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Stationary axisymmetric spacetimes with a conformally coupled scalar field

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arxiv 1412.3539 v2 pith:I5CEU57M submitted 2014-12-11 gr-qc hep-th

Stationary axisymmetric spacetimes with a conformally coupled scalar field

classification gr-qc hep-th
keywords axisymmetricconformallycoupledfieldscalarspacetimesstationaryaddition
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Solution generating techniques for general relativity with a conformally (and minimally) coupled scalar field are pushed forward to build a wide class of asymptotically flat, axisymmetric and stationary spacetimes continuously connected to Kerr. This family contains, amongst other things, rotating extensions of the Bekenstein black hole and also its angular and mass multipolar generalisations. Further addition of NUT charge is also discussed.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. (Super-)renormalizable hairy meronic black holes

    hep-th 2026-04 unverdicted novelty 6.0

    Analytical black hole solutions are constructed in Einstein-Maxwell-Yang-Mills theory with conformally coupled scalars, generalizing MTZ and AC solutions by including non-Abelian gauge fields determined by horizon curvature.

  2. Black holes in rotating, electromagnetic backgrounds and topological Kerr-Newman-NUT spacetimes

    gr-qc 2026-04 unverdicted novelty 6.0

    Essentially all known analytical exact single black hole solutions in four-dimensional Einstein-Maxwell theory belong to the accelerating Kerr-Newman-NUT family placed in backgrounds that are subcases of the conjugate...

  3. (Super-)renormalizable hairy meronic black holes

    hep-th 2026-04 unverdicted novelty 5.0

    Analytical construction of hairy meronic black holes in 4D Einstein-Maxwell-Yang-Mills with conformally coupled scalar, generalizing MTZ and AC solutions via non-Abelian fields and (super-)renormalizable terms.

  4. A new rotating axionic AdS$_4$ black hole dressed with a scalar field

    hep-th 2025-04 unverdicted novelty 4.0

    A new axionically charged rotating AdS4 black hole solution with scalar field is presented, defined by a structural function and parameters, with thermodynamics derived via Euclidean method satisfying the first law.