2013
DOI: 10.1007/jhep04(2013)046
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Multi-superthreads and supersheets

Abstract: We obtain new BPS solutions of six-dimensional, N = 1 supergravity coupled to a tensor multiplet. These solutions are sourced by multiple "superthreads" carrying D1-D5-P charges and two magnetic dipole charges. These new solutions are sourced by multiple threads with independent and arbitrary shapes and include new shape-shape interaction terms. Because the individual superthreads can be given independent profiles, the new solutions can be smeared together into continuous "supersheets," described by arbitrary … Show more

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Cited by 16 publications
(44 citation statements)
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“…2 The same conclusion was reached from a different perspective in [31]. For attempts to construct v-dependent solutions representing unbound superpositions of D1 and D5 charges carrying momentum, see [32][33][34]. 3 In the example of section 5.2 the coordinate system in which the 4D part of the metric is conformally v-independent does not coincide with the coordinate system in which the asymptotic limit of the geometry looks explicitly like…”
Section: Jhep03(2014)007mentioning
confidence: 72%
“…2 The same conclusion was reached from a different perspective in [31]. For attempts to construct v-dependent solutions representing unbound superpositions of D1 and D5 charges carrying momentum, see [32][33][34]. 3 In the example of section 5.2 the coordinate system in which the 4D part of the metric is conformally v-independent does not coincide with the coordinate system in which the asymptotic limit of the geometry looks explicitly like…”
Section: Jhep03(2014)007mentioning
confidence: 72%
“…The entropy of these states does not scale with the charges as rapidly as the black fivebrane entropy, which is larger by a factor of order √ n 5 due to the disparity between the tensions of the fundamental string and the little string. Similarly, the entropy of the largest known class of horizonless microstate geometries [18] is based on placing supertubes at the bottom of a microstate geometry with a long but finite throat and absorbing them into the background; the result does not scale with the charges as rapidly as the BTZ black hole entropy (though that deficiency could be due to an insufficiently general ansatz for the shape modes of the supertube [8,9,58]). At the same time, the long string is not apparent.…”
Section: Jhep11(2015)195mentioning
confidence: 99%
“…Nevertheless, it is a possibility that techniques to construct a finite fraction of three-charge black hole states might be found, so that similar amounts come from geometrical structures and from horizon-wrapping brane condensates. Indeed, a proposal for the "missing" entropy of geometrical solutions has been explored in [8,9,58]. But even if microstate geometries turn out not to be the main contributors to the density of states, the macroscopic entropy already found from geometrical constructions [18], the matching of certain low-energy black hole emission spectra [59][60][61], the possibility of perturbing them slightly to become black holes, and the increasingly precise duality map (see for example [9,10,52,62]) make these objects particularly worthy of further study.…”
Section: Jhep11(2015)195mentioning
confidence: 99%
“…However, it was recently shown in [18] that while the requirements on the five-dimensional spatial background is essentially non-linear, the BPS equations that determine all the charges, two sets of the magnetic fluxes and the angular momentum are, in fact, linear. This means that there are certainly interesting new classes of BPS solution within reach and some of these have already been obtained [18,[27][28][29].…”
Section: Jhep10(2013)137mentioning
confidence: 99%
“…If one removes the condition (5.18), and works with general q ± , k ± , then the foregoing discussion goes through as before except that the collapsing circles and density functions are parametrized by (φ, χ ± η) and χ ∓ η respectively. Using (5.6), one obtains 27) and these define the modes along the circles of finite size at r + = 0 and r − = 0 respectively. This is, of course, consistent with the observation that the finite circle and its modes are defined by r ± α as in section 4.3.…”
Section: Jhep10(2013)137mentioning
confidence: 99%