are calledthe defectindices ofthe contractionA. They provide

a measure on how far A deviates from the unitary operators and play a prominent

role in the unitary dilationtheory.

Propertiesofnumericalrangesofoperatorsarediscussedin[14,Chapter22];those

for nitematricesare in[16,Chapter 1]. Thetwoclassicmonographs[4]and [5]treat

thenumericalrangesofelementsofnormedalgebras;themorerecent[13]emphasizes

applications tonumerical analysis.

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can be exploited to yield special toolswhich are not available for general operators.

OnesuchtoolisthecharacteristicpolynomialofthepencilxRe A+yImAassociated

with any matrix A. This can be utilized in two di erent ways to yield W(A) or its

boundary. One is via Kippenhahn's result that the numerical range of A coincides

withtheconvexhulloftherealpartofthedualcurveofdet(xRe A+yIm A+zI)=0.

In this way, the classical algebraiccurvetheory can bebroughtto bear onthe study

here. On the other hand, a parametric representation of the boundary @W(A) can

alsobeobtained fromthelargesteigenvalue ofcosRe A+sinIm Ayielding useful

informationon W(A). Here we givea brief accountof both approaches.

Let CP 2

be the complex projective plane consisting of all equivalence classes

[x;y;z] of ordered triples of complex numbers x;y and z which are not all zero.

Two such triples [x;y;z] and [x 0 ;y 0 ;z 0 ] are equivalent if x =x 0 ;y=y 0 and z =z 0

for some nonzero . The point [x;y;z] (z 6= 0) in homogeneous coordinates can be

identi ed with (x=z;y=z) in nonhomogeneous coordinates. On the other hand, the

point (u;v) becomes [u;v;1] inhomogeneous coordinates. In this way, C 2

is

embed-ded in CP 2

. If p(x;y;z) is ahomogeneous polynomialof degree d inx;y and z, then

the set of points [x;y;z] in CP 2

satisfying the equation p(x;y;z)=0 is analgebraic

curve of order d. If C issuch a curve, then its dualC  is de ned by C  =f[u;v;w]2CP 2 :ux+vy+wz =0 is atangent lineof Cg: In this case, C 

is also an algebraic curve of order at most d(d 1) and d is called

the class of C 

. It is known that the dual of C 

is C itself. The point[x

0 ;y 0 ;z 0 ] isa

focus of C if it isnot equal to [1;i;0]and the lines through [x

0 ;y 0 ;z 0 ] and [1;i;0]

are tangent to C at points other than [1;i;0]. In general, if a curve is of class d

and isde ned by anequationwith real coeÆcients,then ithas d real fociand d 2

d

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p

A

(x;y;z)=det(xRe A+yImA+zI

n )

and let C(A) denote the dual curve of p

A

(x;y;z) = 0. Since p

A

is a real

homoge-neouspolynomialofdegreen, the curveC(A)isgiven by arealpolynomialofdegree

at most n(n 1), is of class n, and has n real foci [a

j ;b

j

;1];j = 1;;n, which

correspond exactlyto the n eigenvalues a

j +ib

j

of A. The connection of C(A) with

the numerical range W(A) is provided by a result of Kippenhahn [18]: W(A) is the

convex hull of the real points of the curve C(A), namely, the convex hull of the set

fa+ib 2C : a;b 2R;ax+by+z =0 istangent to p

A

(x;y;z)=0g. Kippenhahn's

result can be easily veri ed by noting that x = max (Re (e i

A)) is a supporting

line of W(Re(e i

A)) for any real . Since it can be shown that @W(A) contains

only nitely many line segments, the above result implies that @W(A) is piecewise

algebraic, that is, it isthe union of nitely many algebraiccurves.

There is another way to make the above to be more revealing. For any

nonemp-ty compact convex subset 4 of the plane, there is a natural parametrization of its

boundary @4. For any ;0    2, let L



be the ray from the origin which has

inclination fromthe positive x-axis,and letM



be the supporting line of 4 which

isperpendicular toL



. If d() isthe signed distance fromthe origin toM



, then @4

can be \parametrized" by ()=(x();y()), where

x() = d()cos d 0 ()sin; y() = d()sin+d 0 ()cos:

Itcanbeshownthatd()isdi erentiableforalmostallandisequaltomaxfRe (e i

z):

z 24g. In particular, if 4=W(A) forsome operator A, then

d() = max (Re (e i

A))

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A

inz has d()asa zero. Asan example,if A isthe 3-by-3 matrixdiag (1;i;0),then

d()= 8 > > > < > > > : cos if 0   4 or 3 2  2; sin if  4 ; 0 if    3 2 ;

and the naturalparametrization of @W(A) (=the triangularregion with vertices 1;i

and 0) isgiven by ()= 8 > > > < > > > : 1 if 0< <  4 or 3 2  < <2; i if  4 <<; 0 if < < 3 2 :

In particular, this shows that the natural parametrization is not a parametrization

in the usual sense: it does not traverse the line segments on the boundary; but the

convex hullof its imageequals @4.

4. Compression of the Shift

Compressions ofthe shift are aclass of operators studiedintensively inthe 1960s

and '70s. Playing arole analogous to the companion matrix in the rationalform for

nite matrices, they are the building blocks in the \Jordan form" (under

quasisim-ilarity) for the class of C

0

contractions. The whole theory is subsumed under the

dilation theory for contractions onHilbert spaces developed by Sz.-Nagy and Foias.

Thestandard referenceisthemonograph[30]; amore completeaccountofthe theory

of C

0

contractions isgiven in [3].

We start by noting that the unilateral shift S has another representation as

(Sf)(z) = zf(z) for f in H 2

, the Hardy space of square-summable analytic

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roinvariantsubspaces of S are ofthe formH 2

forsome innerfunction  (is inner

if it is bounded and analytic on D with j(e i

)j = 1 for almost all real ). The

compression of the shiftS() is the operator onH()H 2

H 2

de ned by

S()f =P(zf(z));

where P denotes the (orthogonal) projection from H 2

onto H(). Thus S() is the

operator in the lower-right corner of the 2-by-2 operator matrix representation of S

as 2 4   0 S() 3 5 on H 2 =H 2 H():

Thisclass ofoperatorswas rststudiedby Sarason[29] andhas been underintensive

investigationoverthe past 35years. In particular,it isknown that kS()k=1;S()

is cyclic (there is a vector f(= 1 (0)) in H() such that W

fS() n

f : n  0g=

H()), and its commutant fS()g 0 (fX on H() : XS() =S()Xg) and double commutant fS()g 00 (fY on H(): YX = XY for every X in fS()g 0 g) are both equal toff(S()):f 2H 1

g. The inner function  is the minimal function of S()

inasensesimilar tothe minimalpolynomialofa nite matrix,that is,itissuch that

(a)(S())=0,and(b) isafactor ofanyfunctionf inH 1

forwhichf(S())=0.

AnoperatorAis(unitarilyequivalentto)acompressionofthe shiftif andonlyif itis

acontraction,bothA n

andA n

convergeto0inthestrongoperatortopology,andthe

defect indicesd

A and d

A 

are bothequaltoone. Itfollowsfromtheseconditions that

the compression of the shiftis irreducible, that is, itcan have no nontrivial reducing

subspace.

For nitematrices,thecharacterizationofcompressionsoftheshiftineven easier:

Aissuchanoperatorif andonlyifitisacontraction,ithas noeigenvalueofmodulus

one and d

A

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(z)= n Y j=1 z a j 1 a j z ; wherea j

'sare theeigenvalues ofAinD. We letS

n

denotethe classof such matrices.

An example inS

n is J

n

, the n-by-nnilpotentJordan block

2 6 6 6 6 6 6 6 6 6 4 0 1      1 0 3 7 7 7 7 7 7 7 7 7 5 ;

withthecorrespondinginnerfunction(z)=z n

. BytheresultsinSection2,matrices

in S

n

admit unitary dilations on an (n+1)-dimensionalspace. For this reason, S

n

-matricesare called matricesadmittingunitary borderingorUB-matrices by Mirman

(cf. [21, 22, 23]). Since S() is de ned by its minimal function , we infer that for

any npointsa

1

; ;a

n

inD (notnecessarilydistinct)there isamatrixinS

n

, unique

uptounitaryequivalence,withthea

j

'sasitseigenvalues. Amorespeci cdescription

of a matrix inS

n

with eigenvalues the a

j 's is given by [a ij ] n i;j=1 , where (1) a ij = 8 > > > < > > > : a j if i=j; [ Q j 1 k=i+1 ( a k )](1 ja i j 2 ) 1=2 (1 ja j j 2 ) 1=2 if i<j; 0 if i>j:

This matricialrepresentation was rst discovered by Young [36, p. 235] (cf. also[28,

p. 201], [21, Theorem 4] and [11, Corollary 1.3]). In particular, it follows that S

2

consists of 2-by-2matrices which are unitarily equivalentto amatrix of the form

2 4 a (1 jaj 2 ) 1=2 (1 jbj 2 ) 1=2 0 b 3 5

with a and b in D. There is another representation for matrices in S

n

which is

useful for our discussions in Section 5. If A is in S

n

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diag (1; ;1;a) with 0  a < 1. The equality WAW 

= (WU)D shows that A is

unitarily equivalent to (WU)D, a matrix of the form

(2) [f 1 f n ] whose columns f j satisfy kf j k = 1 for 1  j  n 1;kf n k < 1 and f j ? f k for

1j 6=k n. Conversely, a matrix of the above form with noeigenvalue of

modu-lusone isin S

n .

>From the information we have so far on the compressions of the shift, we can

already deduce certain properties of their numerical ranges. Let A be a matrix in

S

n

. Then W(A) must be contained in the open unit disc D. This is because if  in

W(A)is suchthat jj=1(=kAk),then itwillbea reducing eigenvalue of A, which

contradicts the irreducibility of A. On the other hand, by Donoghue's result and

the irreducibilityof A,wemay deduce that the boundary ofW(A) isadi erentiable

curve. In the subsequent sections, we willdiscuss other ner propertiesof W(A).

5. Poncelet Property

The recentestablishmentofalinkbetweenthe numericalrangesofmatricesinS

n

and some classical geometric results from the 19th century was achieved by Mirman

[21, 23,22, 24] and the present authors [9, 10, 11,12]. Here we give a brief account

of this development.

Our rst result has to do with a geometric theorem of Poncelet. In this treatise

[27] of 1822, there is contained the following result,called Poncelet's porism or

Pon-celet's closure theorem: is C and D are ellipses in the plane with C inside D, and if

there is one n-goncircumscribed about and inscribed in D, that is, the n-gon has n

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the assertion says that some property (the existence of a circumscribing-inscribing

n-gon)eitherfailsor,ifitholdsforone instance,succeeds in nitelymanytimes. Itis

a closuretheorem since, fromany point on D,we draw atangentlineto C, which

intersects D atanother point,then repeatthis process bydrawing tangentlinesfrom

successivepointsobtained inthis fashion,andobtaintheresultingclosedn-gonwhen

thenthtangentlinereachesbackto. Vieweddynamically,thisgivesacon guration

ofrotatingn-gonswith di erentshapesbut allsharingthis circumscribing-inscribing

property. Sincethe appearance ofthis result,ahuge literaturehas been developedto

its explanation, exposition and generalization. A comprehensive survey of this topic

can be found in [6]. We may normalize the outer ellipse D asthe unit circle @D via

some aÆne transformationand the inner ellipse C istransformed into one inD with

then-Ponceletproperty. More precisely,forn3,wesaythatacurve inD has the

n-Poncelet propertyif for every point  on@D there isann-gon which circumscribes

about ,inscribesin@D andhas  asavertex. Itisnaturaltoask whetherthere are

curves other than ellipses in D which also have the n-Poncelet property. The next

theorem provides more examples.

Theorem5.1. Forany matrixAinS

n

andpoint on@D, thereisaunique

(n+1)-gonwhich circumscribesabout @W(A),inscribes in @D andhas as avertex. Infact,

such(n+1)-gonsP arein one-to-onecorrespondencewith(unitary-equivalence

class-es of)unitary dilationsU of Aonan (n+1)-dimensionalspace,underwhichthen+1

vertices of P are exactly the eigenvalues of the corresponding U.

This theoremappearedin[21, Theorem1]and[9,Theorem2.1]. The easypartof

theproofistoshowthatevery(n+1)-dimensionalunitarydilationofamatrixAinS

n

has distincteigenvalueswhichforman(n+1)-goninscribed in@D andcircumscribed

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details, we resort tothe matrix representations (1)and (2) forA togive the speci c

(n+1)-dimensionalunitary dilationsU. If A isrepresented as in(1), then U can be

taken as[b ij ] n+1 i;j=1 , where (3) b ij = 8 > > > > > > < > > > > > > : a ij if 1i;j n; [ Q j 1 k=1 ( a k )](1 ja j j 2 ) 1=2 if i=n+1 and 1j n; [ Q n k=i+1 ( a k )](1 ja i j 2 ) 1=2 if j =n+1 and 1in;  Q n k=1 ( a k ) if i=j =n+1;

for some  in @D. Here  acts as a parameter for the unitary dilations U. On the

other hand, if A isas (2), then U can be

(4) 2 4 f 1  f n 1 f n g 0  0 a kf n k 3 5 ; where jj=1;a=(1 kf n k 2 ) 1=2 >0 and g = 8 < : (a=kf n k)f n if f n 6=0;

any unit vector orthogonal to f

1 ; ;f n 1 if f n =0:

Both (3)and (4) can be used to prove that the (n+1)-gonswith vertices the

eigen-values of U coverall pointsof @D (the latteris in[9, Theorem 2.1]).

Theorem 5.1 yields additional properties for the numerical ranges of matrices in

S

n .

Corollary 5.2. Let A be a matrix in S

n

. Then

(a) W(A) is contained in no m-gon inscribed in @D for mn,

(b) w(A)>cos(=n),

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Here (a) is an easy consequence of the (n+1)-Poncelet property of @W(A), (b)

followsfrom(a),(c)isaconsequenceof,besidesthePonceletproperty,theinterlacing

of theeigenvalues ofRe A andRe U for (n+1)-dimensionalunitarydilationU of A,

and nally(d) follows from(c) by way of Kippenhahn's result. All assertions except

(d) are in [9].

If A is in S

n

, so is e i

A for any real . Hence the eigenvalues of Re (e i

A) are

all distinct by Corollary 5.2 (c). The curves

j ;j = 1;;n, described by j () = (x j ();y j ()) with x j () =  j ()cos  0 j ()sin; y j () =  j ()sin+ 0 j ()cos; where  j

() isthe jthlargest eigenvalue of Re(e i

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