Infinite hierarchies of nonlocal symmetries of the Chen--Kontsevich--Schwarz type for the oriented associativity equations
We construct infinite hierarchies of nonlocal higher symmetries for the oriented associativity equations using solutions of associated vector and scalar spectral problems. The symmetries in question generalize those found by Chen, Kontsevich and Schw…
Authors: Artur Sergyeyev
Infinite hierarc hies of nonlo cal symme tries of the Chen–Kon tsevic h–Sc h w arz t yp e for the orien ted asso ciativit y equations A. Ser gyeyev Mathemat ical Institut e, Si lesian Universit y in Opav a, Na Rybn ´ ı ˇ cku 1, 7 46 01 Opa v a, Czech Republic E-mai l : Artu r.Ser gyeyev@ math.slu.cz June 14 , 2009 W e construct infi nite hierarchies of nonlo cal higher symmetries for the orien ted asso ciativit y equa- tions using solutions of asso ciated v ector and scalar sp ect ral problems. The symmetries in question generalize those found b y Chen, Kon tsevic h and Sc hw arz [40] for the WD VV equations. As a bypro d- uct, we obtain a Darb oux-t yp e transformation and a (conditional) B¨ ac klund transformation for the orien ted asso ciativit y equations. In tro duction The Witten–Dijkgraaf–V erlinde–V erlinde (WD VV) equations [1, 2], and the related geometric s tructures, in particular, the F ro b enius manifolds [3]–[8], hav e attracted considerable atten tion because of their man- ifold applications in ph ysics and mathematics. More recen tly , the oriented asso ciativit y equations, a generalization of the WD VV equations, and t he related geometric structures, F -manifolds, see e.g. [7]–[19], hav e also b ecome a sub ject of in tense researc h. These eq uations ha v e first a pp eared in [3, Prop osition 2.3] as the equations for the displacemen t vec tor. The or iented asso ciativit y equations describ e inter alia isoasso ciative quan tum deformations of commuta- tiv e asso ciative algebras [14 , 15], cf. also [16 ]–[19]. The orien ted asso ciativit y equations (8) admit the gradient reduction (43 ) to the “usual” asso ciativit y equations (44). Equations (44) and the so-called Hes sian reduction (see [20, 21, 22, 23, 24] and [14]) of the o rien ted asso ciativit y equations naturally arise in top ological 2D gr avit y [1, 25], singularity theory and complex geome try ( see e.g. [8, 9]), and in differen tial g eometry and theory of integrable systems, se e [8], [26]–[36] a nd references therein. There is a conside rable b o dy of work on the symmetry prop erties of the WDVV equations, see e.g. [37, 38, 39, 40, 41 ] for the po int symmetries of the WDVV and generalized ( in the sense of [42] and ref- erences therein) WD VV equations, [4, 43, 44, 45] and references therein for finite symmetries, B¨ ac klund 1 transformations a nd dualities, and [26, 46, 47, 48] and references t herein for the higher symmetries and (bi-)Hamiltonian structures for the WDVV equations, a nd also for (44), in three a nd four independen t v ar ia bles. Although the approac h of [26, 46, 47, 48] in princ iple could [26] b e generalized to the WD VV equations in more than fo ur indep enden t v ariables, this w a s not done y et. Nev ertheless, in [3 9, 40] infinite sets of nonlo c al higher symme tries fo r the WD VV equations w ere found. T o the b est of our kno wledge, higher (or generalized [49]) symmetries of the orien te d asso ciativity equations in arbitrary dimension w ere nev er f ully explored. The go al of the presen t pap er is to construct nonlo cal higher symmetries for t he o rien ted asso ciativity equations equations using, in ana lo gy with [40], the solutions of auxiliary sp ectral problems. W e sho w that t he very solutions of the v ector sp ectral problem (9), either p er se or m ultiplied b y a suitably c hosen solution of the scalar sp ectral problem (10) with the opp osite sign of the sp ectral parameter, indee d ar e (infinitesimal) symmetries for the orien ted asso ciativit y equations (8), see Theorem 1 b elo w for details. The fact that solutions of (9) are symmetries for (8) is quite un usual in itself, as symmetries t ypically turn out to b e quadratic [50] ra ther than linear in solutio ns of auxiliary linear problems. Up on p erforming the gradien t reduction to the “usual” asso ciativity equations (44) we repro duce the results of [40], see Corollaries 6 and 8 b elow. Ho w ev er, not all nonlo cal symmetries from Theorem 1 surviv e the gradient reduction a nd yield symmetries for (44), see Corollary 6 and the subsequen t discussion. Expanding solutions of the spectral problems into formal T a ylor series in the spectral parameter yields infinite hierarchies of nonlo cal higher symmetries for (8) and (44), see Corollaries 4 and 8 b elow. Finally , as a b ypro duct, w e obtain a Darb oux-t yp e transformation and some B¨ ac klund-t ype trans- formations relating the solutions of “usual” and orien ted associativity equations, see Prop osition 1 and Corollaries 11 and 12 f o r further details. These transformations, a s w ell as the nonlo cal symmetries discusse d a b o ve, could p ossibly yield new solutions f or the oriented and “usual” asso ciativit y equations. 1 Preliminaries Let the Greek indices α, β , γ , . . . (except for λ, µ, η , ζ , σ , τ , χ, φ, ψ ) r un from 1 to n , where n is a fixed nat- ural n um b er, and summation o v er the rep eated indices b e understo o d unles s otherwis e explic itly stated. In what follow s w e also assume tha t all functions under study are sufficien tly smoo th for all necess ary deriv atives to exist. Consider the oriente d asso ciativity e quations , see e.g. [1 0]–[14], for the structure “constan ts” c δ αβ ( x 1 , . . . , x n ) of a comm utativ e ( c α ν ρ = c α ρν ) alg ebra: c ν αρ c ρ β γ = c ν ργ c ρ αβ , (1) ∂ c α β γ ∂ x ρ = ∂ c α ργ ∂ x β . (2) 2 The condition (1) means that the algebra in question is asso ciativ e, and ( 2 ) means that we consider isoasso ciativ e [14] quantum deformations o f the algebra in question. The oriented asso ciativit y equations (1), (2 ) can b e written as compatibility conditions of the Gauss– Manin equations, see e.g. [4 , 7, 14], for a scalar function χ ( λ ) (for t he sake of brevit y we shall often omit b elo w the dep endence on x 1 , . . . , x n ): ∂ 2 χ ( λ ) ∂ x α ∂ x γ = λc ν αγ ∂ χ ( λ ) ∂ x ν . (3) Here λ is the sp ectral parameter. Thes e eq uations ha v e a v ery interes ting in terpretation, with χ pla ying the role of a w a ve function, in the context of quantum deformations of asso ciativ e a lg ebras [14]. W e also ha v e a zero-curv ature represen tation for (1), (2) of the f o rm (see e.g. [6, 42]) ∂ ψ α ( λ ) ∂ x β = λc α β γ ψ γ ( λ ) , (4) where we again omit, for the sak e of brevit y , t he dep endence of ψ α on x 1 , . . . , x n . In other words, Eqs.(1 ) , (2) are precisely the compatibility conditions for (4). The quan tities ψ α ( λ ) are nothing but the comp onen ts of a generic ve ctor field whic h is cov arian tly constan t (in other terminology , parallel or flat) w ith resp ect to the co v aria n t deriv ativ e asso ciated with the one-parametric family of flat connections − λc α ν ρ . Up on in tro ducing the quantities φ α ( λ ) = ∂ χ ( λ ) /∂ x α Eq.(3) can b e written in the first-order form as ∂ φ α ( λ ) /∂ x β = λc δ αβ φ δ ( λ ) . (5) Quite obvious ly , the sp ectral problem (5) is, up to the c hange of sign of λ , adjoint to (4). No w let χ α ( λ ), α = 1 , . . . , n , b e the solutions of (3) no rmalized by the condition χ α ( λ ) | λ =0 = x α . It is we ll kno wn (see e.g. [4 , 8, 14]) that χ α are nothing but flat co ordina t es fo r the one-par ameter f a mily λc α ν κ of flat connections (the flatness readily follows fro m (1) a nd (2)). F ollowing [3, 4], we can represen t χ α in the form χ α ( λ ) = x α + λK α + O ( λ 2 ) , (6) where K α = K α ( x 1 , . . . , x n ) is the so- called displacemen t ve ctor. Plugging (6) in to (3 ) and restricting our atten t io n to the terms linear in λ yields c α β γ = ∂ 2 K α ∂ x β ∂ x γ . (7) The ansatz (7 ) automatically solv es (2), and (1 ) b oils down to the ov erdetermined system ∂ 2 K ν ∂ x α ∂ x ρ ∂ 2 K ρ ∂ x β ∂ x γ = ∂ 2 K ρ ∂ x α ∂ x β ∂ 2 K ν ∂ x ρ ∂ x γ (8) 3 for K α . In what follow s we shall refer to this system a s to the orien ted asso ciativity equations just as w e referred t o (1), (2), as, in com bination with (7), Eq.(8 ) is equiv alen t to (1), (2) pro vided c α ν ρ = c α ρν . Of course, the equations obtained b y plugging (7) into (4), that is, ∂ ψ α ( λ ) ∂ x β = λ ∂ 2 K α ∂ x β ∂ x γ ψ γ ( λ ) , (9) pro vide a zero-curv ature represen ta tion for (8). Lik ewise, plugging (7) into (3) yields a scalar sp ectral problem for (8): ∂ 2 χ ( λ ) ∂ x α ∂ x γ = λ ∂ 2 K ν ∂ x α ∂ x γ ∂ χ ( λ ) ∂ x ν . (10) 2 Darb o ux-t yp e transformation for orien ted asso ciativit y equations It is w ell kno wn, see e.g. [4, App endix B], [37] and references t herein, tha t there exist c hanges of v ariables that lea v e the se cond deriv a tiv es of the prep otential unc hanged and map solutions of the (generalized) WD VV equations in to new solutions. Quite in terestingly , there is a c hange of v ariables of this kind that in volv es [37] a solution of the spectral problem (4), and th us can b e though t of as a Darb oux-t ype transformation. It turns out tha t this transformation is readily generalized to the o r ien ted a ssociat ivity equations. Namely , the f ollo wing assertion holds. Prop osition 1 L et K α satisfy (8) an d ψ α ( λ ) solve the sp e ctr al pr oblem (9). Supp os e that det ∂ ψ α ( λ ) /∂ x β 6≡ 0 , intr o duc e new i n dep endent variables ˜ x α = ψ α ( λ ) , (11) and de fi ne (lo c al ly) new dep endent va ri a bles ˜ K β by the formulas ∂ ˜ K β ∂ ˜ x γ = ∂ K β ∂ x γ . (12) Then ˜ c α β γ = ∂ 2 ˜ K α ∂ ˜ x β ∂ ˜ x γ , (13) wher e ˜ K α = ˜ K α ( ˜ x ) ar e determine d f r om (12), sa tisfy ˜ c α β γ ˜ c γ ρν = ˜ c α ν γ ˜ c γ ρβ . (14) 4 Pr o of. First of all, w e need to sho w that (12) is w ell-defined, i.e., that there exist, at least lo cally , the functions ˜ K α ( ˜ x ) suc h that (12) holds. Quite clearly , this amoun ts to proving that w e hav e ∂ 2 ˜ K α ∂ ˜ x β ∂ ˜ x γ = ∂ 2 ˜ K α ∂ ˜ x γ ∂ ˜ x β , (15) or equiv alen tly (b y virtue of (12)), ∂ 2 K α ∂ x β ∂ ˜ x γ = ∂ 2 K α ∂ x γ ∂ ˜ x β . (16) F ro m (12) w e hav e ∂ 2 K α ∂ x β ∂ ˜ x γ = ∂ 2 K α ∂ x β ∂ x ε ∂ x ε ∂ ˜ x γ = c α β ε ∂ x ε ∂ ψ γ . (17) Hence, ∂ 2 K α ∂ x β ∂ ˜ x γ − ∂ 2 K α ∂ x γ ∂ ˜ x β = c α β ε ∂ x ε ∂ ψ γ − c α γ ε ∂ x ε ∂ ψ β . (18) W e w an t t o sho w tha t the expression on the left-hand side of (18) v anishes. But this is equiv alen t to v anishing of the following quan t it y: B α ρν = c α β ε ∂ x ε ∂ ψ γ − c α γ ε ∂ x ε ∂ ψ β ∂ ψ γ ∂ x ρ ∂ ψ β ∂ x ν . Using t he obv ious iden tit y ∂ ψ γ ∂ x ρ ∂ x ρ ∂ ψ ν = δ γ ν , where δ γ ν is the Kronec ke r delta, w e find tha t B α ρν = c α β ρ ∂ ψ β ∂ x ν − c α γ ν ∂ ψ γ ∂ x ρ . No w using (4) we obtain B α ρν = λ c α γ ρ c γ ν κ − c α γ ν c γ ρκ ψ κ ( 1 ) = 0 , and thus ∂ 2 K α ∂ x β ∂ ˜ x γ − ∂ 2 K α ∂ x γ ∂ ˜ x β = 0 , so (15) indeed holds, i.e., ˜ c α β γ = ˜ c α γ β . (19) No w w e only need to prov e that (14) holds, or equiv a len tly ˜ c α β γ ˜ c γ ρν − ˜ c α ν γ ˜ c γ ρβ = 0 . (2 0 ) Using ( 1 9), (17) a nd (18) w e o btain ˜ c α β γ = ˜ c α γ β = c α γ ε ∂ x ε ∂ ψ β = ∂ x ε ∂ ψ β c α γ ε . (21) 5 Using (21) for ˜ c α β γ in the first t erm of (20) and for ˜ c α ν γ in the second term of (20), and the formu la tha t immediately follo ws from (17), ˜ c ε κρ = c ε κν ∂ x ν ∂ ψ ρ , for ˜ c γ ρν in the first term o f (20) a nd for ˜ c γ ρβ in the second term of (20), w e see that the ex pression o n the left-hand side of (20) b oils do wn to ˜ c α β γ ˜ c γ ρν − ˜ c α ν γ ˜ c γ ρβ = ∂ x π ∂ ψ β ∂ x κ ∂ ψ ν c α π γ c γ ρκ − c α κγ c γ ρπ ( 1 ) = 0 , (22) and thus (14) indeed holds. 3 Nonlo cal symmetries for orien ted asso ciativi t y equatio n s Recall (see e.g. [49, 51, 52, 53]) that an (infinitesim al higher) symmetry fo r the oriented ass o ciativit y equations (8 ) is an evolutionary v ector field X = G α ∂ / ∂ K α suc h that G α satisfy the linearized v ersion of (8), t ha t is, ∂ 2 G ν ∂ x α ∂ x ρ ∂ 2 K ρ ∂ x β ∂ x γ + ∂ 2 K ν ∂ x α ∂ x ρ ∂ 2 G ρ ∂ x β ∂ x γ = ∂ 2 G ρ ∂ x α ∂ x β ∂ 2 K ν ∂ x ρ ∂ x γ + ∂ 2 K ρ ∂ x α ∂ x β ∂ 2 G ν ∂ x ρ ∂ x γ , (23) mo dulo (8) and differential consequence s thereof (or , informally , on solutions of (8)). This is equiv alent to compatibilit y of (8) with the flo w asso ciated with X , tha t is, ∂ K α /∂ τ = G α . A straightforw ard but somewhat tedious computation pro v es the follo wing generalization of the re- sults of Chen, Kon tsevic h and Sc h warz [40] (see Corollary 6 b elo w for the latt er) to the case of orien ted asso ciativit y eq uations. Theorem 1 The evolutionary ve ctor fields ψ α ( λ ) ∂ ∂ K α and ψ α ( λ ) χ ( − λ ) ∂ ∂ K α , wher e ψ α ( λ ) s a tisfy (9) an d χ ( λ ) satisfies (10), ar e nonlo c al higher symmetries for the oriente d a sso ciativity e quations (8), i.e., the flows ∂ K α ∂ τ λ = ψ α ( λ ) , (24) ∂ K α ∂ σ λ = ψ α ( λ ) χ ( − λ ) , (25) ar e c omp atible with ( 8). 6 Informally , compatibilit y here means that the flows (24 ) and (25) map the set S of (smo oth) solutions of (8) in to itse lf, i.e., S is in v ariant under the flows (24) and (25); see e.g. [5 1, 52, 53, 54, 55, 56] and references therein for the general theory of nonlo cal symmetries. In a more analytic language, Theorem 1 states that G α = ψ α ( λ ) a nd ˜ G α = ψ α ( λ ) χ ( − λ ) satisfy (23) provided (8), (9) and (10) hold. An un usual feature of the symmetries ψ α ( λ ) ∂ /∂ K α from Theorem 1 is that they are linear (rather t ha n quadratic, as it is the case for man y other systems , cf. [50]) in the solutions of auxiliary linear problem. It is natural to a sk whe ther the flows (24) and (25) are in t egrable system s in an y reasonable sense. The fo llo wing r esult provides linear sp ectral pro blems for these flow s and th us suggests t heir inte grabilit y . Corollary 1 T he flows (24) and (25) c an b e (nonuniquely) extende d to the flows for the quantities ψ α ( µ ) and χ ( µ ) as fol lows: ∂ ψ α ( µ ) ∂ τ λ = λµc α ν κ ψ ν ( λ ) ψ κ ( µ ) , (26) ∂ χ ( µ ) ∂ τ λ = λµ λ + µ ψ ν ( λ ) ∂ χ ( µ ) ∂ x ν , (27) ∂ ψ α ( µ ) ∂ σ λ = λµc α ν κ ψ ν ( λ ) ψ κ ( µ ) χ ( − λ ) + λµ λ − µ ∂ χ ( − λ ) ∂ x β ψ β ( µ ) ψ α ( λ ) , (28) ∂ χ ( µ ) ∂ σ λ = λµ λ + µ ψ ν ( λ ) ∂ χ ( µ ) ∂ x ν χ ( − λ ) . (29) In particular, b y Coro lla ry 1 Eq.(26) together with the system ∂ ψ α ( µ ) ∂ x β = µ ∂ 2 K α ∂ x β ∂ x γ ψ γ ( µ ) , (30) pro vide (assuming that (9) holds ) a zero-curv ature represen tation for t he extended system (8), (24), and th us ensure in tegrabilit y thereof. Lik ewise, the flo w (25) is in tegrable b ecaus e Eq.(30) along with the system ∂ 2 χ ( µ ) ∂ x α ∂ x β = µ ∂ 2 K δ ∂ x α ∂ x β ∂ χ ( µ ) ∂ x δ (31) and (28), (29) prov ide (a ssuming that (9) and (10) hold) a linear sp ectral pro blem for the extended system (8), (25), i.e., (8) and (25) are precisely the compatibility conditions for (28)–(3 1), a nd integrabilit y of the extended system in question follows . Using the extended flows fro m Corollary 1 w e readily obtain the follow ing result: Corollary 2 Al l flows (24) and (25) c ommute for al l values of p ar ame ters λ and µ : ∂ 2 K α ∂ τ λ ∂ τ µ = ∂ 2 K α ∂ τ µ ∂ τ λ , ∂ 2 K α ∂ τ λ ∂ σ µ = ∂ 2 K α ∂ σ µ ∂ τ λ , ∂ 2 K α ∂ σ λ ∂ σ µ = ∂ 2 K α ∂ σ µ ∂ σ λ . It is imp o r t an t to stress that this result p er se do es not imply comm utativit y of the extende d flo ws from Coro lla ry 1. Ho we v er, a straightforw ard computation prov es the follo wing assertion. 7 Corollary 3 T he extende d flows (24), (2 6), (27) c ommute, i.e., for al l values of λ , µ and ζ we have ∂ 2 K α ∂ τ λ ∂ τ µ = ∂ 2 K α ∂ τ µ ∂ τ λ , ∂ 2 ψ α ( ζ ) ∂ τ λ ∂ τ µ = ∂ 2 ψ α ( ζ ) ∂ τ µ ∂ τ λ , ∂ 2 χ ( ζ ) ∂ τ λ ∂ τ µ = ∂ 2 χ ( ζ ) ∂ τ µ ∂ τ λ . (32) W e in tend to study the remaining comm utat io n relations for the extended flo ws in more detail elsewhere. 4 Expansion in the s p ec t ral parameter and non lo cal p oten t ials No w consider a fo rmal T aylor expansion for ψ α in λ , ψ α ( λ ) = ∞ X k =0 ψ α k λ k . (33) It is immediate fr o m Theorem 1 that ψ α k ∂ / ∂ K α are symmetries for (8 ) , i.e., the flows ∂ K α ∂ τ k = ψ α k , k = 0 , 1 , 2 , . . . , (34) are compatible with (8). W e readily find from (9) the fo llo wing recursion relation: ∂ ψ α k ∂ x β = ∂ 2 K α ∂ x β ∂ x γ ψ γ k − 1 , k = 1 , 2 , . . . . (35) F or k = 0 w e hav e ∂ ψ α 0 /∂ x β = 0 for all β = 1 , . . . , n . No w let ( w 0 ) α β = δ α β , where δ α β is the Kro nec k er delta, and ( w 1 ) α β = ∂ K α /∂ x β . Define recursiv ely the follo wing sequence of nonlo cal quantities : ∂ ( w k ) β γ ∂ x α = ∂ 2 K β ∂ x α ∂ x ρ ( w k − 1 ) ρ γ , k = 2 , 3 , . . . (36) W e ha v e ψ α k = k X j =0 h γ j ( w k − j ) α γ , k = 0 , 1 , 2 , . . . , (37) where h γ j are arbitr a ry constan ts. In analog y with (33), consider a formal T a ylor expansion for χ in λ , χ ( λ ) = ∞ X k =0 χ k λ k . (38) W e obtain from (10) the following recursion relation: ∂ 2 χ k ∂ x α ∂ x γ = ∂ 2 K ν ∂ x α ∂ x γ ∂ χ k − 1 ∂ x ν , k = 1 , 2 , . . . . (39) 8 Set v α 0 = x α , v α 1 = K α , and, in analogy with (6) and (36), define the following sequence of nonlo cal quan tities v β k , β = 1 , . . . , n : ∂ 2 v β k ∂ x α ∂ x γ = ∂ 2 K ν ∂ x α ∂ x γ ∂ v β k − 1 ∂ x ν , k = 2 , 3 , . . . (40) In terms o f geometric theory of PDEs, see e.g. [51, 52, 55, 56], the quan tities ( w k ) α β and v γ k , α, β , γ = 1 , . . . , n , k = 2 , 3 , . . . , define an infinite-dimensional Ab elian co v ering o v er (8). W e ha v e the fo llo wing coun terpart of (37): χ k = b k + k X j =0 d k − j,γ v γ j , k = 0 , 1 , 2 , . . . , (41) where b k and d j,γ are arbitr a ry constants. Using (33) and (38) w e readily find tha t ψ α ( λ ) χ ( − λ ) = ∞ X k =0 ρ α k λ k , ρ α k def = k X j =0 ( − 1) j χ j ψ α k − j . It is no w immediate from The orem 1 that ( w k ) α β ∂ / ∂ K α and ρ α k ∂ / ∂ K α are symmetries for (8), and for k ≥ 2 these symmetries are nonlo cal. What is more, using Corollary 1 w e readily obtain the follow ing result. Corollary 4 T he oriente d as s o c i a tivity e quations (8) ha ve infinitely ma n y symm etries of the form X k ,β = ( w k ) α β ∂ ∂ K α and Y β k ,γ = k X j =0 ( − 1) j v β j · ( w k − j ) α γ ∂ ∂ K α , and al l asso ci a te d flows , i.e., ∂ K α ∂ τ β k = ( w k ) α β , ∂ K α ∂ σ γ k ,β = k X j =0 ( − 1) j v β j · ( w k − j ) α γ , c ommute: ∂ 2 K α ∂ τ β k ∂ τ ν l = ∂ 2 K α ∂ τ ν l ∂ τ β k , ∂ 2 K α ∂ σ β k ,γ ∂ τ ρ l,ν = ∂ 2 K α ∂ τ ρ l,ν ∂ σ β k ,γ , ∂ 2 K α ∂ σ β k ,γ ∂ σ ρ l,ν = ∂ 2 K α ∂ σ ρ l,ν ∂ σ β k ,γ , k , l = 0 , 1 , 2 , . . . , α, β , γ , δ, ν, ρ = 1 , . . . , n. It is readily seen t ha t the symmetries X k ,β and Y β k ,γ and the asso ciated flo ws a re no nlo cal for k ≥ 2 . W e stress once more that the part of Corollary 4 ab out comm uta t ivity of the flo ws a ssociat ed with X k ,β and Y β k ,γ mak es substan tial use o f the extended flo ws from Corolla ry 1 which are not uniquely defined. Moreov er, Corollary 4 do es not imply comm utativit y of t he extende d flows asso ciated with the symmetries X k ,β and Y β k ,γ . How ev er, the flows asso ciated with the symmetries X k ,β do commute after a (suitable) ex tension to the v ariables ( w k ) α β . Na mely , using Corollar ies 1 and 3 w e readily arriv e a t the following assertion. 9 Corollary 5 T he flows ∂ K α ∂ τ β k = ( w k ) α β , ∂ ( w l ) α π ∂ τ β k = c α ν ρ ( w k − 1 ) ν β ( w l − 1 ) ρ π , l = 0 , 1 , 2 , . . . , (42) wher e ( w 0 ) α β = δ α β , ( w 1 ) α β = ∂ K α /∂ x β , and we set ( w − 1 ) ν β ≡ 0 for c onvenie nc e, comm ute for a l l β , γ = 1 , . . . , n and al l k, l = 0 , 1 , 2 , . . . . Equivalently, the evo l utionary ve ctor fields ¯ X s,β ≡ X s,β = ( w s ) α β ∂ ∂ K α , s = 0 , ¯ X k ,β = ( w k ) α β ∂ ∂ K α + ∞ X l =2 c α κρ ( w k − 1 ) κ β ( w l − 1 ) ρ π ∂ ∂ ( w l ) α π , k = 1 , 2 , 3 , . . . , comm ute , i.e., [ ¯ X k ,β , ¯ X l,γ ] = 0 (se e e.g. [51] for the defin ition of the br ack e t [ , ] ), for al l β , γ = 1 , . . . , n and al l k , l = 0 , 1 , 2 , . . . . Th us, the orien ted asso ciativity equations (8) p ossess an infinite hierarc hy of commuting flows whose existence reconfirms integrabilit y of (8). 5 Nonlo cal symmetries for the gradi e n t reduct ion of orien ted asso ciativit y equations F ollowing [14], consider the so- called gradien t reduction of (8). Namely , assume that there exist a nonde- generate symmetric constant matrix η αβ and a function F = F ( x 1 , . . . , x n ), kno wn as a prep o ten tial in 2D top ological field theories [1, 2 , 3], such that K α = η αβ ∂ F /∂ x β . (43) Then (8) b oils down t o the fa mo us asso ciativit y equations for F [1, 2, 3, 4]: ∂ 3 F ∂ x α ∂ x β ∂ x δ η δγ ∂ 3 F ∂ x γ ∂ x ν ∂ x ρ = ∂ 3 F ∂ x α ∂ x ν ∂ x δ η δγ ∂ 3 F ∂ x γ ∂ x β ∂ x ρ . (44) Note that in t he standard theory of the WD VV equations (see e.g. [1, 2, 3, 4]) it is further required that ∂ 3 F ∂ x α ∂ x β ∂ x 1 = η αβ , (45) where η αβ is a nondegenerate constan t matrix suc h that η αβ η β γ = δ γ α . Ho wev er, in w hat follows w e shall not imp ose (45) and the s o-called quasihomogeneit y condition (see e.g. [1, 2, 3, 4, 7] for the discussion o f these conditions). 10 Up on assuming (43) we find that the auxiliary linear problem (9) also admits a reduction ψ α = η αβ ∂ χ/ ∂ x β . (46) This, along with (43), turns (9) into the following o v erdetermined sy stem of the Gauss–Manin equations for χ : ∂ 2 χ ( λ ) ∂ x α ∂ x γ = λη ρν ∂ 3 F ∂ x α ∂ x γ ∂ x ρ ∂ χ ( λ ) ∂ x ν . (47) This is nothing but ( 1 0) after the substitution (4 3 ), and a g ain the asso ciativity equations ( 44) are nothing but the compatibilit y conditions for (47); see e.g. [3, 4, 30] for the discussion of geometric asp ects of (47). Using Theorem 1 in conjunction with (43) and (46) we reco v er the f ollo wing result fr o m [40]. Corollary 6 F or any so lution χ ( λ ) of (47 ) the quantities χ ( λ ) ∂ ∂ F and χ ( λ ) χ ( − λ ) ∂ ∂ F ar e nonlo c a l higher symmetries for the asso ciativity e quations (44), i.e. , the e quations ∂ F ∂ τ λ = χ ( λ ) , (48) ∂ F ∂ ζ λ = χ ( λ ) χ ( − λ ) (49) ar e c omp atible with ( 44). The ab ove flows c an b e ( n onuniquely) extende d as fol lows ∂ χ ( µ ) ∂ τ λ = λµ λ + µ η ν β ∂ χ ( λ ) ∂ x β ∂ χ ( µ ) ∂ x ν , (50) ∂ χ ( µ ) ∂ ζ λ = λµ λ + µ η ν β ∂ χ ( λ ) ∂ x β ∂ χ ( µ ) ∂ x ν χ ( − λ ) + λµ λ − µ η ν β ∂ χ ( − λ ) ∂ x β ∂ χ ( µ ) ∂ x ν χ ( λ ) . (51) In particular, this result means that χ ( λ ) and χ ( λ ) χ ( − λ ) satisfy the linearized v ersion o f (44 ) pro vided (44) and (47) hold. Using the extended flow s from Corollary 6 w e readily obtain Corollary 7 Al l flows (48) and (49) c ommute: for a l l values of p ar am eters λ and µ w e have ∂ 2 F ∂ τ λ ∂ τ µ = ∂ 2 F ∂ τ µ ∂ τ λ , ∂ 2 F ∂ τ λ ∂ ζ µ = ∂ 2 F ∂ ζ µ ∂ τ λ , ∂ 2 F ∂ ζ λ ∂ ζ µ = ∂ 2 F ∂ ζ µ ∂ ζ λ . P erhaps a bit surprisingly , the prop er coun terpar t of the flow (49) f o r the orien t ed associativity equa- tions (8) is no t (25) itself but a linear combination of t he flow s (25) with the opp osite v alues of λ : ∂ K α ∂ ζ λ = ψ α ( λ ) χ ( − λ ) + ψ α ( − λ ) χ ( λ ) . Consider now a formal T aylor expansion in λ for a solution χ ( λ ) of ( 4 7), χ ( λ ) = ∞ X k =0 χ k λ k . 11 Notice that using a slightly differen t expansion of χ ( λ ), in v olving also λ − 1 , enables one t o construct solutions o f the WDVV equations directly from χ ( λ ), see [58] and references therein. Eqs.(41) remain v alid when χ ( λ ) satisfies (47) instead of (10) if w e substitute η αβ ∂ F /∂ x β for K α in to the definitions of v α k and (41 ). Then expanding the symmetries from Corolla r y 6 in p ow ers of λ yields Corollary 8 T he asso ciativity e quations (44) have infinitely many symmetries of the form ˜ X β k = v β k ∂ ∂ F , a nd ˜ Z αβ k = k X j =0 ( − 1) j v α j v β k − j ∂ ∂ F , k = 0 , 1 , 2 , . . . , α , β = 1 , . . . , n, and al l asso ci a te d flows , i.e., ∂ F ∂ τ β ,k = v β k , ∂ F ∂ ζ αβ ,k = k X j =0 ( − 1) j v α j v β k − j , (52) c ommute: ∂ 2 F ∂ τ β ,k ∂ τ ν,l = ∂ 2 F ∂ τ ν,l ∂ τ β ,k , ∂ 2 F ∂ τ γ ,k ∂ ζ αβ ,l = ∂ 2 F ∂ ζ αβ ,l ∂ τ γ ,k , ∂ 2 F ∂ ζ ρν,k ∂ ζ αβ ,l = ∂ 2 F ∂ ζ αβ ,l ∂ ζ ρν,k , k , l = 0 , 1 , 2 , . . . , α, β , γ , δ , ν, ρ = 1 , . . . , n. Again, it is clear that the symmetries ˜ X β k and ˜ Z αβ k and the asso ciated flows are nonlo cal for k ≥ 2. Note that the ab ov e results do not imply comm utat ivity for al l of the extende d flows fro m Coro llary 6 and therefore do not contradict the results fro m [39, 40]. On the o ther hand, using Corolla r y 3 w e r eadily find that, in p erfect agreemen t with [40], the extended flo ws (48), (50) do comm ute, i.e., ∂ 2 F ∂ τ λ ∂ τ λ ′ = ∂ 2 F ∂ τ λ ′ ∂ τ λ , ∂ 2 χ ( µ ) ∂ τ λ ∂ τ λ ′ = ∂ 2 χ ( µ ) ∂ τ λ ′ ∂ τ λ , (5 3) for a ll v a lues of λ , λ ′ and µ . The quan t it ies χ k coincide, up to a ch oice o f normalization, with the densities of Hamiltonians of in tegra ble bihamiltonian h ydro dynamic-t yp e systems asso ciated to an y solution of t he WDVV equations, see Lecture 6 of [4] and e.g. [57], and r eferences therein. It was mentioned in [4] that it is natural to consider these hy dro dynamic-t ype systems as higher (Lie–B¨ ac klund) symmetries for the WD VV equations, b ecause using these systems one can construct [4] the B¨ a cklund transformat io n for the WD VV equations. W e hav e no w seen that χ k and v α k can also b e in terpreted as symm etries o f the asso ciativity equations (44) (a nd, up on imp osing necess ary restrictions on F and χ , of the WDVV equations) in a far mor e straightforw ard manner. 6 In termed iate integrals and B¨ ac klund- typ e t r ans formations The compatibility conditions ∂ 2 ( w 2 ) β γ ∂ x α ∂ x ν = ∂ 2 ( w 2 ) β γ ∂ x ν ∂ x α for ( 36) with k = 2 yield precisely Eqs.(8), and w e hav e 12 Corollary 9 I f the functions K α and G β γ satisfy the system ∂ 2 K β ∂ x α ∂ x ρ ∂ K ρ ∂ x γ = ∂ G β γ ∂ x α , (54) then K α automatic al ly satisfy the oriente d asso c i ativity e quations ( 8 ). In p a rticular, if under t he ab o ve assumptions K α = η αβ ∂ F /∂ x β , wher e η αβ is a symmetric nonde gen- er ate c onstant matrix, then F automatic al ly s a tisfies the asso ci a tivity e quations (44). Just lik e (5 4), the compatibility conditions ∂ 3 v ν 2 ∂ x α ∂ x β ∂ x γ = ∂ 3 v ν 2 ∂ x γ ∂ x β ∂ x α for ( 40) with k = 2 also yield nothing but Eqs.(8), and w e obtain Corollary 10 I f the functions K α and G β satisfy ∂ 2 K ν ∂ x α ∂ x γ ∂ K β ∂ x ν = ∂ 2 G β ∂ x α ∂ x γ , (55) then K α automatic al ly satisfy the oriente d asso c i ativity e quations ( 8 ). In p a rticular, if under t he ab o ve assumptions K α = η αβ ∂ F /∂ x β , wher e η αβ is a symmetric nonde gen- er ate c onstant matrix, then F automatic al ly s a tisfies the asso ci a tivity e quations (44). Th us, (54) and (55) yield a kind of in t ermediate in tegrals for (8) (or, if K α = η αβ ∂ F /∂ x β , for (44)). In the terminology of [51, 52, 5 5, 56], (54) and (55) a lso define co v erings ov er (8) (resp ectiv ely , if K α = η αβ ∂ F /∂ x β , o v er (44)): for an y solution K α of (8) (resp. for any solution F o f (44)) there exist, at least lo cally , the functions G α β and G α suc h that ( 5 4) and ( 5 5) hold. Moreo ver, w e hav e the following observ ation. Corollary 11 I f the functions K α and H α satisfy the system ∂ 2 K β ∂ x α ∂ x ρ ∂ K ρ ∂ x γ = ∂ 2 H β ∂ x α ∂ x γ , (56) then K α and ˜ K α = H α automatic al ly satisfy the oriente d asso c i ativity e quations ( 8 ). Hence, (56) provides a conditional B¨ ac klund transformation for (8): if K α satisfy (8) a nd the conditions ∂ 2 K β ∂ x α ∂ x ρ ∂ K ρ ∂ x γ = ∂ 2 K β ∂ x γ ∂ x ρ ∂ K ρ ∂ x α (57) whic h are necessary for (56) to hold, then there exist, at least lo cally , ˜ K α = H α suc h that (56) holds and, moreo ver, these ˜ K α also satisfy (8). Setting K α = η αβ ∂ F /∂ x β , where η αβ is a symmetric nondegenerate constan t matrix, in Corollary 11 yields 13 Corollary 12 L et the functions F and H α satisfy the system η β ν η ρκ ∂ 3 F ∂ x α ∂ x ρ ∂ x ν ∂ 2 F ∂ x γ ∂ x κ = ∂ 2 H β ∂ x α ∂ x γ . (58) Then F automatic al ly sa tisfi e s the asso cia tivity e q uations (44) and ˜ K α = H α automatic al ly satisfy the oriente d ass o c iativity e quations (8). In complete analo g y with the ab ov e, (58) prov ides a B¨ ac klund tra nsformation relating the asso ciativity equations (4 4 ) supplemen ted with the conditions η ρκ ∂ 3 F ∂ x α ∂ x ρ ∂ x ν ∂ 2 F ∂ x γ ∂ x κ = η ρκ ∂ 3 F ∂ x γ ∂ x ρ ∂ x ν ∂ 2 F ∂ x α ∂ x κ (59) whic h a re necessary for (58) to hold, and the o rien ted asso ciativit y equ ations (8) for ˜ K α = H α . Note that the system (59) w as originally fo und and studied in [20, 22, 23] (in [20] it w as referred to as a condition for compat ible p o ten tial deformation of a pair o f the F r ob enius algebras) b ecause this sys- tem pla ys an imp ortan t ro le in classification of compatible Hamiltonian structures of hy dro dynamic type. Moreo ver, in [59] (cf. also [29]) it w as pro ved that (59) is also equiv alen t to the condition of inv olutivit y for a certain set of functionals constructed from the function F with resp ect to the constan t homogeneous first-order Poiss on brac k et of hydrodynamic type asso ciated with the flat contra v ariant metric η αβ . 7 Conclus ions and op en proble ms In the presen t pap er w e hav e found infinite hierarc hies of nonlo cal higher sym metries for the orien ted and “usual” asso ciativit y eq uations (8) and (44). These symme tries can b e emplo y ed for pro ducing new solutions from the kno wn ones and for constructing in v a rian t solutions using the standard tec hniques as presen ted e.g. in [4 9, 51, 52]. Moreo ver, it is natura l to ask whether there exist nonlo cal symme tries and conserv ation laws for (8) (resp. for (44)) that dep end o n the nonlo cal v ariables (36), ( 4 0) (resp. (40) with K α = η αβ ∂ F /∂ x β ) in a more complicated f ashion that t he symmetries found in Coro lla ry 4 (resp. Corollary 8). F or instance, o ne could lo ok for p oten tial (in the sense of [53, 60] and references therein) symmetries and conserv at io n law s of (8) in v olving the nonlo cal v a r iables (36) and (40). The next steps to tak e include elucidating the relatio nship among the nonlo cal symmetries o f (44) from Corollary 6 a nd the sym metries found in [37] for the gene ralized (in t he sens e of [42]) WDVV equations. The relationship (if an y exists) of t he flo ws (52) to the flo ws (5.15) from [61] could be of in terest to o . Understanding the precise relationship of t he symmetries from Corollary 8 to the tau- function a nd the B¨ a c klund transforma t io ns for the WDVV equations from [4] is y et another c hallenge. It w ould b e also 14 in teresting to find recursion op era t ors or master symmetries fo r (8) and (44) that generate the hierarc hies from Coro lla ries 4 and 8. Finally , it remains to b e seen whether the Darb oux-type transfor ma t io n from section 2 and the results from section 6 could indeed yield new solutions f or the oriented a nd “usual” asso ciativit y equations. W e in tend to address some of the ab o v e issues in our future w ork. Ac kno wledgmen ts This researc h w as supp orted in part by the Ministry of Education, Y outh and Sp orts of the Czec h Republic (M ˇ SMT ˇ CR) under grant MSM 4781305 9 04, and by Silesian Univ ersity in Opav a under gra nt IGS 9/2008. 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