Abstract

We consider space and time dependent fuzzy spheres S 2 p arising in D 1 – D ( 2 p + 1 ) intersections in IIB string theory and collapsing D ( 2 p ) -branes in IIA string theory. In the case of S 2 , where the periodic space and time-dependent solutions can be described by Jacobi elliptic functions, there is a duality of the form r to 1 / r which relates the space and time dependent solutions. This duality is related to complex multiplication properties of the Jacobi elliptic functions. For S 4 funnels, the description of the periodic space and time dependent solutions involves the Jacobi inversion problem on a hyper-elliptic Riemann surface of genus 3. Special symmetries of the Riemann surface allow the reduction of the problem to one involving a product of genus one surfaces. The symmetries also allow a generalisation of the r to 1 / r duality. Some of these considerations extend to the case of the fuzzy S 6 .

Highlights

  • Fuzzy spheres of two, four, six dimensions arise in a variety of related contexts

  • It is of interest to consider using the constraint to solve u1 in terms of u2 and describe x1 as a function of u2. The reason for this is that the automorphisms of the Riemann surface allow us to relate the large r behaviour of the spatial problem described in terms of the u1 variable, to the small r behaviour of the time dependent problem described in terms of the u2 variable and vice versa

  • The space and time dependence of fuzzy spheres S2, S4 and S6 are governed by equations which follow from the DBI action of D-branes

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Summary

Introduction

Four, six dimensions arise in a variety of related contexts. On the one hand they describe the cross-sections of fuzzy funnels appearing at the intersection of. In the case of the fuzzy 2-sphere, there are purely spatial and purely time-dependent solutions described in terms of Jacobi elliptic functions. For solutions described in terms of elliptic functions, the inversion symmetry is related to the property of complex multiplication u1 → iu. Using the conservation laws of the spatial or time evolution, the time elapsed or distance along the 1-brane can be expressed in terms of an integral of a holomorphic differential on the genus 3 hyper-elliptic curve. The solution r(t, σ) can still be related to a constrained Jacobi inversion problem, which can be solved in terms of genus 3 Riemann theta functions. Appendix C describes the derivation of the Jacobi-Cn solution for the fuzzy S2 by steps using Weierstrass ℘ functions, since the discussion of section 5 on the fuzzy S6 is expressed in terms of higher genus generalisations of the ℘ functions

Space and Time-Dependent Fuzzy S2
Space and Time dependent fuzzy S4
Solutions for the space-dependent fuzzy spheres
Solutions for the time-dependent fuzzy spheres
Geometry and Automorphisms of Hyper-elliptic curve for the fuzzy S4
Evaluation of integrals
Series expansion of u2 as a function of u1
Evaluation of the time of collapse and the distance to blowup
Solution of the problem in terms of the u2 variable and largesmall duality
Large-small duality at finite r0
Space and Time dependent Fuzzy-S6
Jacobi inversion problem and θ functions
Summary and Outlook
Lorentz Invariance of the BPS condition
Chern-Simons terms and D-brane charges for D1-D3 system
B Lagrangians for holomorphic differentials

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