6,762 research outputs found

    Supersymmetric AdS5AdS_5 black holes and strings from 5D N=4N=4 gauged supergravity

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    We study supersymmetric AdS3×Σ2AdS_3\times \Sigma_2 and AdS2×Σ3AdS_2\times \Sigma_3 solutions, with Σ2=S2,H2\Sigma_2=S^2,H^2 and Σ3=S3,H3\Sigma_3=S^3,H^3, in five-dimensional N=4N=4 gauged supergravity coupled to five vector multiplets. The gauge groups considered here are U(1)×SU(2)×SU(2)U(1)\times SU(2)\times SU(2), U(1)×SO(3,1)U(1)\times SO(3,1) and U(1)×SL(3,R)U(1)\times SL(3,\mathbb{R}). For U(1)×SU(2)×SU(2)U(1)\times SU(2)\times SU(2) gauge group admiting two supersymmetric N=4N=4 AdS5AdS_5 vacua, we identify a new class of AdS3×Σ2AdS_3\times \Sigma_2 and AdS2×H3AdS_2\times H^3 solutions preserving four supercharges. Holographic RG flows describing twisted compactifications of N=2N=2 four-dimensional SCFTs dual to the AdS5AdS_5 vacua to the SCFTs in two and one dimensions dual to these geometries are numerically given. The solutions can also be interpreted as supersymmetric black strings and black holes in asymptotically AdS5AdS_5 spaces with near horizon geometries given by AdS3×Σ2AdS_3\times \Sigma_2 and AdS2×H3AdS_2\times H^3, respectively. These solutions broaden previously known black brane solutions including half-supersymmetric AdS5AdS_5 black strings recently found in N=4N=4 gauged supergravity. Similar solutions are also studied in non-compact gauge groups U(1)×SO(3,1)U(1)\times SO(3,1) and U(1)×SL(3,R)U(1)\times SL(3,\mathbb{R}).Comment: 35 pages, 12 figures, substantial extension of the results in arXiv:1811.01608, typos corrected, references adde

    On the (non)rigidity of the Frobenius Endomorphism over Gorenstein Rings

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    It is well-known that for a large class of local rings of positive characteristic, including complete intersection rings, the Frobenius endomorphism can be used as a test for finite projective dimension. In this paper, we exploit this property to study the structure of such rings. One of our results states that the Picard group of the punctured spectrum of such a ring RR cannot have pp-torsion. When RR is a local complete intersection, this recovers (with a purely local algebra proof) an analogous statement for complete intersections in projective spaces first given in SGA and also a special case of a conjecture by Gabber. Our method also leads to many simply constructed examples where rigidity for the Frobenius endomorphism does not hold, even when the rings are Gorenstein with isolated singularity. This is in stark contrast to the situation for complete intersection rings. Also, a related length criterion for modules of finite length and finite projective dimension is discussed towards the end.Comment: Minor changes in Example 2.2 and Theorem 2.9. Conjecture 1.2 was added

    New cosmological solutions from type II de-Sitter gaugings in 4D N=4N=4 gauged supergravity

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    In this work, which is a follow-up of arXiv:2102.06512, we document new cosmological solutions from four-dimensional N=4N=4 matter-coupled supergravity. The solutions smoothly interpolate between a dS2×S2dS_2\times S^2 spacetime at tt\rightarrow -\infty and a dS4dS_4 spacetime at t+t\rightarrow +\infty and arise from the second-order equations of motion. Unlike the previously reported solutions in arXiv:2102.06512 that involve the diagonal U(1)U(1) subgroup of both the electric and magnetic factors in the gauging, these solutions only require a single U(1)U(1) factor from either the electric or magnetic part. Two additional features of these solutions that distinguish them from the previously presented solutions are the nonvanishing value of the dilaton ϕ\phi and the fact that they are only admitted by the type II de-Sitter gauged theories.Comment: This is a follow-up work of arXiv:2102.0651
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