Supersymmetric backgrounds and black holes in N = 1 , 1 $$ \mathcal{N}=\left(1,\;1\right) $$ cosmological new massive supergravity

Alkaç, Gökhan; Basanisi, Luca; Bergshoeff, Eric; Devecioğlu, Deniz Olgu; Ozkan, Mehmet

doi:10.1007/jhep10(2015)141

Cited by 7 publications

(24 citation statements)

References 40 publications

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“…only in GMG and not in NMG or TMG. Additionally, we also find some solutions that were overlooked in earlier works [17,18]. We conclude in section 5 with some comments and future directions.…”

Section: Conditionsmentioning

confidence: 75%

“…Furthermore, if S is a real constant one finds that supersymmetry actually requires the vector field to vanish and the Killing spinor becomes a constant spinor [17,18]. Now, we…”

Section: The Null Killing Vectormentioning

confidence: 88%

“…The limit m 2 → ∞ corresponds to N = (1, 1) TMG and the limit µ → ∞ corresponds to N = (1, 1) NMG models. Their supersymmetric solutions were studied in [17] and [18], respectively. The model can be truncated to N = 1 GMG [10,11] by setting the vector field V and the imaginary part of the scalar field, i.e.…”

Section: N = (1 1) General Massive Supergravitymentioning

confidence: 99%

“…A big advantage of working with off-shell supergravities is that such an analysis remains valid for any extension of the model, only field equations change. Later, supersymmetric solutions of N = (1, 1) NMG were examined in [18] and it was found that some additional backgrounds are allowed compared to N = (1, 1) TMG, such as static Lifshitz spacetime. We will show that for N = (1, 1) GMG even more configurations appear such as stationary Lifshitz spacetime and a timelike warped AdS with no restriction on the norm of the warping.…”

Section: Introductionmentioning

confidence: 99%

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Supersymmetric solutions of N=(1,1) general massive supergravity

2018

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We construct supersymmetric solutions of three-dimensional N ¼ ð1; 1Þ general massive supergravity (GMG). Solutions with a null Killing vector are, in general, pp-waves. We identify those that appear at critical points of the model, some of which do not exist in N ¼ ð1; 1Þ new massive supergravity (NMG). In the timelike case, we find that many solutions are common with NMG, but there is a new class that is genuine to GMG, two members of which are stationary Lifshitz and timelike squashed AdS spacetimes. We also show that in addition to the fully supersymmetric AdS vacuum, there is a second AdS background with a nonzero vector field that preserves 1=4 supersymmetry.

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Section: Conditionsmentioning

confidence: 75%

“…Furthermore, if S is a real constant one finds that supersymmetry actually requires the vector field to vanish and the Killing spinor becomes a constant spinor [17,18]. Now, we…”

Section: The Null Killing Vectormentioning

confidence: 88%

Section: N = (1 1) General Massive Supergravitymentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

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Supersymmetric solutions of N=(1,1) general massive supergravity

2018

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“…been found in [24][25][26]. In this paper, we are going to consider the N = (1, 1) supersymmetrization of GMG.…”

Section: Jhep04(2018)105mentioning

confidence: 99%

Critical $$ \mathcal{N} $$ = (1, 1) general massive supergravity

Deger

Moutsopoulos

Rosseel

2018

J. High Energ. Phys.

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In this paper we study the supermultiplet structure of N = (1, 1) General Massive Supergravity at non-critical and critical points of its parameter space. To do this, we first linearize the theory around its maximally supersymmetric AdS 3 vacuum and obtain the full linearized Lagrangian including fermionic terms. At generic values, linearized modes can be organized as two massless and 2 massive multiplets where supersymmetry relates them in the standard way. At critical points logarithmic modes appear and we find that in three of such points some of the supersymmetry transformations are noninvertible in logarithmic multiplets. However, in the fourth critical point, there is a massive logarithmic multiplet with invertible supersymmetry transformations.

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3D supergravity from wrapped M5-branes

Karndumri

Colgáin

2016

J. High Energ. Phys.

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Through consistent Kaluza-Klein reduction, we construct 3D N = 2 gauged supergravities corresponding to twisted compactifications of M5-branes on a product of constant curvature Riemann surfaces, including Kähler-Einstein four-manifolds. We extend the reduction to fermionic supersymmetry variations in order to determine the 3D Killing spinor equations and classify all timelike supersymmetric solutions. As a by-product, we identify an infinite class of new supersymmetric warped AdS 3 (Gödel) and warped dS 3 solutions. Moreover, we show that the superpotential T encodes the central charge and R symmetry of the dual N = (0, 2) SCFTs in the large N limit. We demonstrate that the R symmetry matches the canonical U(1) isometry from existing classifications of supersymmetric AdS 3 solutions to 11D supergravity with N = (0, 2) supersymmetry.

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Supersymmetric backgrounds and black holes in N = 1 , 1 $$ \mathcal{N}=\left(1,\;1\right) $$ cosmological new massive supergravity

Cited by 7 publications

References 40 publications

Supersymmetric solutions of N=(1,1) general massive supergravity

Supersymmetric solutions of N=(1,1) general massive supergravity

Critical $$ \mathcal{N} $$ = (1, 1) general massive supergravity

3D supergravity from wrapped M5-branes

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