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<titex><![CDATA[Zeroes of zeta functions and symmetry]]></titex>
<tihtml><![CDATA[Zeroes of zeta functions and symmetry
]]></tihtml>
<tiunicode><![CDATA[Zeroes of zeta functions and symmetry]]></tiunicode>
<tinomath>Zeroes of zeta functions and symmetry </tinomath>
<resauthor><![CDATA[Nicholas M. Katz]]></resauthor>
<author>
<autex>
<fntex><![CDATA[Nicholas]]></fntex>
<mntex><![CDATA[M.]]></mntex>
<lntex><![CDATA[Katz]]></lntex>
</autex>
<auhtml>
<fnhtml><![CDATA[Nicholas]]></fnhtml>
<mnhtml><![CDATA[M.]]></mnhtml>
<lnhtml><![CDATA[Katz]]></lnhtml>
</auhtml>
<auunicode>
<fnuni><![CDATA[Nicholas]]></fnuni>
<mnuni><![CDATA[M.]]></mnuni>
<lnuni><![CDATA[Katz]]></lnuni>
</auunicode>
<auascii>
<fnascii>Nicholas</fnascii>
<mnascii>M.</mnascii>
<lnascii>Katz</lnascii>
</auascii>
<email>nmk@math.princeton.edu</email>
<afftex><![CDATA[Department of Mathematics, Princeton University, Fine Hall, Washington Road, Princeton, New Jersey 08544]]></afftex>
<affhtml><![CDATA[Department of Mathematics, Princeton University, Fine Hall, Washington Road, Princeton, New Jersey 08544]]></affhtml>
<affunicode><![CDATA[Department of Mathematics, Princeton University, Fine Hall, Washington Road, Princeton, New Jersey 08544]]></affunicode>
<currafftex><![CDATA[]]></currafftex><curraffhtml></curraffhtml>
<curraffunicode><![CDATA[]]></curraffunicode>
<curremail><![CDATA[]]></curremail>
<urladdr></urladdr>
</author>
<author>
<autex>
<fntex><![CDATA[Peter]]></fntex>
<mntex><![CDATA[]]></mntex>
<lntex><![CDATA[Sarnak]]></lntex>
</autex>
<auhtml>
<fnhtml><![CDATA[Peter]]></fnhtml>
<mnhtml><![CDATA[]]></mnhtml>
<lnhtml><![CDATA[Sarnak]]></lnhtml>
</auhtml>
<auunicode>
<fnuni><![CDATA[Peter]]></fnuni>
<mnuni><![CDATA[]]></mnuni>
<lnuni><![CDATA[Sarnak]]></lnuni>
</auunicode>
<auascii>
<fnascii>Peter</fnascii>
<mnascii></mnascii>
<lnascii>Sarnak</lnascii>
</auascii>
<email>sarnak@math.princeton.edu</email>
<afftex><![CDATA[Department of Mathematics, Princeton University, Fine Hall, Washington Road, Princeton, New Jersey 08544]]></afftex>
<affhtml><![CDATA[Department of Mathematics, Princeton University, Fine Hall, Washington Road, Princeton, New Jersey 08544]]></affhtml>
<affunicode><![CDATA[Department of Mathematics, Princeton University, Fine Hall, Washington Road, Princeton, New Jersey 08544]]></affunicode>
<currafftex><![CDATA[]]></currafftex><curraffhtml></curraffhtml>
<curraffunicode><![CDATA[]]></curraffunicode>
<curremail><![CDATA[]]></curremail>
<urladdr></urladdr>
</author>

<cn>Katz_Nicholas M | Sarnak_Peter</cn>
<abstract>
<abstex><![CDATA[ Hilbert and Polya suggested that there might be a natural spectral interpretation of the zeroes of the Riemann Zeta function.  While at the time there was little evidence for this, today the evidence is quite convincing.  Firstly, there are the ``function field'' analogues, that is zeta functions of curves over finite fields and their generalizations.  For these a spectral interpretation for their zeroes exists in terms of eigenvalues of Frobenius on cohomology.  Secondly, the developments, both theoretical and numerical, on the local spacing distributions between the high zeroes of the zeta function and its generalizations give striking evidence for such a spectral connection. Moreover, the low-lying zeroes of various families of zeta functions follow laws for the eigenvalue distributions of members of the classical groups.  In this paper we review these developments.  In order to present the material fluently, we do not proceed in chronological order of discovery.  Also, in concentrating entirely on the subject matter of the title, we are ignoring the standard body of important work that has been done on the zeta function and $L$-functions.]]></abstex>
<abshtml><![CDATA[Hilbert and Polya suggested that there might be a natural spectral
interpretation of the zeroes of the Riemann Zeta function.  While at the
time there was little evidence for this, today the evidence is quite
convincing.  Firstly, there are the ``function field'' analogues, that
is zeta functions of curves over finite fields and their
generalizations.  For these a spectral interpretation for their zeroes
exists in terms of eigenvalues of Frobenius on cohomology.  Secondly,
the developments, both theoretical and numerical, on the local spacing
distributions between the high zeroes of the zeta function and its
generalizations give striking evidence for such a spectral connection.
Moreover, the low-lying zeroes of various families of zeta functions
follow laws for the eigenvalue distributions of members of the classical
groups.  In this paper we review these developments.  In order to
present the material fluently, we do not proceed in chronological order
of discovery.  Also, in concentrating entirely on the subject matter of
the title, we are ignoring the standard body of important work that has
been done on the zeta function and <IMG  ALIGN=BOTTOM ALT="$L$" SRC="/bull/1999-36-01/S0273-0979-99-00766-1/gif-abstract/img22.gif" HEIGHT=14 WIDTH=12>-functions.
<P>
]]></abshtml>
<absascii>Hilbert and Polya suggested that there might be a natural spectral
interpretation of the zeroes of the Riemann Zeta function. While at the
time there was little evidence for this, today the evidence is quite
convincing. Firstly, there are the function field'' analogues, that
is zeta functions of curves over finite fields and their
generalizations. For these a spectral interpretation for their zeroes
exists in terms of eigenvalues of Frobenius on cohomology. Secondly,
the developments, both theoretical and numerical, on the local spacing
distributions between the high zeroes of the zeta function and its
generalizations give striking evidence for such a spectral connection.
Moreover, the low-lying zeroes of various families of zeta functions
follow laws for the eigenvalue distributions of members of the classical
groups. In this paper we review these developments. In order to
present the material fluently, we do not proceed in chronological order
of discovery. Also, in concentrating entirely on the subject matter of
the title, we are ignoring the standard body of important work that has
been done on the zeta function and -functions.</absascii>
</abstract>

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Zeta Function,'' <i>Proc. Sym. Pure Math.</i>, <b>24</b>, <i>AMS</i>,
181-193, (1973). <A HREF="http://www.ams.org/mathscinet-getitem?mr=49:2590">MR <STRONG>49:2590</STRONG></A>
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<DT><A NAME=OD><STRONG>[OD]</STRONG></A><DD> A. Odlyzko, ``The <IMG  ALIGN=BOTTOM  ALT="$10^{20}$" SRC="/bull/1999-36-01/S0273-0979-99-00766-1/gif-references/img901.gif" HEIGHT=16 WIDTH=33>-th Zero of the Riemann Zeta
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<DT><A NAME=O2dS><STRONG>[O-S]</STRONG></A><DD> A. Ozluk, C. Snyder, ``Small Zeroes of Quadratic
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a Geometric Analogue,'' Seminar Bourbaki, Fev, (1966, Exp. 306). CMP <STRONG>98:09</STRONG>
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 A. Weil, ``Sur les Functions Algebriques &agrave; corps de Constantes
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(preprint), (1996). 
</DL><BR>
]]></refhtml>
<copyrightyr>1999</copyrightyr>
<copyrtholder>American Mathematical Society</copyrtholder>
<series></series>
<journal>Bulletin of the American Mathematical Society</journal>
<jnl>Bull. Amer. Math. Soc.</jnl>
<publjnl>bull</publjnl>
<volume>36</volume>
<issue1>01</issue1>
<issue2></issue2>
<pubdate>19990101</pubdate>
<received>October 15, 1997, and in revised form August 28, 1998</received>
<revised></revised>
<postdate></postdate>
<thanks><![CDATA[Research partially  supported by NSF grants DMS 9506412 and DMS 9401571.]]></thanks>

<thankshtml><![CDATA[Research partially  supported by NSF grants DMS 9506412 and DMS 9401571.]]></thankshtml>

<dedicate><![CDATA[]]></dedicate>
<dedicatehtml><![CDATA[]]></dedicatehtml>
<commby><![CDATA[]]></commby>
<commbyhtml><![CDATA[]]></commbyhtml>
<keyword></keyword>
<fpage>1</fpage>
<dpage>1-26</dpage>
<pgcount>26</pgcount>
<pii>S0273-0979-99-00766-1</pii>
<doi>10.1090/S0273-0979-99-00766-1</doi>
<issnp>0273-0979</issnp>
<issne>1088-9485</issne>
<seealso></seealso>
<language>English</language>
<doctype></doctype>
<msc>11G 11M 11R 11Y</msc>
<mscsec>60B 81Q</mscsec>
<msctype>1991</msctype>
<vno></vno>
<mr></mr>
<hline></hline>
<ftlink>http://www.ams.org/jourcgi/jour-getitem?pii=S0273-0979-99-00766-1</ftlink>
<sequence></sequence>
<erratum></erratum>
<corrigendum></corrigendum>
<addendum></addendum>
<supplement></supplement>
<comments></comments>
<corrections></corrections>
<misc><misclabel></misclabel><miscurl></miscurl><misctext></misctext></misc>
<origpub></origpub>
<origarticle></origarticle>
<doctext>
The Montgomery-Odlyzko Law 
We begin with the Riemann Zeta function and some phenomenology
associated with it.
 equation 
( s ) , , n 1 ; n -s , , p ;
( 1 - p -s ) -1 ,
 equation 
the product being over the primes, and it converges for Re (s) 1 . As
was shown by Riemann RI 
 ( s ) has a continuation
to the complex plane and satisfies a functional equation
 equation 
(s): -s 2 , (s 2) , ( s ) , , ( 1 - s );
 equation 
 (s) is entire except for simple poles at s 0 and 1 . We
write the zeroes of (s) as
 equation 
12 i .
 equation 
From (1) it is clear that Im () 1 2 . 
Hadamard and de la Vallee Poisson in their (independent) proofs of the
Prime Number Theorem established that Im () 1 2 . The
well known Riemann Hypothesis RH'' asserts that .
In what follows we are interested in finer questions about the
distribution of the zeroes. Let's assume RH (needless to say, in the
numerical experiments reported on below all zeroes found were 
on the line Re (s)
 12 ) and order the ordinates :
 equation 
 -1 , , 0 , , 
 1 , , 2 . 
 equation 
Then j , , - -j , j 1 , 2 , , 
and in fact 1 is rather large, being equal to 14.1347 . It is known (apparently already to Riemann) that
 equation 
 j : , 0 , j , , T T T 2 , as T .
 equation 
In particular, the mean spacing between the j s tends to
zero as j . In order to examine the (statistical)
law of the local spacings between these 
numbers we re-normalize (or unfold''
as it is sometimes called) as follows:
Set
 equation 
 j , , 
 j , , j 2 .8em for 
 .8em j , , 1.
 equation 
The consecutive spacings j are defined to be
 equation 
 j , , j 1 , - , j , , j , 
 , 1 , 2 , .
 equation 
More generally, the k - th consecutive spacings are
 equation 
 (k) j , , 
 j k , - j , , j , , 1 , 2 , .
 equation 
What laws (i.e. distributions), if any, do these numbers obey 
 figure bull766el-fig-1 
 Nearest neighbor spacings among 70 million zeroes beyond the 10 20 -th zero of zeta, verses 1 ( GUE ) . 
 figure 
During the years 1980-present, Odlyzko OD has made an extensive and
profound numerical study of the zeroes and in particular their local
spacings. He finds that they obey the laws for the (scaled) spacings
between the eigenvalues of a typical large unitary matrix. That is they
obey the laws of the Gaussian (or equivalently, Circular) Unitary Ensemble
GUE (see Section 2 for definitions). In Figure 1, the histogram of the
spacings j for 10 20 j 10 20 7.10 6 is
plotted against the GUE prediction ( 1 (GUE) - the Gaudin
distribution of Section 2). At the phenomenological level this is
perhaps the most striking discovery about zeta since Riemann. The big
questions, which we attempt to answer here, are, why is this so and what
does it tell us about the nature (e.g. spectral) of the zeroes Also,
what is the symmetry behind this GUE'' law 
Odlyzko's computations were inspired by the 1974 discovery of Montgomery
 MO2 that the pair correlation'' of the zeroes is, at least for a
restricted class of test functions, equal to the GUE pair correlation
 R 2 (GUE) (see Section 2). Precisely, he proves that for any ( ) for which the support of 
 ( ) 
 - , 
( x ) e -2 i x d x is contained in (
- 1 , 1) 
 equation 
 N ; 1N ;
 1 j k N ; ; ( j , -
 k ) , ,
 - ; ( x ) , r 2 ( GUE )(x) dx
 equation 
where
 equation 
r 2 ( GUE ) ( x ) , , 1 , - , ( x x ) 2.
 equation 
The significance of the interval (-1 , 1) is that 
 r 2 ( GUE ) ( ) 
changes its analytic character at 1 , and this signals
that for s whose support is outside -1 , 1 there
will be new non-diagonal'' (the main contribution to the limit in (9)
for restricted comes from the diagonal) terms contributing
to the main term. Montgomery conjectured that (9) holds without any
restrictions on the support of , and in GO-MO 
 he and Goldston
give an equivalence of this conjecture in terms of prime numbers. In
Figure 2 a comparison of (9) for s which are
characteristic functions of small intervals (i.e. the histogram) with R 2
( GUE ) is displayed.
 figure bull766el-fig-2 
 Pair correlation for zeros of zeta based on 8 10 6 zeros near the 10 20 -th zero, versus the GUE conjectured density 1 , - , ( 
 x x ) 2 . 
 figure 
One can look at triple and higher generalizations of the left hand side
of (9); see R-S . Indeed, the knowledge of the n -level
correlations for all n determines all the local spacing laws (see
 K-S1 ) and in particular the k -th consecutive spacings. In HE ,
Hejhal, using Montgomery's method, established that the triple
correlation is the GUE triple correlation as determined by Dyson DY .
Rudnick and Sarnak R-S by a somewhat different method (which in fact
does not appeal to RH) establish that all the n 2 correlations
are as predicted by GUE. All of these results are restricted as in
(9); that is they are proven only for test functions whose Fourier
Transforms are restricted so that only the diagonal'' terms are
responsible for the main term. A heuristic derivation of the n -level
correlations without any restrictions on the Fourier Transform has been
given by Bogomolny and Keating B-K . The calculations of the
correlations above are based on the explicit formula'' (see R-S ) 
which allows one to express the correlations in terms of multiple
sums over primes. The combinatorics which take one from these sums over
primes to the GUE n -level correlations are fascinating but hardly
illuminating in connection with gaining any deeper insight relating the
zeroes and GUE. 
The Riemann Zeta Function is but the first of a zoo of zeta and
 L -functions for which we can ask similar questions. There are the
Dirichlet L -functions L ( s , ) defined as follows: q 1 
is an integer, 
 : ( q ) 
a (primitive) character and we extend to by making
it periodic, and ( m ) 0 if (m , q ) 1 . Then 
 equation 
L ( s , ) , , n 1 ,
( n ) n -s , , p , ( 1 - ( p ) p -s 
) -1 .
 equation 
The analogue of (2) is known:
 equation 
( s , ) : -s 2 , , 
( s a 2 ) , L ( s , ) , , q s-
12 
 , ( 1 - s , ) (11 ) 
 equation 
where a 0 if ( - 1 ) 1 and is 1 if ( - 1 ) -
1 , while 1 
and is in fact a unitarized Gauss sum. q is
called the conductor of . The proof of (11 ) is the
same as for zeta and is based on Poisson summation DA . 
More generally by the
work of Godement and Jacquet JA if f is an automorphic
 cusp form on GL m , m 1 , its (standard)
 L -function L ( s , f ) is entire (if f is not the trivial
representation on GL 1 ) and satisfies a functional equation similar to
(2) (with an appropriate conductor and -factor). Such an
 L -function, L ( s , f ) , is given by an Euler product of degree m :
 equation 
L ( s , f ) , , p , L ( s , f p )
 equation 
where
 equation 
L ( s , f p ) , , m j 1 ,
( 1 - j , f ( p ) , p -s ) -1 .
 equation 
The j , f ( p ) s are eigenvalues of local (at p )
Hecke algebra's acting on f . In all these cases L (s , f ) is
expected to satisfy RH; that is its non-trivial
 zeroes are on the line Re (s)
 1 2 . General Conjectures of Langlands LA assert that all
 L -functions are finite products of these standard (cuspidal)
 L -functions, L ( s , f ) .
A classical and concrete example of a form on GL 2 is f :
 equation 
( q ) : , q , n 1 , ( 1 - q n ) 24 , ,
 n 1 , ( n ) q n.
 equation 
With q e 2 i z , ( z ) is a holomorphic cusp form of
weight 12 for SL 2 ( ) . That is for z ,
the upper half plane, we have
 equation 
( a z b c z d ) , ,
(c z d ) 12 , (z) , 
 equation 
for all a , b , c , d , 
ad - bc , , 1. 
 figure b minipage .45 
 scale .90 bull766el-fig-3 
 2pc Nearest neighbor spacings distribution
for the Ramanujan L -function,
 N 138693 . 
 minipage 
 minipage .45 
 scale .90 bull766el-fig-4 
 2pc Nearest neighbor spacings distribution
for the L -function associated to
 Ey 2 y x 3-x,N 5374 . 
 minipage 
 figure 
Its L -function is 
 equation 
L ( s , ) , , n 1 ,
 ( n ) n 11 2 , n -s , , p ,
( 1 - ( p ) p 11 2 , p -s , , p -2s 
) -1 ,
 equation 
and it is entire and satisfies
 equation 
( s , ) , ,
(2 ) -s ,
( s , 11 2 ) ,
L ( s , ) , ,
( 1 - s , ) .
 equation 
Other basic examples in GL 2 are L ( s , E ) 
where E is an
elliptic curve SI1 . The prescription of the local (degree 2) factor
at each prime p is given in terms of an analysis of E over
 p (see SI1 ). A well known conjecture of Shimura and Taniyama,
first formulated precisely in Weil WE1 , asserts that 
 L ( s , E ) L ( s , f ) where f is a holomorphic cusp form of weight 2
for 0 (N) where N is the conductor of 
 E (see SI1 ). Here
 ( 
 0 ( N ) 
 array c
 a b c d 
 array 
 , 
SL 2 ( ) : N c ) and f ( z ) 
satisfies:
 equation 
f ( z ) , , ( cz d ) 2 f ( z ) , : ,
 0 , ( N ).
 equation 
The results of Rudnick and Sarnak R-S were carried out in the general
context of f being an automorphic cusp form for GL m . 
They show that
the n 2 correlations of the zeroes of L ( s , f ) (again in
restricted ranges) are universally the GUE ones Numerical
experimentation by Rumely RUM for Dirichlet L -functions and by
Rubinstein RUB 
 for a variety of GL 2 forms f strongly confirm
this universality (so in particular confirm that no restrictions on the
test functions are needed). 
For example, the consecutive spacings for the zeroes
of L ( s , ) versus 1 (GUE) are given in Figure 3 
and similarly for an L ( s , E ) in Figure 4.
We call this phenomenon - that the high zeroes of any fixed L ( s , f ) ,
 f a cusp form on GL m obey GUE spacing laws - the 
 Montgomery-Odlyzko Law''. 
 Random matrix models 
In the 50's (see WI ) Wigner suggested that the resonance lines of a
heavy nucleus (their determination by analytic means being intractable)
might be modeled by the spectrum of a large random matrix. To this end
he considered various ensembles (i.e. probability distributions) on spaces
of matrices: in particular, the Gaussian Orthogonal Ensemble, GOE', and
Gaussian Unitary Ensemble, GUE'. These live on the linear space of real
symmetric (resp. hermitian) N N matrices and are orthogonal
(resp. unitary) invariant ensembles. He raised the question of the
local (scaled) spacing distributions between the eigenvalues of typical
members of these ensembles as N . The answer was
provided by Gaudin GA and Gaudin-Mehta G-M , who make
ingenious
use of orthogonal polynomials. This technique is a key tool in the
derivation of the results below. Later Dyson DY introduced his three
closely related circular ensembles: COE, CUE, as well as CSE with it's
associated Gaussian Symplectic Ensemble, GSE'. These circular
ensembles may be realized as the compact Riemannian symmetric spaces
(with their volume form as probability measure) U ( N ) O ( N ) , U
( N ) and U ( 2N) USp ( 2 N) , respectively. He investigated the
local spacing statistics for the eigenvalues of the matrices in these
ensembles (in their standard realization, see Table 1 below) as N
 . He shows that these statistics agree with the
corresponding matrices from the GOE, GUE and GSE ensembles.
Now the above are but 3 of the 11 classical compact irreducible
symmetric spaces (we ignore the center U ( 1 ) of U ( N ) which in
the limit N plays no role) of Cartan (see HEL ).
That some of these other matrix models are of importance in the theory
of L -functions will become clear below. 
Apparently there are also some
physical problems which require some of the other symmetric spaces
 A-Z . We list 6 of the 11 symmetry types: 
For our purposes of symmetry associated with L -functions, only the
first 4 ensembles in Table 1 will play a role. These 4 are the
classical compact groups which with a bi-invariant metric yield the so-called
type II symmetric spaces (see HEL ). The invariant volume form on
 G(N) is just Haar measure.
 2 
 3pt 
 table h 
 tabular l l 
1 c Symmetry Type G 
1 c Realization of G(N) as Matrices 
 U U(N) , the compact group of 
 N N unitary matrices. 
 SO (even) SO(2N) , the compact group of 
 2N 2N unitary( ) matrices preserving 
 the orthogonal form I , i.e. unitary matrices A satisfying A t A I .
 SO (odd) SO ( 2 N 1 ) and as above. 
 Sp U Sp ( 2 N ) , the compact group of 2N 2N unitary
matrices A satisfying 
 A t JA J , ( J 
 array r
 0 I N 
 -I N 0 
 array 
 . ) 
COE U ( N ) O ( N ) , symmetric unitary N N matrices 
identified with the 
 above cosets via B B t B . 
CSE U (2N) USp(2N) , 2N 2N unitary matrices satisfying 
 J t H t J H 
 identified by B BJB tJ t . tabular 
 table 
The ensemble U ( N ) is Dyson's CUE. The non-compact dual
symmetric space of U ( N ) is GL N ( ) U ( N ) , which is
the space on which GUE lives. Similarly, the non-compact dual of U ( N
) O(N) is GL N ( ) O(N) , that is GOE, and of U(2N) USp(2N) 
is U (2N) USp(2N) (see HEL , whose notation we adopt),which is the
space for GSE.
Let G(N) be any one of the ensembles in Table 1 realized as unitary
matrices A G ( N ) . Let dA denote the invariant measure and
 e i 1 (A) , , e i 2 (A) , , e i N(A) 
the eigenvalues of A . We order these 
 equation 
0 1 ( A ) 2 ( A ) N ( A ) 2
.
 equation 
The local (scaled) spacing distributions between the eigenvalues of A 
are defined as follows:
 itemize 
the k -th consecutive spacings k ( A ) are a measure on 
0, ) 
 equation 
 k ( A ) , a , b , ,
 1 j N 
 2 , ( j k -
 j) , , a , b N. (19 ) 
 equation 
The scaling factor N 2 normalizes k ( A ) to have mean equal
to k .
The pair-correlation R 2 (A) measures the distribution between
all pairs of eigenvalues of A . For a , b a compact interval
 equation 
R 2(A) a,b , , j k , , 
 2 , ( j , - k ) , a , b N.
 equation 
Higher correlations may be defined similarly. 
 itemize 
The main question to be answered here is the behavior of these measures
as N . For G(N) any one of the type 
II symmetric
spaces above, Katz and Sarnak K-S1 establish the following:
 itemize 
Fix k 1 . There are measures k ( GUE ) such that for
any G ( N ) of type II
 equation 
 N , 
 G ( N ) : k ( A ) d A , ,
 k ( GUE ).
 equation 
A Law of Large Numbers which ensures that for a typical (in
measure) A G ( N ) , k ( A ) and R 2 (A) approach k
( GUE ) and R 2 ( GUE ) as N . Precisely
 equation 
 N , G(N) , D ( k ( A ) , k (
 GUE ) ) , dA , , 0
 equation 
where D ( 1 , 2) is the Kolomogorof-Smirnov distance between
 1 and 2 ; that is 
D ( 1 , 2 ) , ,
 1 ( I ) , - 2 ( I ) , , : I 
 an interval .
 itemize 
For a , b (compact)
 equation 
 N , G ( N ) , R 2 ( A ) , a , b
 , - R 2 ( GUE ) a,b , , dA 0
 equation 
where
R 2 ( GUE ) a , b , , b a , r 2 ( GUE ) ( x ) dx
and r 2 ( GUE ) is given in (10).
Given that the answer is universal for type II symmetric spaces, and since
CUE is of this type and as pointed out above CUE and GUE have the same
local spacing statistics, it follows that type II local spacings are GUE
(as indicated by the notation in (21) and (22)). 
Gaudin in the original paper GA 
expressed the measures k ( GUE ) in terms of a Fredholm determinant:
 equation 
d k ( GUE ) , ,
 d 2 ds 2 , (
 k j 0 , k-j j , ( T 
) j , ( I T K ( s ) ) T 1 ) ,
ds
 equation 
where K(s) is the trace class operator on L 2 -s 2, s 2 whose
kernel is 
 equation 
K ( x , y ) , , ( x - y ) ( x - y ) .
 equation 
He also noted that (23) allows one to compute k numerically.
Indeed, the eigenfunctions of the integral equation
 equation 
 s 2 -s 2 , K ( x , y ) , f ( y ) , dy , , f ( x
)
 equation 
are prolate-spheroidal functions MEH . One may use this to compute the
eigenvalues j ( s ) and eigenfunctions f j ( x , s ) of
(26) and from it the densities of the measures k (GUE).
The density of 1 (GUE) is the solid curve in Figure 1. Notice that
the density vanishes to second order at s 0 , which says that the
eigenvalues of a typical A in a large G(N) tend to repel'' each
other. For the ensembles COE and CSE the analogous measures k (COE) and
 k (CSE) have been determined (see Mehta MEH ); they are
quite different from k (GUE) as well as from each other.
While the above results show that the local spacings between all the
eigenvalues of a typical A in any G(N) of type II are universally
GUE as N , the distribution of the eigenvalue
nearest to 1 is sensitive to the particular symmetry G . For k 1 , let k (G(N)) be the measure on 0,) which gives the
distribution of the k -th eigenvalue of A , as A varies over G(N) .
That is
 equation 
 k (G(N)) a,b , , Haar , A G ( N ) ,
 k ( A ) N 2 , a , b . equation 
Similarly one forms the 1-level scaling density (or more generally
 n -level densities) of eigenvalues of A near 1. For such an A G
( N ) and a , b , let 
 equation 
( A ) a, b , , 
( A ) 
 e i (A) is an eigenvalue 
 of A and ( ( A ) N) 2 , , a, b 
 .
 equation 
 figure scale .90 bull766el-fig-5 
 figure 
The average of ( A ) is denoted by W ; that is
 equation 
W(G(N)) , , G ( N ) , ( A ) , d A.
 equation 
In K-S1 it is shown that there are measures k ( G ) on 0
, ) which depend on the symmetry G such that 
 equation 
 N , k ( G (N)) , , k ( G ).
 equation 
For the densities we have
 equation 
 N , W ( G ( N ) ) , a , b , ,
 b a , w ( G ) ( x ) , d x
 equation where
 equation 
w(G) (x) , ; 
 array ll 
1 if G , , U or SU 
1 - , 2 x 2 x if G Sp 
1 , 2 x 2 x if G SO , ( even )
 0 1 - , 2 x 2 x if G SO , (
 odd ).
 array 
. 31' equation 
As with the measures k (GUE), the measures k ( G ) may be
expressed in terms of Fredholm determinants ( K-S1 ), and this
allows for their numerical calculation. The densities of 1 ( U ) ,
 1 (Sp) and 1 ( SO( even )) are displayed in Figure 5. 
Clearly, 1 (SO ( odd )) 0 , and it turns out that
 2 ( SO( odd )) 1 (Sp) . Note that Sp is unique in
having the density of 1 vanish (in fact to second order) at s 
0 . This shows that the eigenvalues of a typical A in a large 
 U S p ( 2 N) are repelled by 1 .
We end this section by remarking that the same questions for the most
reducible of the compact symmetric spaces, T N U ( 1 ) U ( 1 )
U ( 1 ) , have very different answers. Note that T N 
with the measure dx 1 2 , dx 2 2 , ,
 dx N 2 corresponds to choosing x 1 , x 2 , x N 
independently at random (or if we think of these as matrices, then we are
choosing a random diagonal matrix). The local spacing
statistics for these have been much studied in the probability literature. It
is well known FE that the local spacings for this model approximate a
Poisson process as N . The k -th consecutive
spacing measures converge to 
 k ( T ) s k-1 e -s , d s (k-1) 
(note that 1 has no repulsion at zero), while the
limiting pair correlation R 2 (T) is simply the density d x on .
 Function fields 
One can get much insight into the source of the Montgomery Odlyzko Law
by considering its function field analogue. Replace the field of
rational numbers by a field k which is a finite extension of the
field q (t) of rational functions in t with coefficients in
 q , the finite field of q elements. In analogy with the
Riemann Zeta Function, Artin AR introduced a zeta function (T,
k ) . It is defined by the product over all places v of k (see WE2 )
 equation 
( T , k ) , , v , ( 1 - T ( v ) ) -1 .
 equation 
One can also think of ( T , k ) as the zeta function of a
nonsingular curve C over q whose field of functions is k .
For example, let C q be a plane curve given by an equation
 equation 
f ( X 1 , X 2 , X 3 ) , , 0
 equation 
where f is nonsingular and homogeneous of some degree and has
coefficients in q . For each n 1 let N n be the
number of projective solutions to (33) in q n . The zeta
function of the field of functions k of C is the same as the zeta
function of the curve C over q which is defined as 
 equation 
( T , C q ) , , (
 n 1 ; N n T n n ).
 equation 
This geometric point of view is very powerful. For example, the
Riemann-Roch Theorem on the curve C plays the role of the Poisson
summation formula SCH and shows that
 equation 
( T , C q ) , , P( T , C q
) (1 - T ) , ( 1- q T) 
 equation 
where P T is of degree 2g , g being the
genus of the curve C . It also gives the functional equation P( T ) q g
T 2g P( 1 qT ) . The Riemann-Hypothesis
for these zeta functions, which was put forth and tested in many examples
by Artin, asserts that all the zeroes lie on T 1 . This
was proven by Weil. By now there are several different proofs: 
Weil WE3 , WE4 , elementary proofs by Stepanov ST and 
Bombieri BO , and
proofs by Deligne DE which have the advantage of applying much more
generally. One reason for being able to proceed in the function field
setting is that one has a spectral interpretation of the zeroes of ( T , C q ) . The number N n is the number of fixed points
of the n -th iterate of Frobenius (which is the operation of raising
the co-ordinates of q -points on C to the power q ).
Via a suitable Lefschetz trace formula this allows one to interpret the
zeroes of ( T , C q ) as the reciprocals of the
eigenvalues of Frobenius acting on the first cohomology group (with
 -adic coefficients) of the curve C .
Turning to the distribution of the zeroes of these zeta functions, we
write them as
 equation 
 j , , e i j , , j , , 1 , 2, ,
2g.
 equation 
Now order the 's as in (19) and form the local spacing
measures as in (19 ). We denote by k ( C q ) 
the k -th consecutive spacing measure between its zeroes. For a fixed
 ( T , C q) there are 2 g ( C ) zeroes and so there
cannot be any spacing law. We therefore let the genus go to infinity.
However, this alone does not lead to a unique (or even the existence of
a)
limiting law. For example, consider the curves C f , f 1 given
in affine form by Y 2 X q - X over the field q , q 
p f , p 2 . Its genus is (q - 1) 2 , and as explained in 
 K-S1 the consecutive spacing measure 1 ( C f q ) 
converges to a point mass 0 at zero, as f .
In K-S1 we therefore consider the typical'' curve of large genus
over a large field q . We show that as q and g go to
infinity the local spacings between the zeroes follow the GUE model -
that is the Montgomery-Odlyzko Law is valid for these zetas. Precisely,
if g ( q ) denotes the (finite) set of isomorphism classes
of curves of genus g over q and k 1 , then 
 equation 
 g : 
 q ;
1
 g ( q) 
 C g ( q ) ; 
D ( k ( C 
 q ) , , k ( GUE )) , , 0.
 equation 
In particular, since D 0 we have that for any 0 and
 q and g large enough ( g depending on q )
 equation 
C g ( q ) , , D ( k ( C q ) , ,
 k ( GUE ) ) , , , 
 , . C g ( q ) ;
 equation 
that is to say the zeta functions of almost all curves C satisfy the
Montgomery-Odlyzko Law as q and g go to infinity.
There are three key ingredients that go into the proof of (37). The
first is the monodromy of the family g . For technical
reasons instead of the family of curves of genus g one considers the
family g , 3K of curves of genus g together with a basis
of sections of 3K , K being the canonical class of the curve. The
monodromy representation of 1 of g , 3K 
on H 1 of a given curve has image whose Zariski closure (this being
the monodromy of this family) is the full symplectic group Sp (2g) 
 K-S1 . That this monodromy is symplectic in the first place is a
consequence of it preserving the intersection pairing of cycles in the
first homology group of a curve. Via this representation one can
associate to each C g ( q ) 
a unitarized Frobenius conjugacy class 
 ( C q ) in U S p ( 2 g) 
such that 
 equation 
P( T , C q ) , , ( 1 - ; T ( C q ) ).
 equation 
The second ingredient is Deligne's main result DE which can be
used to show (see K-S1 ) that for any continuous class function f on
 USp (2g) 
 equation 
 q 
 C g ( q) 
 f ( ( C q )) 
 Aut ( C q ) 
 C g ( q ) 
1 Aut ( C q ) 
 U Sp(2g) ; f ( A ) , d A.
 equation 
The number of C g ( q ) for which Aut 
( C q ) 2 can be shown to be of lower order as q
 . Applying (40) with the continuous function f (
A ) D ( k ( A ), k ( GUE ) ) , together with the third
ingredient - the Law of Large Numbers (22) of Section 2 (applied with
 G ( N ) USp ( 2N )) - leads to (37).
One can prove similar results for other families of zeta or
 L -functions of curves or varieties V over finite fields; see K-S1 .
The universal Montgomery-Odlyzko Law is valid at least if the monodromy
of the family is big, that is, if it is (or is close to) any of the G ( N
) 's of type II in Table 1.
Thus in the function field, the source of the GUE phenomenon is clearly
identified. It is the monodromy (or symmetry group) of the family and
its scaling limit, combined with the universality of the spacing
statistics for the type II symmetric spaces. The latter washes out the
fine structure to the extent of not even betraying the specific symmetry
type of the family. As was mentioned in Section 2 the measures k 
are more sensitive, and we exploit this next. 
 Families and low lying zeroes 
The following table summarizes some known analogies between zeta
functions over and function fields.
 2 
 1pt 
 table h 
 tabular l l l l 
 1 c A 
 1 c B 1 Type of Number Field Function Field 
 Zeta Function ( s ) , L ( s , ) , L ( s , f ) 
 ( T, C q ) , ( T , V q ) , V a variety. 
2 Analytic Continuation Established via Poisson Established using
Riemann-Roch 
 and Functional Equation Summation or Automorphic and in general
Etale Cohomology. 
 Properties of f . 
3 Spectral Interpretation Known via the Action of Frobenius 
 of Zeroes on Cohomology. 
4 RH Expected Proven, Weil, Deligne. 
5 Montgomery-Odlyzko Law Expected Valid for almost all curves. 
 for Local Spacings 
 between Zeroes 
6 Monodromy (or Symmetry) Known via the representation 
 for Families and of 1 of the Family 
 Equi-distribution on Cohomology Groups. tabular 
 table 
We view the entry 5-A and the evidence towards it described in Sections
1 and 3 as strongly suggesting an entry of expected'' in 3-A. An interesting possibility for a 
spectral interpretation of the zeroes
has been suggested by Connes CO . Also
worth noting is that Deligne's first proof of 4-B is based on monodromy
for a family. For example, to establish RH for ( T , V ) , V a
smooth hyper-surface in N , he proceeds by putting V in a
family V t (for an exposition see KA1 ). RH is established for all
 V t 's at once by exploiting the monodromy of the family which glues
the V t 's together. Thus, a positive entry in 6-A is most desirable.
This is the topic of this section.
We begin with the function field where the notion of a family has a
precise meaning. Consider the set of all quadratic extensions of k 
 q ( t ) . We may realize these as follows:
Let H n ( q) be the set of all monic square-free polynomials
of degree n with coefficients in q . The quadratic
extensions are k k ( ) with H n (
 q ) . For each n , these function fields correspond to hyper-elliptic
curves, Y 2 ( X ) , H n and form
a family of curves. The genus g g ( n ) of k satisfies n
 2g 2 if n is even and n 2g 1 if n is odd. Thus ( T ,
k ) , which may be written as L ( T , ) ( 1 - T )
( 1 - q T ) with the corresponding quadratic character,
has 2g ( n ) zeroes with angles 1 ( ) , 2 (
) , , 2g ( ) which we normalize and order
as in (36) and (19). For j 1 fixed we examine the distribution
of j ( ) as varies over 
 H n ( q) , n
 . This amounts to studying the distribution of the
zeroes near the central point. Using the equi-distribution techniques
described in Section 3 together with the scaling limits (30) for
 USp (2g) (the monodromy of this hyper-elliptic family again being the
full Sp (2g) ), one shows (see K-S1 ) that for f C 0 ( 0 ) a test function
 equation 
 n :
 q :
1 H n ( q ) ;
 H n ( q ) ;
f (
 j ( ) 2 g 2 ) 
 0 :
f ( x ) , d j ( Sp ) ( x ).
 equation 
We conjecture (though the techniques leading to (41) offer nothing in
the way of a proof) that (41) holds without taking the inner q limit,
that is
 equation 
 n ;
1 H n ( q ) ;
 H n ( q) ;
f (
 j ( ) g 
) , ,
 0 ;
f ( x ) d j ( Sp ) ( x ).
 equation 
Equations (41) and (42) assert that the distributions of the zeroes near T 1 
 (the central or symmetry point) of the quadratic extensions
 k of k q ( t ) follow the symplectic scaling limit
laws.
We give a second example in the function field of a family for which the
distribution of the zeroes near the central point is dictated by, and in
turn reveals, the symmetry group of the family. Let E k be an
elliptic curve with non-constant j -invariant ( SI1 ). For each place
 v of k (that is each irreducible polynomial p ( t ) q
 t or the place at infinity - degree'') the residue field k v is a
finite extension of q of degree d v . Let E v be the curve
 E k v . At a place at which E has good reduction, write
 equation 
 E v , , k v , , 1 , - v , - v .8em 
 with .8em v v , , k v .
 equation 
The L -function of E k is defined to be 
 equation 
L ( T , E ) , , v ,
( 1 - v , T d v ) -1 , 
( 1 - v , T d v ) -1 
 equation 
(for the places v of k at which E does not have good reduction,
the local factor is described in SI1 ). L ( T , E ) satisfies a
functional equation and Riemann Hypothesis TA , DE .
For example, consider the Legendre curve 
 equation 
E: Y 2 , , X ( X - t ) (X-1).
 equation 
For n ( q ) , the set of H n (
 q ) with no zeroes in 0 , 1 , the twist of E by
 has L -function
 equation 
L ( T , E ) , ,
 v , (
1 - v , ( v ) , T d v ) -1 ,
(
1 - v , ( v ) , T d v ) -1 ,
 equation 
and its degree is N where N is 2n if n is even and 2n-1 if n 
is odd. The zeroes of L( T , E ) are of modulus
 1 q , and we write them as q -1 e i 1 , : q -1 e i
 2 , , q -1 e i N with 
 equation 
0 1 ( E ) 2 ( E D ) , , , N ( E ) , ,
2 .
 equation 
Denote by ( E D ) ( 1 ) the sign of the
functional equation. Each of the two values is shared roughly equally by the
 's in n ( q ) as n .
Let n , ( q) denote those n ( q) with equal to 1 and -1 
respectively. As with the last example one can (see KA2 ) compute the
monodromy of this family L ( T , E ) , n ( q ) .
It is equal to O(N) . The reason for this difference between the families 
 L (s, ) and L (s, E ) is that the
Frobenius acts on H 1 of a curve with coefficients which are
orthogonally self dual in the first case and symplectically self dual in
the second. By standard properties of cup-product, the autoduality on
such H 1 is reversed. 
As above, the equi-distribution techniques
together with (30) with G O lead to: 
Fix j 1 and f C 0 ( 0 ) ;
then (see K-S1 )
 equation 
 n ,
 q ;
1 n ( q) ; 
 n ( q ) ;
f ( 
 N j ( E ) 2 ) , ,
 0 ; f ( x) d j ,
( SO ( even ))( x )
 equation 
and
 equation 
 n , q ;
1 n - ( q ) ;
 - n ( q ) ;
f , (
 N j ( E ) 2 ) , ,
 0 ,
f ( x ) d j ( SO ( odd ))(x).
 equation 
So this is a family with an orthogonal symmetry and a corresponding
distribution of zeroes near the central point. As in the first example
we conjecture that (48) and (49) hold without the inner q limit - that
is they hold for a fixed q .
In principle in this function field setting, as long as one can compute
the monodromy of the family and its scaling limits, as is done in the
above examples, one obtains the scaled spacing distribution of zeroes
near the central point.
We turn to the rational number setting. The analogues of the two families
considered above are clear enough. The first consists of the Dirichlet
 L -functions L ( s , ) with 2 1 . The second of L ( s ,
E ) where E is an elliptic curve and a
quadratic character as in the first family. The corresponding question
concerns the distribution of the zeroes near s 1 2 (we always
normalize the L -functions to have functional equation s 1
- s so that 1 2 is the central point) of these L -functions. We
will examine a number of different families . To each
automorphic form f let c f be its conductor (see the
line above (12)). Assume further that the sets X 
f c f X are finite and that the
asymptotics X , as X goes to infinity, can
be determined. Write the nontrivial zeroes of L ( s , f ) as 
 equation 
12 , , i f,
 equation 
and assuming RH order these
 equation 
 f (-2) , , (-1) f , ,
0 , , (1) f , , (2) f , .
 equation 
For j 1 consider the distribution of the numbers 
 equation 
 (j) f , c f 2 
 equation 
as f varies over X , X .
That is, we study the distribution of the j -th lowest zero (that the
normalization (52) is appropriate will become clear from the results
below). Form the analogues of the measures k (see (27)) and the
density and W ((28), (29))
 equation 
 j ( X , ) a , b , , 
f X ; 
 (j) f , c f 2 ; a , b 
 X .
 equation 
For ( ) a test function, set
 equation 
( f , ) , , f , ( f c f 2 )
 equation 
and 
 equation 
W ( X , , ) , ,
1 X , c f X , ( f
, ).
 equation 
One can also form several variable joint densities (see K-S1 ), and
these determine the j 's as well as all the local scaled distributions
of zeroes near s 1 2 . By analogy with the function field we might
expect that j ( X , ) and W ( X , 
, ) converge to j ( ) and -
 ( x ) w ( ) ( x ) d x , where j ( 
) and w ( ) correspond to the symmetry type G(
 ) ''. If the family has a function field
analogue, then G ( ) and the corresponding j (
 ), w ( ) can be predicted by the analysis
described in the two examples above. This idea has been carried 
out and tested analytically and numerically for various families, some 
of which are as follows (for the rest of this section we assume RH for
all L ( s , f ) 's):
 namelist xxxxx 
 I. The family of Dirichlet L -functions L ( s ,
) , (primitive) of conductor c , , q and 
quadratic (i.e. 2 1 ) . L ( s , ) is self-dual (that is its
functional equation is back into itself) and the sign is
equal to 1 for all .
 namelist xxxx 
 (a) The discussion of the function field analogue suggests that
 G ( ) Sp .
 (b) K-S2 (see also Ozluk-Snyder O-S )
W ( X , , ) -
 , ( x ) w (Sp ) ( x ) d x as X 
 figure t bull766el-fig-6 
 1 level density for L(s, d) ,
 10 12 d 10 12 , , 200000, 7243 d 's,
mean of 1st zero above 0 equals 0.8268, renormalized to have mean 0.78. 
 figure for any ( ) 
whose Fourier transform is supported
in (-2,2). The density 
 w ( S p ) ( x ) is given in (31 ). 
 (c) In his recent thesis RUB Rubinstein establishes that the 
 n 2 joint densities converge to the Sp densities (see K-S1 )
for test functions ( x 1 , , x n ) whose Fourier
transforms are supported in a small neighborhood of 0 .
 (d) Numerical experiments, Rubinstein RUB for q of size
 10 12 give an excellent fit of the j 's and W with the Sp 
predictions. For example, the density of zeroes (scaled) versus w(Sp) 
is given in Figure 6. The distribution of the lowest zero 
 1 ( X , ) for 
 q 10 12 is displayed in Figure 7. It is
compared with 1 (Sp) . Note that in the analysis I(b) above, the
convergence to the limit is at a speed of 1 q 
and moreover there is a
term of one sign which shifts the answer by this amount. While this
term disappears in the limit q , it does affect the
mean numerically, and the data displayed incorporates a re-normalization
taking this into account. According to the Sp predictions, the mean
value of q 2 should be the mean of
 1 (Sp) which is 0.7827.... The numerics confirm this though the
convergence is slow (like 1 log q ) and the approach is from above. 
 figure t bull766el-fig-7 
 1st zero above 0 for L ( s , d ) , 10 12 d 10 12 200000, 7243 d 's,
mean of 1st zero above 0 equals 0.8268, renormalized to have mean 0.7827. 
 figure 
 (e) The first person to compute numerically the zeroes of 
 L ( s , ) in this family appears to be Hazelgrave. He found that the
zeroes repel'' the point s 1 2 , and this is referred to as the
Hazelgrave phenomenon. One can carry out all of the above for L
( s , ) , 3 1 (or any other order bigger than 2). One
finds a unitary symmetry and the zeroes do not repel s 
1 2 . As remarked in 
Section 2 the density 1 (Sp) 
vanishes to second order at s 0 . Thus, the Hazelgrave
phenomenon is a manifestation of the symplectic symmetry 
 namelist 
 II. The family where is the weight
12-cusp form in (15) and runs over the quadratic characters. The
conductor c is q 2 and can be both 1 and -1 . L ( s , ) is self-dual.
 namelist xxxx 
 (a) 
From function field considerations we expect 
 G ( ) O 
with the refinement that the sub-family with 
 1 has an 
 SO (even) symmetry and - with -1 an
 SO (odd) symmetry.
 (b) K-S2 For this family or more generally with any GL 2 
cusp form f (with trivial central character) replacing , we
have 
W ( X , , ) -
 ( x ) w ( SO ( even ) ) ( x ) d x 
and 
 W ( X , - , ) -
 ( x ) w ( SO( odd )) ( x ) dx 
for any ( ) 
whose Fourier transform is
supported in (-1,1) . The densities w (SO) ( x ) 
are given in (31 ). 
The last applies in particular to L ( s , E ) 
with E an elliptic curve, which of course is consistent with the
function field example mentioned at the beginning of this section.
 (c) 
Rubinstein RUB has shown that the n 2 level densities converge
to the orthogonal densities for a ( x 1 , , x n ) with
 ( 1 , , n ) supported in a small
neighborhood of 0 .
 figure t bull766el-fig-8 
 1-level density for L (s, d even), 350000 d 650000, 11464 d 's,
mean of 1st zero above 0 equals 0.2926, renormalized to have mean 0.3214. 
 figure 
 (d) Numerical experiments (Rubinstein RUB ) for q of size
about 500,000 give an excellent fit with the orthogonal predictions. In
Figure 8, the density of 
 is plotted against w (SO( even )) ,
and in Figure 9 the density of - against w (
SO( odd )) (for the latter there is always a zero at 
 s 1 2 and a 
 0 in the
density; these are suppressed). In Figure 10, 
 1 ( ) is
displayed against 
 1 ( SO( even )) , and in Figure 11 
 2 ( - ) against 
 2 ( SO( odd )). 
 namelist 
 III. 
The family H(N) of holomorphic Hecke-eigen forms of weight 2 for 
 0 ( N ) (as in (18)). 
For simplicity we assume that N is prime. 
 L ( s , f ) has conductor c f N and is self-dual. As in the last
family approximately half of the f 's have f 1 , with the
remaining half having f -1 . Let H (N) and H - (N) 
denote the corresponding sets. We have that 
 ( H ( N)) ( H - (N)) N 24 as N .
 namelist xxxx 
 (a) The expected symmetry G ( ) is O , though as yet
we have not understood the function field analogue.
 (b) 
(See Iwaniec-Luo-Sarnak I-L-S ):
 figure h bull766el-fig-9 
 1-level density for L (s, d odd) 350000 d 650000, 11390 d 's,
mean of 1st zero above 0 equals 0.7186, renormalized to have mean 0.7827. 
 figure 
As N 
1 ( H (N)) ;
 f H (N) , ( , f ) ,
 - , ( x ) w (SO ( even )) ( x ) d
x
1 ( H - (N)) ;
 f H - ( N ) , ( , f ) , 
 - , ( x ) w (SO( odd )) ( x ) d x
for any ( ) 
with support ( - 2 , 2
) .
 namelist 
 figure t bull766el-fig-10 
 1st zero above 0 for L ( s , d 
even) 350000 d 650000, 11464 d 's,
mean of 1st zero above 0 equals 0.2926, renormalized to have mean 0.3214. 
 figure 
 figure b 
 bull766el-fig-11 
 1st zero above 0 for L (s, d odd)
 350000 d 650000, 11390 d 's, mean of 1st zero above 0 equals 0.7186, renormalized to have mean 0.7827. 
 figure 
 IV. 
The family of symmetric-square L -functions (see SH1 ) 
 L (s , sym 2 f) 
where f is a Hecke eigenform of even integral weight k on
 for SL 2 ( ) (as in (15) above). The
dimension of this space of cusp forms is 12 as k
 . The appropriate (analytic) analogue of the
conductor of 
 c sym 2 f of L(s , sym 2 f ) is k 2 . For this family
the averaging is over all such sym 2 f with c sym 2 f X .
 L ( s , sym 2 f ) is an Euler-product of degree three, and by a theorem
of Gelbart and Jacquet G-J these are L -functions of self-dual cusp
forms on GL 3 . The sign of the functional equation sym 2 f 
is equal to 1 .
 namelist xxxx 
 (a) Being self-dual forms on GL 3 we expect G ( ) 
Sp .
 (b) In I-L-S it is proven that 
W ( X , , ) -
 , ( x ) w ( Sp ) ( x ) dx
as X , for any ( ) 
with support ( - 43, 43) .
 namelist 
 namelist 
 remarks 
 enumerate 
All of these results confirm, to the extent that they apply, the
predictions of the G ( ) symmetry. We call the conjecture
that the sums W ( X , , ) converge to the claimed
density without any restrictions on , the Density
Conjecture for .
The proofs of the results about densities all proceed by
expressing ( f , ) via the explicit formula, in terms of sums
involving the Hecke eigenvalues of f . The method used for averaging
such quantities over f for the families III and IV
draws heavily on the tools developed in Iwaniec-Sarnak I-S (see also
Section 5).
With the exception of the family II, all of the results allow for
the support of to be larger than -1 , 1 . This is
rather significant since 
 w(Sp) ( ) , 
 w ( SO)( even ) ( ) and 
 w (SO)( odd ) () 
are all discontinuous at 
 1 . This signals that new non-diagonal terms enter as
main terms as soon as the support of is larger than 
 - 1 , 1 . Thus, what is shown here goes beyond anything that has been
established for the correlations of the high zeroes of 
 (s) , as discussed in Section 1. 
For the families III and IV these new terms
arise out of a far reaching analysis with Kloosterman sums 
(see also D-F-I for related analyses). 
That these fundamentally new
non-diagonal contributions yield precisely the conjectured 
 G ( ) answers is very pleasing evidence for this symmetry picture,
at least for these families.
Other families for which similar results have been derived are:
The family L ( s , f ) , f varying over holomorphic cusp forms of
weight k for SL 2 ( ) as k , with
symmetry G( ) O I-L-S . The family 
 L ( s , f D ) as in II above but where f is now any
fixed self-dual cusp form on GL m , whose symmetry is Sp or O 
according to whether L ( s , sym 2 f ) 
does or does not have a pole at s 1 K-S2 . 
The family L ( s , ) n 1 , n 3 .
These L -functions are not self-dual and the symmetry is U n - the
subgroup of the unitary group whose elements have their determinant an 
 n -th root of 1 KA3 . 
 enumerate 
 remarks 
 Applications 
The interest in the zeroes of L -functions lies in their fundamental
influence on arithmetical problems. In particular, the question of
vanishing of an L -function at a special point on the critical line
arises in the Birch and Swinnerton-Dyer Conjecture B-S (which for
certain f relates the vanishing of L ( s , f ) and its derivatives
to ranks of elliptic curves and abelian varieties (see below)), in the
Shimura correspondence SH2 and in spectral deformation theory (see
Phillips-Sarnak P-S ). The distribution of zeroes for a family L ( s
,f ) near s 1 2 as discussed in Section 4 has immediate
applications to vanishing at that point. By varying the test function
 in the Density Conjecture for any of the above families
 , one is led to (assuming the Density Conjecture):
 equation 
 X ; 
 f X f 1 , , L (
12, f ) , , 0 
 f X f 1 , , 1
 equation 
and
 equation 
 X ;
 f X f -1 , , L (
12 , f ) , , 0 
 f X f -1 ; , 1.
 equation 
The results of Section 4 are approximations to the Density Conjecture
and give corresponding approximations to (56) and (57). We illustrate
this in the cases of families II(b) and III.
Let E be an elliptic curve which is given in the form
 equation 
E: ; Y 2 X 3 A X B.
 equation 
The twist of E by a square free integer D is the curve
 equation 
E D: ; D Y 2 X 3 A X B.
 equation 
We assume that E is modular so that the L -function L ( s , E D) ,
which equals L ( s , E D ) , is also modular. The Birch
and Swinnerton-Dyer Conjecture assert that the order of vanishing of L
( s , E D) at s 1 2 is equal to the rank of the group of
 -rational points on E D . Kolyvagin K-L 
 has shown that if L (
12, E D) 0 , then rank (E D) 0 . This together with the
Density-Conjecture via (56) implies the following conjectures of Goldfeld
 GO :
 itemize 
The rank of E D is zero for 100 
 D X , 
 E D 1 , as X .
Assuming further the Birch and Swinnerton-Dyer Conjecture and
applying (57) show that the rank of E D is equal to one for 100 
the D 's with D X , 
 E D - 1 ,
as X . 
 itemize 
The approximation II(b) of Section 4 implies (assuming RH for the 
 L ( s , E D) 's) that rank ( E D) 0 for at least 25 
 E D 1 . This result is due to Brumer and Heath-Brown 
 B-HB . A challenging problem, which is as yet at the border of known
techniques (see P-P ), is to give an unconditional proof that rank
 E D 0 for a positive proportion of D X , as X . (For certain curves E such a result is known by
algebraic methods HB , WO ). We note that for this family L ( s ,
E D ) (as well as for some others below), unlike the case
of L ( s , D) discussed in II, there are many D ,
with E D 1 and L ( 12 , E D ) 0 . By choosing X and Y first and then D in
(59), Gouvea and Mazur GO-MA show that there are at least X 1 2 , D 's with D X D 1 and L (
12 , E D ) 0 , as X .
This certainly affects the numerics for the distribution of low-lying
zeroes for this family when X is of moderate size.
We turn to the family in III. By choosing 
 () , 
 ( 0 ) 1 , 0 , support 
 ( - 2 , 2 ) 
and for which 
 - , ( x ) 
 w ( , x ) d x is minimized (see I-L-S ),
we conclude from the
results in III (which we recall assume RH for 
 L ( s , f ) ) that for N prime and large enough
 equation 
 f H ( N ) L ( 12, f ) 0 
 H ( N ) , , 9 16 
 equation 
 equation 
 f H - ( N ) L ( 12, f ) 0 
 H - ( N ) ; , 15 16 
 equation 
and
 equation 
 H 2 ( N ) 2 , , ,
( H 2 ( N ) ) , , 
 f H 2 (N) ,
 ord , ( 12 , L ( s , f ) ) , ,
 99 100 ,
( H ( N ) )
 equation 
where ord ( s 0 , L ( s , f )) is the order of vanishing of L (
s , f ) at s s 0 . Note that H ( N ) 12 and
as Murty MU points out (and this does not assume RH) H ( N )
 H ( N ) 2 . Thus, the lower bound in (62) is clear.
Concerning the upper bound in (62), Brumer BR established such a
result with 99 100 replaced by 3 2. One can reduce this 3 2 to 1
without appealing to the off-diagonal'' analysis which leads to III.
However, to get anything below 1 in (62) already relies on the extended
ranges in III. A similar remark applies to (60), the off-diagonal
analysis allowing for the lower bound which exceeds 50 
significant as will become clear from what follows.
One can apply (60), (61) and (62) to estimate the rank of the Jacobian
 J 0 ( N ) of the curves X 0 (N) (which analytically is 0
( N ) ) by combining those results with known partial results
towards the Birch and Swinnerton-Dyer Conjectures (Kolyvagin K-L and
Gross-Zagier G-Z ). Let M 0 ( N ) be the quotient of J 0 (N) 
considered by Merel MER . It corresponds to those 
 f H (N) for
which 
 L ( 12, f ) 0 ,
and it is no doubt the largest
quotient of J 0 (N) of rank zero. It is of great interest to know its
size ( MA , MER ). Brumer BR 
 has computed these for N 10 4 , and
based on his findings, he conjectures that 
 equation 
 N : 
 M 0 ( N ) H (N) , , 1
 equation 
 equation 
 N : rank J 0 ( N ) J 0 ( N
) , , 12.
 equation 
Note that Density Conjectures for this family via (56) and (57) and 
 K-L and G-Z 
 imply these conjectures of Brumer. In the same way (60),(61)
imply (still assuming RH for L ( s , f ) ) that for N large
 equation 
M 0 ( N ) , , 9 16 , H (N)
 equation 
and 
 equation 
 rank J 0 ( N ) , , 15 32 , J 0 ( N ).
 equation 
Moreover, if one further assumes the Birch and Swinnerton-Dyer
Conjecture then (62) shows that for N large 
 equation 
 J 0 (N) 2 , , (N) , , rank J 0 (
N ) , , 99 100 , J 0 ( N ).
 equation 
It is remarkable that the results (65) and (66) can be established
unconditionally with almost as good quality. The techniques that achieve
this are quite different from and more sophisticated than those used to
establish the density results for the family III though both make use of
the methods for averaging over such a family, developed in I-S . 
In DU , Duke examines the averages of L ( 12, f) and L 2 (
12 , f ) over the set H(N) . 
This allows him to show that at least N (N) 2 of the L (
12, f ) 's are non-zero. Introducing mollifiers'' and other
tools into analysis of weighted averaging of L ( 12, f) and
 L 2 ( 12, f ) , Iwaniec and Sarnak I-S show that given
 0 0 there is an effective N 0 N 0 ( 0 ) such
that for N N 0 
 equation 
 f H ( N ) L ( 12, f ) , , ( N
) -2 
 f H ( N ) , , 12 , - 0.
 equation 
This unconditional result is rather close to the conditional (65) and
the 50 
 I-S that if (68) holds with any 
 c 12 replacing
 12 , then there are no Siegel zeroes (A Siegel zero is a zero
of a Dirichlet L -function L ( s , q ) , 2 q 1 which is
very close, in terms of q the conductor of , to 1.) The precise
result that c 12 would yield is that there is an effective
 c 0 such that 
 L ( 1 , q ) c (q ) -2 .
Using variations of the techniques above among many other ideas,
Kowalski and Michel K-M1 and independently VanderKam have shown
that for N large
 equation 
 rank J 0 ( N ) , , B , J 0 ( N )
 equation 
( K-M1 show that B 19 54 works while establishes the
result with B 1 100 ). 
In another work, Kowalski and Michel K-M2 
establish the upper bound in (62) unconditionally with 99 100 
replaced by 10. 
We conclude this section with a comment about more general families
 and the distribution of low-lying zeroes. While symmetry
alone appears to dictate the laws of this distribution for the families
discussed in Section 4, some caution must be exercised in general. For
example, consider the family of isogeny classes of all
elliptic curves E ordered by their conductors. Function field analogues
(as in example 2 of Section 4) suggest that the symmetry G (
 ) of this family is O . In particular (and this can be
proven for the function field with the usual caveat of letting q
 first), zero percent of the E 's in of
conductor at most N have rank at least two, as N .
However, numerical experimentation with moderate size N for this
family and some other
 families of elliptic curves K-Z , SI2 , B-M 
indicate that
this percentage is positive and even that it is not very small. It is
premature to say whether this is an artifact of a too restricted range
of computation and is due to effects like there being points of small
height on these curves (like the Gouvea-Mazur result GO-MA ),
 or whether the distribution of low-lying zeroes for such a
family does not follow the O -predictions. Understanding the source of
this excess rank'' for moderate N will no doubt reveal
some very interesting new features.
 Conclusion 
Phenomenologically, it is found that the distribution of the high zeroes
of any L -function follow the universal GUE Laws, while the
distribution of the low-lying zeroes of certain families follow the laws
dictated by symmetries associated with the family. The function field
analogues of these phenomena can be established, and the source of the
symmetry is the monodromy of the family and its scaling limits. Analytic
results concerning the distribution of high zeroes for an individual
 L -function and low zeroes of a family of L -functions, to the extent
to which these can be established, confirm these findings above. 
Whether in the case of L -functions (over ) there is indeed some
kind of underlying monodromy group which glues the family and is the
source of the symmetry is a fascinating question. Our belief is that
there is. One can imagine that to each L ( s , f ) , f , there is a natural interpretation of the zeroes of L ( s ,
f ) as the eigenvalues of an operator U ( f ) on some space H . As
 f varies over these U ( f ) 's become equi-distributed in
the space of such operators with a given symmetry type. For the families
discussed in Section 4 these symmetries are identified. In particular,
the Riemann Zeta function sits in Family I of Section 4 which has a
symplectic symmetry. We infer that in the proposed spectral
interpretation of the zeroes of the Riemann Zeta function, the operator
should preserve a symplectic form Apparently the cohomological
formalism of Denniger DEN accounts for the operator'' corresponding
 (s ) preserving a skew-symmetric form. 
We believe that the further
understanding of the source of such symmetries holds the key to finding
a natural spectral interpretation of the zeroes.

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