Real symplectic formulation of local special geometry

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1 CERN-PH-TH/ IFIC/06-3 arxiv:hep-th/0603 v 3 May 006 Real symplectic formulation of local special geometry Sergio Ferrara and Óscar Maciá Physics Department, Theory Unit, CERN, CH- Geneva 3, Switzerland Sergio.Ferrara@cern.ch INFN, Laboratori Nazionali di Frascati, Via Enrico Fermi 40, I Frascati, Italy Departament de Física Teòrica, Universitat de València and IFIC C/Dr. Moliner, 50, E-4600 Burjassot València), Spain. Oscar.Macia@ific.uv.es Abstract We consider a formulation of local special geometry in terms of Darboux special coordinates P I = p i,q i ), I =,...,n. A general formula for the metric is obtained which is manifestly Spn, R) covariant. Unlike the rigid case the metric is not given by the Hessian of the real function SP) which is the Legendre transform of the imaginary part of the holomorphic prepotential. Rather it is given by an expression that contains S, its Hessian and the conjugate momenta S I = S. Only in the one-dimensional case n = ) is the P I real two-dimensional) metric proportional to the Hessian with an appropriate conformal factor.

2 Introduction Local special geometry [], [], [3], [4], [5], is the underlying geometry of N= supergravity in four dimensions coupled to vector multiplets. It also emerges in any compactification, obtained from a higher-dimensional theory, when eight supersymmetries are preserved in four dimensions or, in a more general setting, when the lower-dimensional theory can be viewed as a deformation of a N = locally supersymmetric Lagrangian. These theories include Calabi Yau compactifications from type II supergravity [3], [4] as well as compactifications on more general manifolds with G = SU3) structures [6], [7], [8], [9], [0]. Special geometry also plays an important role in the physics of black holes, attractor equations [], [], [3], [4], which control the horizon geometry, and more recently it has been used also to connect the black hole entropy to topological partition functions in superstring theory [5], [6], [7]. In this framework it is useful to reconsider a formulation of special geometry in real [8], [9], [0], rather than complex variables. Real variables, will be denoted as Darboux coordinates P I = p i, q i ), i =,..., n where n is the complex dimension of the local) special manifold. One of the reasons to adopt these coordinates is that the attractor equations can be written as real equations [], [], [3], [4], [], [], [3], which determine the real charge vector Q = m Λ, e Λ ), Λ = 0,,..., n) in terms of the holomorphic sections V = X Λ, F Λ = Λ F) of special geometry [], [], [3], [5]; A direct real formulation of the geometry may therefore have a simplifying role. In this note we extend a previous investigation [4] on the real formulation of rigid special geometry to the local case. The main result is the derivation of a general formula for the metric in special Darboux coordinates and also comment on the main differences from the rigid case. A very important role is also played here by a n n symplectic real symmetric matrix MRf ij, If ij ) constructed in terms of the holomorphic matrix f ij = ft) t i t j where t i = Xi are the special coordinates of the local special geometry and ft) is the X 0 holomorphic prepotential in special coordinates. As in the rigid case the M matrix which satisfies MΩM = Ω where Ω is the invariant symplectic form of Spn, R)) is related to the Hessian H IJ = P I P J of a certain Hamiltonian function Sp, q) written in Darboux special coordinates but, unlike the rigid case, the general formula for the metric is given by S g IJ P) = S H IJ + 4S S IS J + HΩS) I HΩS) J ) ) The first term is analogous to the term that is present in the rigid case. The second term, due to the Hodge-Kähler structure of local special geometry, has no rigid analogue and depends, other

3 than S and its Hessian, also on the conjugate momenta S I = S P I, of the Darboux coordinates P I. Note that HΩS) I denotes the expression HΩS) I = H IK Ω KL S L, Ω KL = Ω KL This paper is organized as follows. In section we describe local special geometry in holomorphic and Darboux special coordinates and compute the Kähler metric in real symplectic coordinates. In section 3 we compute the real symmetric) metric in the real symplectic Darboux coordinates, and we show the explicit Spn, R) covariance of this metric and its differences from the rigid case. In section 4 some examples are given. Local special geometry in Darboux coordinates We consider local special geometry in special coordinates t Λ = XΛ X 0 coordinates the holomorphic symplectic sections = t 0 =, t i ). In these take the simple form V = V = X Λ, Λ F) ), t i ; f 0 = f t i f i, f i = f ) t i in terms of the prepotential ft) = X 0 ) FX) where FX) is homogeneous of degree [] X Λ Λ F = F From this, it follows that ft) is a fairly arbitrary holomorphic function fo t i. Moreover t i are scalar sections of the Hodge bundle since under a holomorphic gauge transformation X Λ, F Λ ) e α X Λ, F Λ ), i α = 0 4) the special coordinates t i and the prepotential ft) are invariant. Property 4) is crucial in defining real coordinates. In fact, while it makes sense to define the real part of the holomorphic special coordinates t i, it would not make sense to define a real part of X Λ since this operation would be incompatible with the Hodge structure of the manifold. Note that this is also the main difference between the local and the rigid cases [8], [9], [4], [4], since in the latter the Hodge structure is absent and this obstruction does not arise. We also note that in local special coordinates the Spn +, R) covariance is lost by the Kähler gauge-fixing X 0 = ) but still a Spn, R) structure is present with respect to the reduced n-dimensional holomorphic section V R = t i, f i = f ) 5) t i 3) 3

4 In particular, in terms of the matrix f ij = f, we can construct a real symmetric n n t i t j symplectic matrix Mf ij ) as follows [6], []: ) Ifij + Rf Mf ij ) = ik If ) kl Rf lj Rf ik If ) kj If ) ik Rf kj If ) ij 6) with the obvious property MΩM = Ω. We note at this point that the Mf ij ) matrix considered here is not the MF) matrix considered in [6], []. Indeed while MF) Spn +, R) is a n + ) n + ) symplectic matrix, the matrix considered here is n n and it is Spn, R) symplectic. However, it is this last matrix which plays a role in our considerations. The Kähler potential of special geometry in these coordinates is K = logy 7) from which the following expression for the metric holds: By explicit computations the two terms in 9) give: Y = i f f t i t i )f i + f i ) ) 8) g i j = i j K = Y Y i j + Y Y iy j 9) K i j = i Y f ij f ij ) + Y fi f i + t k t k )f ki ) f j f j + t k t k ) f kj ) ) 0) We now go to Darboux special coordinates exactly as we did in the rigid case [4] i.e. we define t i = p i + iφ i, f i = q i + iψ i ) and the Legendre transform Sp, q) of the imaginary part of the prepotential L = If ) Then the q i, φ i ) and p i, ψ i ) real sections are pairs of conjugate variables for L and in terms of S given by we have the following set of equations q i = L φ i, ψ i = L p i 3) Sp, q) = q i φ i p, q) Lp, φp, q)) 4) φ i = S q i, ψ i = S p i 5) 4

5 By comparing 4) and 8) we realize that [5], [7], [7], [6] Y = 4S 6) i.e. S = 4 e K 7) Eq. 7) is the main difference between rigid and local special geometry. We just recall that in the former the square of the) distance ds is given by [8], [9], [4], [5] K ij dz i d z j = H IJ dp I dp J 8) where H IJ = S is the Hessian of the S functional. In the next section we will see how the P I P J rigid formula 8) is modified in the local case. The change of variables from the holomorphic sections t i, f i ) to the Darboux variables p i, q i ) and φ i, ψ i ) is exactly as in the rigid case it is still true [4] that the H matrix ) S S ) p H = i p j p i q j Sij S j = i Sj i S ij 9) S q i p j S q i q j is equal to the negative of the) M matrix defined in 6), then it follows that HΩH = Ω i.e. S k i S kj S k j S ki = 0 S ik S j k Sjk S i k = 0 0) S ik S kj S k i S j k = δ j i By comparing the M ij and M i j entries of M with H it also follows that where S ) kj = S kj ) is the inverse of S kj defined by 9). f ij = S k i + iδk i )S ) kj ) We can now write Eq. 0) in Darboux special coordinates by means of Eqs. ), 3), and ) and we finally obtain K i j = S Sij ) + S S 4S p i p + S S f j ki flj + S S q k q l q k p f j ki + S ) S q k p f i kj ) where f ij is given by ). We just note that while in the rigid case K i j = S ij ), in the local case ) also depends on S and the canonical momenta S I = S. The second term in ) is the main difference P I between the rigid and local case. 5

6 3 The real symplectic metric In order to compute the real metric we have to transform the distance from holomorphic to Darboux special coordinates ds = K i jdt i d t j = g IJ dp I dp J 3) The result is obtained by computing the differentials dt i dt j in Darboux coordinates and then comparing the two expressions in Eq. 3). We just mention that the computation of dt i d t j is exactly the same as in the rigid case [4] since the Legendre transform and the conjugate variables are the same. Indeed only Eqs. 9), 0), ) which are the same as in rigid special geometry really matter. The change of variables in the differentials was given in Eq. 50) of reference [4] and it is reproduced here for the benefit of the reader. )) dt i d t j = δkδ i j l + S S q i p k q j p + i S l q i p k δj l S q j p lδi k dp k dp l )) S S + + S S S + i δ j k q i q l q j p k q i p k q j q l q i q S δk i dp k dq l l q j q l ) S S + dq k dq l 4) q i q k q j q l By explicit multiplication of ) with 4) we finally obtain, from the first term in ) S Sij ) dt i d t j = S H IJdP I dp J 5) For the second term of ) by multiplying by dt i d t j ) we find where and 8S S K H KI S J S K H KJ S I ) dpl H LI dp J dp L H LJ dp I) 6) S K = Ω KI S I, H LJ = H LJ ), dp L = Ω LI dp I Ω KI = Ω KI ) = Ω KI By multiplying the four terms in 6) we finally obtain: where 4S S IS J + HΩS) I HΩS) J ) 7) HΩS) I = H IK Ω KL S L The final expression for the real symmetric metric in Darboux coordinates, for local special geometry, is therefore given by g IJ P) = S H IJ + 4S S IS J + HΩS) I HΩS) J ) 8) 6

7 We note at this point that a major simplification occurs for I =, which corresponds to one-dimensional complex special geometry. Indeed in this case and then 6) becomes In this case, the metric therefore is S K H KI S J S K H KJ S I = Ω IJ S K H ) KL S L 9) dp L H LI dp J dp L H LJ dp I = Ω IJ dp L H LK dp K 30) 4S S KH ) KL S L H IJ dp I dp J 3) g IJ = S + ) S) H 4S SH IJ 3) We finally note that the metric given by 8) has a manifest Spn, R) covariant structure. The simplification occurring in 9) is due to the fact that for Sp, R) the antisymmetric representation is the identity while the traceless part is non-vanishing for n > ; and this is the reason why 8) and 3) are equivalent only for n =. It is obvious that in special coordinates the Spn+, R) structure of the geometry is lost and only a Spn, R) structure is manifest. Nevertheless we have shown that this is what is needed to obtain a general expression for the metric in terms of the Darboux data of local special geometry. The Spn +, R) covariance will be considered elsewhere. 4 Some examples In this section we compute the real metric in some examples of special geometry. The two examples in question correspond to a cubic and quadratic prepotential, for one complex scalar: Let us first consider the cubic case. The S functional is ft) = 3 t3 33) ft) = i 4 t ) 34) 4S = Y = 8 3 It)3 35) where S = 3 It)3 so that It < 0. Note that in this case If tt = It < 0 and therefore the Hessian will be positive definite. Going to Darboux coordinates we find q = p φ φ = ±p q) 36) so we have p > q and also the negative root must be chosen such that S is positive. From 36) and 35) we obtain S = 3 p q) 3 37) 7

8 The Hessian matrix is given by H = p q) p q) p p Since DetH) = and also p q) TrH) = p q) + > 0, H is indeed positive definite. We can now compute the metric by using 3). First, by computing the second term, we obtain ) 38) SH S = p q) 3 39) and then S + SH S = 3 4S ) p 3 q) 3 = 8 8 p q) 3 40) so that the metric is g IJ p, q) = 3 8 p q) p q) p p We now turn to the second example 34) where now therefore we must take p + φ <. Since we have It follows that The Hessian matrix is ) 4) Y = 4S = t t = p φ 4) If = 4 p φ ) = L q = L φ = φ φ = q Y = 4S = p 4q, S = 4 p 4 q 43) H = 0 0 and it is negative definite. The conjugate momenta are We then have and the conformal factor becomes The local metric is then finally given by S p = p, g IJ p, q) = ) S q = q SH S = p + 4q ) p 4q ) p 4q ) ) 44) 45)

9 5 Acknowledgements We would like to thank M.A. Lledó for enlightening discussions. S.F. would like to thank the Theoretical Physics Department at the University of Valencia where part of this work was performed. S.F. was partially supported by funds of the INFN- CICYT bilateral agreement. The work of S.F. has also been supported in part by the European Community Human Potential Program under contract MRTN-CT Constituents, fundamental forces and symmetries of the Universe, in association with INFN Frascati National Laboratories and by the D.O.E. grant DE-FG03-9ER4066, Task C. O.M. wants to thank the Department of Physics, Theory Division at CERN for its kind hospitality during the realization of this work. The work of O.M. has been supported by an FPI fellowship from the Spanish Ministerio de Educación y Ciencia MEC), through the grant FIS MEC) and EU FEDER funds, by the Generalitat Valenciana, contracts GV04B- 6, GV05/0 and by the EU network MRTN-CT Constituents, fundamental forces and symmetries of the Universe. References [] B. de Wit, P.G. Lauwers, A. Van Proeyen, Lagrangians of N= supergravity-matter systems Nucl.Phys.B 55:569, 985 [] A. Strominger, Special geometry, Commun.Math.Phys. 33:63-80, 990 [3] S. Ferrara, A. Strominger, N= space-time supersymmetry and Calabi-Yau moduli space, Presented at Strings 89 Workshop, College Station Coll.Station Workshop 989:045-5 P. Candelas, X. de la Ossa, Moduli space of Calabi-Yau manifolds, Nucl.Phys.B 355:455-48, 99, Coll.Station Wkshp. 990: L. Castellani, R. D Auria, S. Ferrara, Special Kähler geometry: An intrinsic formulation form N= space-time supersymmetry, Phys.Lett.B 4:57, 990 [4] S. Cecotti, S. Ferrara, L.Girardello Geometry of type II superstrings and the moduli of superconformal field theories Int. J.Mod.Phys. A4:475,989 [5] L. Andrianopoli, M. Bertolini, A. Ceresole, R. D Auria, S. Ferrara, P. Fré, T. Magri, N= supergravity and N= superyang-mills theory on general scalar manifolds: symplectic covariance, gaugings and the momentum map, J.Geom.Phys. 3:-89, 997, hepth/ [6] S. Gurrieri, J. Louis, A. Micu, D. Waldram, Mirror symmetry in generalized Calabi Yau compactifications. Nucl.Phys.B 654:6-3, 003, hep-th/00 [7] S. Kachru, M.B. Schulz, P.K. Tripathy, S.P. Trivedi, New supersymmetric string compactifications, JHEP 0303:06,003, hep-th/08 [8] G. Lopes-Cardoso, G. Curio, G. Dall Agata, D. Lust, P. Manousselis, G. Zoupanos, Nonkähler string backgrounds and their five torsion classes, Nucl.Phys.B65:5-34, 003, hep-th/08 9

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