{"arxiv_id":"1308.1439","incoming":{"papers":32,"sentences":72,"groups":[{"kind":"contests","label":"Contests it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1802.04733","title":"Supersymmetric objects in gauged supergravities","url":"/paper/1802.04733","section":"Gauging, $AdS$ Vacua and Near-Horizon Analysis","sentence":"In particular the method studying near-horizon geometries developed in [ref] for the case of symmetric special Kähler manifolds doesn't work in this case, since the model is neither symmetric nor homogeneous.","intent_p":0.56,"contests_p":0.77}]},{"kind":"method_or_tool","label":"Uses its method or tool","papers":4,"sentences":4,"quotes":[{"arxiv_id":"1507.05553","title":"BPS black holes in a non-homogeneous deformation of the stu model of $N=2$, $D=4$ gauged supergravity","url":"/paper/1507.05553","section":"Dyonic Fayet-Iliopoulos gaugings and near-horizon analysis","sentence":"Following the procedure described in [ref] [The equations [ref] are based on [ref] , with some misprints corrected.], the BPS equations in the near-horizon limit [ref] provide a set of equations for the variables ${R_1,R_2,λ^i}$ as functions of the gaugings $g_0,g^i$ and the charges $p^0,q_i$.In particular, since $R_2$ is directly related to the black hole entropy $S$, this yields an expression for $S$ in terms of the gaugings and charges.","intent_p":0.96,"contests_p":null},{"arxiv_id":"1312.2766","title":"Supersymmetric Black Holes in AdS4 from Very Special Geometry","url":"/paper/1312.2766","section":"$AdS_2×_g$: IR boundary conditions","sentence":"Assuming that these conditions are satisfied we can use the results of [ref] to analyze regular horizon geometries.","intent_p":0.94,"contests_p":null},{"arxiv_id":"1706.01823","title":"BPS black hole horizons from massive IIA","url":"/paper/1706.01823","section":"Motivation and outlook","sentence":"The classification of horizon configurations can be performed by virtue of the attractor mechanism [ref] which fixes the values of the scalars at the horizon in terms of the vector charges.","intent_p":0.8,"contests_p":null},{"arxiv_id":"1503.04686","title":"Quarter-BPS Black Holes in AdS$_4$-NUT from $N=2$ Gauged Supergravity","url":"/paper/1503.04686","section":"The Black Hole Ansatz","sentence":"Exactly as in [ref] , in this work our strategy is to consider sections $$ which come from a cubic prepotential and allow for dyonic gauge couplings.","intent_p":0.93,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":6,"sentences":6,"quotes":[{"arxiv_id":"1408.2831","title":"Static BPS Black Holes in AdS4 with General Dyonic Charges","url":"/paper/1408.2831","section":"Introduction","sentence":"For the STU-model in particular, this gives a five-dimensional solution space whereas the analysis of [ref] predicts that there should be a six-dimensional solution space.","intent_p":0.92,"contests_p":null},{"arxiv_id":"1409.6310","title":"Abelian Hypermultiplet Gaugings and BPS Vacua in N = 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