11,431 research outputs found

    Fundamental strings and NS5-branes from unstable D-branes in supergravity

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    By using the non-supersymmetric pp-brane solutions delocalized in arbitrary number of transverse directions in type II supergravities, we show how they can be regarded as interpolating solutions between unstable Dpp-branes (a non-BPS D-brane or a pair of coincident D-brane-antiD-brane) and fundamental strings and also between unstable Dpp-branes and NS5-branes. We also show that some of these solutions can be regarded as interpolating solutions between NS5/NSˉ\bar{\rm NS}5 and Dpp-branes (for p≀5p \leq 5). This gives a closed string description of the tachyon condensation and lends support to the conjecture that the open string theory on unstable D-branes at the tachyonic vacuum has soliton solutions describing not only the lower dimensional BPS D-branes, but also the fundamental strings as well as the NS5-branes.Comment: 11 pages, LaTeX, one statement corrected and one reference added, v3: more details of the solution used is given, version to appear in Phys. Lett.

    Non-SUSY pp-branes delocalized in two directions, tachyon condensation and T-duality

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    We here generalize our previous construction [hep-th/0409019] of non-supersymmetric pp-branes delocalized in one transverse spatial direction to two transverse spatial directions in supergravities in arbitrary dimensions (dd). These solutions are characterized by five parameters. We show how these solutions in d=10d=10 interpolate between D(p+2p+2)-anti-D(p+2p+2) brane system, non-BPS D(p+1)(p+1)-branes (delocalized in one direction) and BPS Dpp-branes by adjusting and scaling the parameters in suitable ways. This picture is very similar to the descent relations obtained by Sen in the open string effective description of non-BPS D(p+1)(p+1) brane and BPS Dpp-brane as the respective tachyonic kink and vortex solutions on the D(p+2)(p+2)-anti-D(p+2)(p+2) brane system (with some differences). We compare this process with the T-duality transformation which also has the effect of increasing (or decreasing) the dimensionality of the branes by one.Comment: 19 pages, late

    Non-SUSY pp-branes, bubbles and tubular branes

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    We consider non-supersymmetric pp-brane solutions of type II string theories characterized by three parameters. When the charge parameter vanishes and one of the other two takes a specific value, the corresponding chargeless solutions can be regular and describe ``bubbles'' in static (unstable) equilibrium when lifted to d=11d = 11. In appropriate coordinates, they represent D6 branes with a tubular topology R1,p^{1,p} ×\times S6−p^{6-p} when reduced to d=10d=10, called the tubular D6 branes, held in static equilibrium by a fixed magnetic flux (fluxbrane). Moreover, a `rotation parameter' can be introduced to either of the above two eleven dimensional configurations, giving rise to a generalized configuration labelling by the parameter. As such, it brings out the relations among non-supersymmetric pp-branes, bubbles and tubular D6 branes. Given our understanding on tubular D6 branes, we are able to reinforce the interpretation of the chargeless non-supersymmetric pp-branes as representing pp-brane-antipp-brane (or non-BPS pp-brane) systems, and understand the static nature and various singularities of these systems in a classical supergravity approximation.Comment: 18 pages, footnote 7 removed due to some erro
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