Owen Vaughan
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Owen Vaughan has a total of 10 co-authors. Here are the top co-authors by number of shared publications:
- Thomas Mohaupt
University of Liverpool
4 shared publications - David Errington
Department of Mathematical Sciences University of Liverpool Peach Street L69 7ZL Liverpool UK
2 shared publications - Paul Dempster
Seoul National University
2 shared publications - Vicente Cortés
Department of Mathematics and Center for Mathematical Physics, University of Hamburg, Hamburg, Germany
2 shared publications - Wafic A. Sabra
American University of Beirut
2 shared publications - Alessandra Gnecchi
INFN, Sezione di Padova
1 shared publication
Latest Publications
- Open Access
The para-HK/QK correspondence
We generalise the hyper-Kahler/quaternionic Kahler (HK/QK) correspondence to include para-geometries, and present a new concise proof that the target manifold of the HK/QK correspondence is quaternionic Kahler. As an application, we construct one-parameter deformations of the temporal and Euclidean supergravity c-map metrics and show that they are para-quaternionic Kahler.
Open AccessThe para-HK/QK correspondence
We generalise the hyper-Kahler/quaternionic Kahler (HK/QK) correspondence to include para-geometries, and present a new concise proof that the target manifold of the HK/QK correspondence is quaternionic Kahler. As an application, we construct one-parameter deformations of the temporal and Euclidean supergravity c-map metrics and show that they are para-quaternionic Kahler.
- Open Access
10D to 4D Euclidean Supergravity over a Calabi-Yau three-fold
We dimensionally reduce the bosonic sector of 10D Euclidean type IIA supergravity over a Calabi-Yau three-fold. The resulting theory describes the bosonic sector of 4D, N = 2 Euclidean supergravity coupled to vector- and hyper-multiplets. We show that the scalar target manifold of the vector-multiplets is projective special para-Kahler, and is therefore of split signature, whereas the target manifold of the hyper-multiplets is (positive-definite) quaternionic Kahler.
Open Access10D to 4D Euclidean Supergravity over a Calabi-Yau three-fold
We dimensionally reduce the bosonic sector of 10D Euclidean type IIA supergravity over a Calabi-Yau three-fold. The resulting theory describes the bosonic sector of 4D, N = 2 Euclidean supergravity coupled to vector- and hyper-multiplets. We show that the scalar target manifold of the vector-multiplets is projective special para-Kahler, and is therefore of split signature, whereas the target manifold of the hyper-multiplets is (positive-definite) quaternionic Kahler.
- Open Access
- 11 December 2015
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 33 (1) , 015010
10D to 4D Euclidean supergravity over a Calabi-Yau three-fold
We dimensionally reduce the bosonic sector of 10D Euclidean type IIA supergravity over a Calabi-Yau three-fold. The resulting theory describes the bosonic sector of 4D, Euclidean supergravity coupled to vector- and hyper-multiplets. We show that the scalar target manifold of the vector-multiplets is projective special para-Kähler, and is therefore of split signature, whereas the target manifold of the hyper-multiplets is (positive-definite) quaternionic Kähler.
- 11 December 2015
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 33 (1) , 015010
Open Access10D to 4D Euclidean supergravity over a Calabi-Yau three-fold
We dimensionally reduce the bosonic sector of 10D Euclidean type IIA supergravity over a Calabi-Yau three-fold. The resulting theory describes the bosonic sector of 4D, Euclidean supergravity coupled to vector- and hyper-multiplets. We show that the scalar target manifold of the vector-multiplets is projective special para-Kähler, and is therefore of split signature, whereas the target manifold of the hyper-multiplets is (positive-definite) quaternionic Kähler.
- Open Access
- 11 October 2015
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2015 (10) , 1-61
Special geometry of Euclidean supersymmetry IV: the local c-map
- 11 October 2015
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2015 (10) , 1-61
Open AccessSpecial geometry of Euclidean supersymmetry IV: the local c-map
- Open Access
Special Geometry of Euclidean Supersymmetry IV: the local c-map
We consider timelike and spacelike reductions of 4D, N = 2 Minkowskian and Euclidean vector multiplets coupled to supergravity and the maps induced on the scalar geometry. In particular, we investigate (i) the (standard) spatial c-map, (ii) the temporal c-map, which corresponds to the reduction of the Minkowskian theory over time, and (iii) the Euclidean c-map, which corresponds to the reduction of the Euclidean theory over space. In the last two cases we prove that the target manifold is para-quaternionic Kahler. In cases (i) and (ii) we construct two integrable complex structures on the target manifold, one of which belongs to the quaternionic and para-quaternionic structure, respectively. In case (iii) we construct two integrable para-complex structures, one of which belongs to the para-quaternionic structure. In addition we provide a new global construction of the spatial, temporal and Euclidean c-maps, and separately consider a description of the target manifold as a fibre bundle over a projective special Kahler or para-Kahler base.
Open AccessSpecial Geometry of Euclidean Supersymmetry IV: the local c-map
We consider timelike and spacelike reductions of 4D, N = 2 Minkowskian and Euclidean vector multiplets coupled to supergravity and the maps induced on the scalar geometry. In particular, we investigate (i) the (standard) spatial c-map, (ii) the temporal c-map, which corresponds to the reduction of the Minkowskian theory over time, and (iii) the Euclidean c-map, which corresponds to the reduction of the Euclidean theory over space. In the last two cases we prove that the target manifold is para-quaternionic Kahler. In cases (i) and (ii) we construct two integrable complex structures on the target manifold, one of which belongs to the quaternionic and para-quaternionic structure, respectively. In case (iii) we construct two integrable para-complex structures, one of which belongs to the para-quaternionic structure. In addition we provide a new global construction of the spatial, temporal and Euclidean c-maps, and separately consider a description of the target manifold as a fibre bundle over a projective special Kahler or para-Kahler base.
- Open Access
Non-extremal black hole solutions from the c-map
We construct new static, spherically symmetric non-extremal black hole solutions of four-dimensional ${\cal N}=2$ supergravity, using a systematic technique based on dimensional reduction over time (the c-map) and the real formulation of special geometry. For a certain class of models we actually obtain the general solution to the full second order equations of motion, whilst for other classes of models, such as those obtainable by dimensional reduction from five dimensions, heterotic tree-level models, and type-II Calabi-Yau compactifications in the large volume limit a partial set of solutions are found. When considering specifically non-extremal black hole solutions we find that regularity conditions reduce the number of integration constants by one half. Such solutions satisfy a unique set of first order equations, which we identify. Several models are investigated in detail, including examples of non-homogeneous spaces such as the quantum deformed $STU$ model. Though we focus on static, spherically symmetric solutions of ungauged supergravity, the method is adaptable to other types of solutions and to gauged supergravity.Open AccessNon-extremal black hole solutions from the c-map
We construct new static, spherically symmetric non-extremal black hole solutions of four-dimensional ${\cal N}=2$ supergravity, using a systematic technique based on dimensional reduction over time (the c-map) and the real formulation of special geometry. For a certain class of models we actually obtain the general solution to the full second order equations of motion, whilst for other classes of models, such as those obtainable by dimensional reduction from five dimensions, heterotic tree-level models, and type-II Calabi-Yau compactifications in the large volume limit a partial set of solutions are found. When considering specifically non-extremal black hole solutions we find that regularity conditions reduce the number of integration constants by one half. Such solutions satisfy a unique set of first order equations, which we identify. Several models are investigated in detail, including examples of non-homogeneous spaces such as the quantum deformed $STU$ model. Though we focus on static, spherically symmetric solutions of ungauged supergravity, the method is adaptable to other types of solutions and to gauged supergravity. - Open Access
- 11 May 2015
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2015 (5) , 1-57
Non-extremal black hole solutions from the c-map
- 11 May 2015
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2015 (5) , 1-57
Open AccessNon-extremal black hole solutions from the c-map
- Open Access
- 23 January 2014
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2014 (1) , 1-32
Rotating black holes in 4d gauged supergravity
- 23 January 2014
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2014 (1) , 1-32
Open AccessRotating black holes in 4d gauged supergravity