<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>2</mml:mn><mml:mn /></mml:math>supergravity in ten dimensions

Giani, F.; Pernici, M.

doi:10.1103/physrevd.30.325

Cited by 137 publications

(207 citation statements)

References 27 publications

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“…for D = 10, I RR = {0, 2} (I RR = {1, 3}) and I NS = {1} [38][39][40] and eleven-dimensional supergravity for D = 11 and I M = {2} [41]. In general, the D/NS/M-branes couple both electrically and magnetically to the above potentials.…”

Section: Jhep04(2015)171mentioning

confidence: 99%

Probing the hydrodynamic limit of (super)gravity

Dato

Gath

Pedersen

2015

J. High Energ. Phys.

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Abstract:We study the long-wavelength effective description of two general classes of charged dilatonic (asymptotically flat) black p-branes including D/NS/M-branes in ten and eleven dimensional supergravity. In particular, we consider gravitational brane solutions in a hydrodynamic derivative expansion (to first order) for arbitrary dilaton coupling and for general brane and co-dimension and determine their effective electro-fluid-dynamic descriptions by exacting the characterizing transport coefficients. We also investigate the stability properties of the corresponding hydrodynamic systems by analyzing their response to small long-wavelength perturbations. For branes carrying unsmeared charge, we find that in a certain regime of parameter space there exists a branch of stable charged configurations. This is in accordance with the expectation that D/NS/M-branes have stable configurations, except for the D5, D6, and NS5. In contrast, we find that Maxwell charged brane configurations are Gregory-Laflamme unstable independently of the charge and, in particular, verify that smeared configurations of D0-branes are unstable. Finally, we provide a modification to the mapping presented in arXiv:1211.2815 and utilize it to provide a non-trivial cross-check on a certain subset of our transport coefficients with the results of arXiv:1110.2320.

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Section: Jhep04(2015)171mentioning

confidence: 99%

Probing the hydrodynamic limit of (super)gravity

Dato

Gath

Pedersen

2015

J. High Energ. Phys.

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“…Collecting all the previous subsectors, taking the expansions (5.9) into account, we finally arrive at the complete four-point Lagrangian: 36) where the tensors u, v, are defined in appendix E. The sums over M, . .…”

Section: Pole-subtractionmentioning

confidence: 99%

“…3 To compare, for example, with the conventions of [36], one should set √ 2κ → 1 in the formulae of the present paper, and make the following substitutions in equation (1.19) …”

Section: Bosonic Termsmentioning

confidence: 99%

R ⁴ , purified

Policastro¹,

Tsimpis²

2006

Class. Quantum Grav.

104

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We derive, using the pure-spinor formalism, the complete -including the fermions -fourpoint effective action of both type II superstrings to all orders in α ′ , at tree level in string loops. We find that, in the quartic-field approximation, the supergravity Lagrangian can be thought of as the tensor product, in a suitable sense, of two copies of the superYang-Mills Lagrangian in ten dimensions. The NS-NS three-form enters the supergravity Lagrangian through a modified connection with torsion. As a byproduct, we derive the complete, i.e. to all orders in the θ-expansion, closed-string vertex operator in a flat target-space background.

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“…The first construction of massive type IIA supergravity is due to Romans [13] and its main step is to give a mass to the two-form potential of standard IIA supergravity [14,15,16] through the replacement…”

Section: Massive Iia Supergravitymentioning

confidence: 99%

Massive type IIA supergravity and E₁₀

Henneaux

Jamsin²,

Kleinschmidt

et al. 2009

Fortschritte der Physik

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In this talk we investigate the symmetry under E10 of Romans' massive type IIA supergravity. We show that the dynamics of a spinning particle in a non-linear sigma model on the coset space E10/K(E10) reproduces the bosonic and fermionic dynamics of massive IIA supergravity, in the standard truncation. In particular, we identify Romans' mass with a generator of E10 that is beyond the realm of the generators of E10 considered in the eleven-dimensional analysis, but using the same, underformed sigma model. As a consequence, this work provides a dynamical unification of the massless and massive versions of type IIA supergravitiy inside E10.

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N=2supergravity in ten dimensions

Abstract: We construct the complete Lagrangian of extended supergravity in ten dimensions by dimensional reduction of the eleven-dimensional theory. We find a compactification of the D = 10 model to the D =4 model with internal manifold M4(compact )%S2.

Cited by 137 publications

References 27 publications

Probing the hydrodynamic limit of (super)gravity

Probing the hydrodynamic limit of (super)gravity

R ⁴ , purified

Massive type IIA supergravity and E₁₀

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N=2supergravity in ten dimensions

Abstract: We construct the complete Lagrangian of extended supergravity in ten dimensions by dimensional reduction of the eleven-dimensional theory. We find a compactification of the D = 10 model to the D =4 model with internal manifold M4(compact )%S2.

Cited by 137 publications

References 27 publications

Probing the hydrodynamic limit of (super)gravity

Probing the hydrodynamic limit of (super)gravity

R 4 , purified

Massive type IIA supergravity and E10

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R ⁴ , purified

Massive type IIA supergravity and E₁₀