Miok Park
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Miok Park has a total of 3 co-authors. Here are the top co-authors by number of shared publications:
- Robert B. Mann
University of Waterloo
6 shared publications - Paul L. McGrath
Department of Physics and Astronomy University of Waterloo N2L 3G1 Waterloo Ontario Canada
2 shared publications - Sean Stotyn
Department of Physics and Astronomy Faculty of Science University of Calgary 2500 University Drive NW T2N 1N4 Calgary AB Canada
2 shared publications
Latest Publications
- 1 August 2013
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2013 (8) , 1-38
Deformations of Lifshitz holography with the Gauss-Bonnet term in (n + 1) dimensions
- 1 August 2013
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2013 (8) , 1-38
Deformations of Lifshitz holography with the Gauss-Bonnet term in (n + 1) dimensions
- 19 December 2012
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2012 (12) , 1-29
Holographic renormalization of asymptotically flat gravity
- 19 December 2012
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2012 (12) , 1-29
Holographic renormalization of asymptotically flat gravity
- Open Access
Holographic Renormalization of Asymptotically Flat Gravity
We compute the boundary stress tensor associated with Mann-Marolf counterterm in asymptotic flat and static spacetime for cylindrical boundary surface as $r \rightarrow \infty$, and find that the form of the boundary stress tensor is the same as the hyperbolic boundary case in 4 dimensions, but has additional terms in higher than 4 dimensions. We find that these additional terms are impotent and do not contribute to conserved charges. We also check the conservation of the boundary stress tensor in a sense that $\mathcal{D}^a T_{ab} = 0$, and apply our result to the ($n+3$)-dimensional static black hole solution. As a result, we show that the stress boundary tensor with Mann-Marolf counterterm works well in standard boundary surfaces.Open AccessHolographic Renormalization of Asymptotically Flat Gravity
We compute the boundary stress tensor associated with Mann-Marolf counterterm in asymptotic flat and static spacetime for cylindrical boundary surface as $r \rightarrow \infty$, and find that the form of the boundary stress tensor is the same as the hyperbolic boundary case in 4 dimensions, but has additional terms in higher than 4 dimensions. We find that these additional terms are impotent and do not contribute to conserved charges. We also check the conservation of the boundary stress tensor in a sense that $\mathcal{D}^a T_{ab} = 0$, and apply our result to the ($n+3$)-dimensional static black hole solution. As a result, we show that the stress boundary tensor with Mann-Marolf counterterm works well in standard boundary surfaces. - 27 July 2012
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2012 (7) , 1-29
Deformations of Lifshitz holography in (n+1)-dimensions
- 27 July 2012
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2012 (7) , 1-29
Deformations of Lifshitz holography in (n+1)-dimensions
- 15 February 2012
- Published by American Physical Society (APS) in Physical Review D
- Vol. 85 (4)
Black holes and boson stars with one Killing field in arbitrary odd dimensions
We extend the recent D=5 results of Dias, Horowitz, and Santos by finding asymptotically anti\char21{}de~Sitter rotating black hole and boson star solutions with scalar hair in arbitrary odd spacetime dimension. Both the black holes and the boson stars are invariant under a single Killing vector field which corotates with the scalar field and, in the black hole case, is tangent to the generator of the horizon. Furthermore, we explicitly construct boson star and small black hole (r+$\ll${}$\ell${}) solutions perturbatively assuming a small amplitude for the scalar field, resulting in solutions valid for low energies and angular momenta. We find that just as in D=5, the angular momentum is primarily carried by the scalar field in D>5, whereas unlike D=5 the energy is also primarily carried by the scalar field in D>5; the thermodynamics in D=5 are governed by both the black hole and scalar field whereas in D>5 they are governed primarily by the scalar field alone. We focus on cataloging these solutions for the spacetime dimensions of interest in string theory, namely D=5,7,9,11.
- 15 February 2012
- Published by American Physical Society (APS) in Physical Review D
- Vol. 85 (4)
Black holes and boson stars with one Killing field in arbitrary odd dimensions
We extend the recent D=5 results of Dias, Horowitz, and Santos by finding asymptotically anti\char21{}de~Sitter rotating black hole and boson star solutions with scalar hair in arbitrary odd spacetime dimension. Both the black holes and the boson stars are invariant under a single Killing vector field which corotates with the scalar field and, in the black hole case, is tangent to the generator of the horizon. Furthermore, we explicitly construct boson star and small black hole (r+$\ll${}$\ell${}) solutions perturbatively assuming a small amplitude for the scalar field, resulting in solutions valid for low energies and angular momenta. We find that just as in D=5, the angular momentum is primarily carried by the scalar field in D>5, whereas unlike D=5 the energy is also primarily carried by the scalar field in D>5; the thermodynamics in D=5 are governed by both the black hole and scalar field whereas in D>5 they are governed primarily by the scalar field alone. We focus on cataloging these solutions for the spacetime dimensions of interest in string theory, namely D=5,7,9,11.
- Open Access
Black Holes and Boson Stars with One Killing Field in Arbitrary Odd Dimensions
We extend the recent D=5 results of Dias, Horowitz and Santos by finding asymptotically AdS rotating black hole and boson star solutions with scalar hair in arbitrary odd spacetime dimension. Both the black holes and the boson stars are invariant under a single Killing vector field which co-rotates with the scalar field and, in the black hole case, is tangent to the generator of the horizon. Furthermore, we explicitly construct boson star and small black hole ($r_+ \ll \ell$) solutions perturbatively assuming a small amplitude for the scalar field, resulting in solutions valid for low energies and angular momenta. We find that just as in D=5, the angular momentum is primarily carried by the scalar field in $D>5$, whereas unlike D=5 the energy is also primarily carried by the scalar field in $D>5$; the thermodynamics in D=5 are governed by both the black hole and scalar field whereas in $D>5$ they are governed primarily by the scalar field alone. We focus on cataloguing these solutions for the spacetime dimensions of interest in string theory, namely $D=5,7,9,11$.Open AccessBlack Holes and Boson Stars with One Killing Field in Arbitrary Odd Dimensions
We extend the recent D=5 results of Dias, Horowitz and Santos by finding asymptotically AdS rotating black hole and boson star solutions with scalar hair in arbitrary odd spacetime dimension. Both the black holes and the boson stars are invariant under a single Killing vector field which co-rotates with the scalar field and, in the black hole case, is tangent to the generator of the horizon. Furthermore, we explicitly construct boson star and small black hole ($r_+ \ll \ell$) solutions perturbatively assuming a small amplitude for the scalar field, resulting in solutions valid for low energies and angular momenta. We find that just as in D=5, the angular momentum is primarily carried by the scalar field in $D>5$, whereas unlike D=5 the energy is also primarily carried by the scalar field in $D>5$; the thermodynamics in D=5 are governed by both the black hole and scalar field whereas in $D>5$ they are governed primarily by the scalar field alone. We focus on cataloguing these solutions for the spacetime dimensions of interest in string theory, namely $D=5,7,9,11$.