2019
DOI: 10.48550/arxiv.1904.05361
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Black Holes and (0,4) SCFTs from Type IIB on K3

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Cited by 7 publications
(11 citation statements)
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“…B The Dibitetto-Petri flow in minimal N = 1 7d supergravity The solution discussed in section 6 was obtained in [6] taking the following ansatz: ds 2 7 = e 2U (r) ds 2 (AdS 3 ) + e 2V (r) dr 2 + e 2W (r) ds 2 (S 3 ), X = X(r), B In these expressions g and h are the gauge coupling of the vector fields 17 and the topological mass of the 3-form potential, respectively, of minimal N = 1 7d supergravity.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…B The Dibitetto-Petri flow in minimal N = 1 7d supergravity The solution discussed in section 6 was obtained in [6] taking the following ansatz: ds 2 7 = e 2U (r) ds 2 (AdS 3 ) + e 2V (r) dr 2 + e 2W (r) ds 2 (S 3 ), X = X(r), B In these expressions g and h are the gauge coupling of the vector fields 17 and the topological mass of the 3-form potential, respectively, of minimal N = 1 7d supergravity.…”
Section: Discussionmentioning
confidence: 99%
“…This provides a new scenario in which 2d (0,4) CFTs appear in string theory. 2d (0,4) CFTs play a key role in the microscopical description of 5d black holes with AdS 3 ×S 2 near horizon geometries [12][13][14][15][16][17]. In string theory they can be realised in D1-D5-KK systems [18][19][20][21] and D1-D5-D9 systems [22].…”
Section: Introductionmentioning
confidence: 99%
“…Conversely v, w are only linear functions away from localised sources -globally they need only be piecewise linear provided that the resulting δ-functions appearing in their second derivatives gives rise to a source corrected Bianchi identity, and this source is calibrated. Given the form of this expression it might be tempting to interpret a shift in v as coincident D8-D6 and D4-D2 bound states -however such configurations fail to obey the calibration condition discussed in the previous section at generic points along the interval -so cannot be used to glue solutions together without breaking supersymmetry 22 . Shifts in w on the other hand are different and give rise to something new.…”
Section: Towards Global Solutions With Defects From Section 34mentioning
confidence: 99%
“…These describe the near horizon limit of D1 and D5 branes intersecting with KKmonopoles [12][13][14][15] or D9-branes [16]. These systems play a prominent role in the microscopical description of five dimensional black holes [17][18][19][20][21][22]. 2d (4,0) CFTs are also central in the description of self-dual strings in 6d (1,0) CFTs, realised in M and F theory [23][24][25][26][27][28].…”
Section: Introductionmentioning
confidence: 99%
“…This line of research remains to be further exploited. See [81,82,83]. In particular it would be interesting to apply exact calculational techniques (see [84]) to the new classes of solutions, since this would provide for a deeper understanding of the IR regime of the different theories.…”
Section: Discussionmentioning
confidence: 99%