2007
DOI: 10.1088/1126-6708/2007/08/058
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Direct integration of the topological string

Abstract: We present a new method to solve the holomorphic anomaly equations governing the free energies of type B topological strings. The method is based on direct integration with respect to the non-holomorphic dependence of the amplitudes, and relies on the interplay between non-holomorphicity and modularity properties of the topological string amplitudes. We develop a formalism valid for any Calabi-Yau manifold and we study in detail two examples, providing closed expressions for the amplitudes at low genus, as wel… Show more

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Cited by 131 publications
(245 citation statements)
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“…We derive a generalization of the Zamolodchikov renormalization formula [19][20][21] (see also [8,[22][23][24][25]) for this class of constrained quiver theories, which includes the first-order differential equations for the effective couplings and their implicit solution via the Thomae formulas. Finally, we study another kind of non-linear differential equations for the ex-…”
Section: Jhep05(2014)097mentioning
confidence: 99%
“…We derive a generalization of the Zamolodchikov renormalization formula [19][20][21] (see also [8,[22][23][24][25]) for this class of constrained quiver theories, which includes the first-order differential equations for the effective couplings and their implicit solution via the Thomae formulas. Finally, we study another kind of non-linear differential equations for the ex-…”
Section: Jhep05(2014)097mentioning
confidence: 99%
“…It is self-mirror and thereby does not have experience any worldsheet instanton corrections at the twoderivative level [33]. There is however a non-trivial pattern of higher-derivative corrections for this background (graviphoton-curvature couplings), some of which have been computed in [35,36]. We begin by considering the harmonic forms on the Enriques Calabi-Yau Y = (K3 × T 2 )/Z τ 2 .…”
Section: The Enriques Calabi-yaumentioning
confidence: 99%
“…Turning now to the case of g > 1 closed amplitudes, let us first of all recall the main statements put forward in [7,56] for the computation of higher genus free energies. As mentioned in section 6.3.2, modular symmetry is an amazingly stringent constraint.…”
Section: Generalities On G > 1 Free Energiesmentioning
confidence: 99%
“…c (g) 0 (τ ). In the 1-parameter cases analyzed in [7,56], this is systematically done by plugging into (6.52) an ansatz for c (g) 0 (τ ) which is then determined from extra boundary data. More in detail, this works as follows: at fixed genus g, c (g) 0 (τ ) is a weight w = 6g − 3 modular form 8 .…”
Section: Generalities On G > 1 Free Energiesmentioning
confidence: 99%
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