modular forms of weight one and stark heegner points
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Starks Conjecture and related topics p -adic iterated integrals , modular forms of weight one, and Stark-Heegner points. Henri Darmon San Diego, September 20-22, 2013 (Joint with Alan Lauder and Victor Rotger ) Starks conjectures


  1. Stark’s Conjecture and related topics p -adic iterated integrals , modular forms of weight one, and Stark-Heegner points. Henri Darmon San Diego, September 20-22, 2013

  2. (Joint with Alan Lauder and Victor Rotger )

  3. Stark’s conjectures Stark’s conjectures give complex analytic formulae for units in number fields (more precisely, for their logarithms ) in terms of leading terms of Artin L -functions at s = 0. Are there similar formulae for algebraic points on elliptic curves ? Heegner points, whose heights are related to L -series via the Gross-Zagier formula, are analogous to circular or elliptic units. We refer to conjectural extensions of these as “Stark-Heegner points” because they would simultaneously generalise Stark units and Heegner points.

  4. Modular forms of weight one Let g = � a n ( g ) q n be a cusp form of weight one, level N , and (odd) character χ . Deligne-Serre . There is an odd two-dimensional Artin representation ρ g : G Q − → GL 2 ( C ) attached to g , satisfying � i ∞ y s g ( iy ) dy L ( ρ g , s ) = L ( g , s ) = (2 π ) 2 Γ( s ) − 1 y . 0

  5. From Artin representations to weight one forms Buzzard-Taylor, Khare-Wintenberger . Conversely, if ρ is an odd, irreducible two-dimensional Artin representation, there is a weight one newform g satisfying L ( ρ, s ) = L ( g , s ) . Odd two-dimensional Artin representations are therefore an ideal testing ground for Stark’s conjectures.

  6. Stark units attached to forms of weight one Let H g := the field cut out by the Artin representation ρ g ; L ⊂ Q ( ζ n ) := field generated by the fourier coefficients of g ; V g := the L -vector space underlying ρ g . Conjecture (Stark). Let g be a cuspidal newform of weight one, with Fourier coefficients in L. Then there is a unit H g ⊗ L ) σ ∞ =1 satisfying u g ∈ ( O × � ∞ � � g ( iy ) dy L ′ ( g , 0) = = log u g . y 0

  7. A real quadratic example √ K = Q ( 5). √ √ � � � � The prime 29 = λ ¯ 11 − 5 11+ 5 λ = splits in K . 2 2 ψ g = character of K of order 4 and conductor λ ∞ 1 . Inducing ψ g from K to Q yields an odd, irreducible representation ρ g which cannot be obtained as the induced representation from an imaginary quadratic field. It corresponds to a cusp form χ 4 = 1 , g ∈ S 1 (5 · 29 , χ ) , cond ( χ ) = 5 · 29 .

  8. Stark’s calculation � ∞ 1 g )( iy ) dy ( g + ¯ = 1 . 65074962913147 · · · 2 y 0 log( u ) = 1 . 65074962913158 · · · , where √ √ √ √ √ � � � (3 + 2 5) + 7 + 2 5 + (20 + 14 5) + (6 + 4 5) 7 + 2 5 u = . 4

  9. Classification of odd two-dimensional Artin representations By projective image, in order of increasing arithmetic complexity: A. Reducible representations (sums of Dirichlet characters). B. Dihedral, induced from an imaginary quadratic field. C. Dihedral, induced from a real quadratic field. D. Tetrahedral case: projective image A 4 . E. Octahedral case: projective image S 4 . F. Icosahedral case: projective image A 5 .

  10. The status of Stark’s conjecture A. In the reducible case, it follows from the theory of circular units and Dirichlet’s class number formula. B. In the imaginary dihedral case, it follows from the theory of elliptic units and from Kronecker’s limit formula (as Stark observes). C. Stark has numerically verified many real dihedral cases. The “exotic” (tetrahedral, octahedral and icosahedral) cases appear to have been relatively less studied, even numerically.

  11. Stark-Heegner points Let E be an elliptic curve attached to f ∈ S 2 (Γ 0 ( N )). To extend Stark’s conjecture to elliptic curves, it is natural to replace Artin L -series by Hasse-Weil-Artin L -series L ( E , ρ g , s ) = L ( f ⊗ g , s ) . Remark . The BSD conjecture leads us to expect that the leading terms of L ( E , ρ g , s ) ought to encode the N´ eron-Tate heights of global points on E , and not their logarithms, which in any case are not numbers at all but elements of C / Λ.

  12. p -adic methods Motivation . This issue does not arise in a p -adic setting: the p -adic logarithms of global points are well-defined p -adic numbers. In fact, p -adic logarithms of global points do arise as leading terms of p -adic L -series attached to elliptic curves: a) The Katz p -adic L -function (Rubin, 1992); b) The Mazur-Swinnerton Dyer p -adic L -function (Perrin-Riou, 1993); c) Various types of p -adic Rankin L -functions attached to f ⊗ θ ψ (Bertolini-D, 1995; Bertolini-D-Prasanna, 2008); d) p -adic Garrett-Rankin L -functions attached to f ⊗ g ⊗ h (D-Rotger, 2012).

  13. p -adic iterated integrals D, Rotger . The leading terms of p -adic Garrett-Rankin L -functions can be expressed in terms of certain explicit analytic expressions, referred to as “p-adic iterated integrals” . These iterated integrals are attached to a triple ( f , g , h ) of newforms of weights (2 , k , k ), k ≥ 1. Their definition is based on the theory of p -adic and overconvergent modular forms.

  14. p -adic and overconvergent modular forms Let χ be a Dirichlet character of modulus N prime to p . M k ( Np , χ ) the space of classical modular forms of weight k , level Np and character χ ; M ( p ) k ( N , χ ) the corresponding space of p -adic modular forms; M oc k ( N , χ ) the subspace of overconvergent modular forms. The latter is a p -adic Banach space, on which the Atkin U p operator acts completely continuously . k ( N , χ ) ⊂ M ( p ) M k ( Np , χ ) ⊂ M oc k ( N , χ ) . Coleman’s classicality theorem . If h is overconvergent and ordinary (slope zero) of weight ≥ 2, then h is classical.

  15. The d operator Let d = q d dq be the Atkin-Serre d operator on p -adic modular forms.   n n j a n q n � if j ≥ 0;  d j ( � a n q n ) =  n p ∤ n n j a n q n � if j < 0 .  • If f ∈ M oc 2 ( N ), then F := d − 1 f ∈ M oc 0 ( N ) . • If h belongs to M k ( Np , χ ), then F × h ∈ M oc k ( N , χ ) , e ord ( F × h ) ∈ M k ( Np , χ ) ⊗ C p , where e ord := lim n U n ! p is Hida’s ordinary projector .

  16. p -adic iterated integrals: definition Suppose γ ∈ M k ( Np , χ ) ∨ , f ∈ S 2 ( N ) , h ∈ M k ( N , χ ) . Definition The p-adic iterated integral of f and h along γ is � f · h := γ ( e ord ( F × h )) ∈ C p . γ The terminology is motivated from the case k = 2, where f and h correspond to differentials on a modular curve. Remark: They differ from those that arise in Chen’s theory and Coleman’s p -adic extension, where one focusses on integrands that are “path independent”.

  17. Lauder’s “fast ordinary projection” algorithm • Given an overconvergent form, represented as a truncated q -series g = � N n =1 a n q n , the calculation of (mod p M ) e ord ( g ) typically requires (in favorable circumstances) applying U p to g roughly M times. • But the first N fourier coefficients of U M p g depend on knowing the first Np M fourier coefficients of g : so this naive algorithm runs in “exponential time” in the desired p -adic accuracy. • Alan Lauder’s fast “ordinary projection” algorithm calculates the ordinary projection in “polynomial time”. • Our experiments rely crucially on this powerful tool.

  18. The set-up f ∈ S 2 ( N ) corresponds to an elliptic curve E ; g ∈ M 1 ( N , χ − 1 ) , h ∈ M 1 ( N , χ ) classical weight one eigenforms; V gh := V g ⊗ V h , a 4-dimensional self-dual Artin representation, H gh the field cut out by it. Let g α ∈ M 1 ( Np , χ − 1 ) be an ordinary p -stabilisation of g attached to a root α g of the Hecke polynomial x 2 − a p ( g ) x + χ − 1 ( p ) = ( x − α g )( x − β g ) . Assume that γ = γ g α has the same system of Hecke eigenvalues as g α , γ g α ∈ M k ( Np , χ ) ∨ [ g α ]

  19. The question Give an arithmetic interpretation for � as γ g α ∈ M 1 ( Np , χ ) ∨ [ g α ] , f · h , γ g α in terms of the arithmetic of E over the field H gh .

  20. Some assumptions I. Certain local signs in the functional equation for L ( E , V gh , s ) are all 1. In particular, L ( E , V gh , s ) vanishes to even order at s = 1. II. The self-dual representation V gh breaks up as V gh = V 1 ⊕ V 2 ⊕ W , and ord s =1 L ( E , V 1 , s ) = ord s =1 L ( E , V 2 , s ) = 1 , L ( E , W , 1) � = 0 . The BSD conjecture then predicts that V 1 and V 2 occur in E ( H gh ) ⊗ L with multiplicity one . III. The frobenius σ p at p acting on V 1 (resp V 2 ) has the eigenvalue α g α h (resp. α g β h ). IV. (Not essential) The eigenvalues ( α g α h , α g β h ) do not arise in ( V 2 , V 1 ) at the same time, when V 1 � = V 2 .

  21. The conjecture Stark-Heegner Conjecture (D-Lauder-Rotger) Under the above assumptions, f · h = log E , p ( P 1 ) log E , p ( P 2 ) � , where log p u g α γ g α • P j ∈ V j -isotypic component of E ( H gh ) ⊗ L , and σ p P 1 = α g α h · P 1 , σ p P 2 = α g β h · P 2 ; • u g α = Stark unit in Ad 0 ( V g )-isotypic part of ( O × H g ) ⊗ L ; σ p u g α = α g · u g α . β g

  22. Remarks about the Stark-Heegner conjecture • The RHS of this conjecture belongs to L ⊗ Q p , because ( α g α h )( α g β h ) = α 2 g χ ( p ) = α g /β g . • The term log p ( u g α ) that appears in the denominator can be viewed as a p -adic avatar of � g α , g α � , and is defined over the field cut out by the adjoint of V g . In particular it depends only on the projective representation attached to g . • The unit u g α is closely related to the Stark units that will come up in Bill Duke’s lecture tomorrow.

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