Homogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole Spacetimes

This Dissertation covers three aspects of General Relativity: inequivalent Einstein metrics on Lie Group Manifolds, proving the Hoop Conjecture for Black Rings, and investigating ergoregions in magnetised black hole spacetimes. A number of analytical and numerical techniques are employed to that end...

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Main Author: Mujtaba, Abid Hasan
Other Authors: Pope, Christopher N
Format: Others
Published: 2013
Subjects:
Online Access:http://hdl.handle.net/1969.1/149262
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spelling ndltd-tamu.edu-oai-repository.tamu.edu-1969.1-1492622013-10-04T04:55:02ZHomogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole SpacetimesMujtaba, Abid HasanEinstein metricsSU(n)Hoop ConjectureBlack RingsErgoregionsKerr-NewmanMelvinThis Dissertation covers three aspects of General Relativity: inequivalent Einstein metrics on Lie Group Manifolds, proving the Hoop Conjecture for Black Rings, and investigating ergoregions in magnetised black hole spacetimes. A number of analytical and numerical techniques are employed to that end. It is known that every compact simple Lie Group admits a bi-invariant homogeneous Einstein metric. We use two ansatze to probe the existence of additional inequivalent Einstein metrics on the Lie Group SU (n). We provide an explicit construction of 2k + 1 and 2k inequivalent Einstein metrics on SU (2k) and SU (2k + 1) respectively. We prove the Hoop Conjecture for neutral and charged, singly and doubly rotating black rings. This allows one to determine whether a rotating mass distribution has an event horizon, that it is in fact a black ring. We investigate ergoregions in magnetised black hole spacetimes. We show that, in general, rotating charged black holes (Kerr-Newman) immersed in an external magnetic field have ergoregions that extend to infinity near the central axis unless we restrict the charge to q = amB and keep B below a maximal value. Additionally, we show that as B is increased from zero the ergoregion adjacent to the event horizon shrinks, vanishing altogether at a critical value, before reappearing and growing until it is no longer bounded as B becomes greater than the maximal value.Pope, Christopher NSezgin, ErginDutta, BhaskarFulling, Stephen2013-10-02T21:27:29Z2013-10-02T21:27:29Z2013-052013-01-09May 20132013-10-02T21:27:29ZThesistextapplication/pdfhttp://hdl.handle.net/1969.1/149262
collection NDLTD
format Others
sources NDLTD
topic Einstein metrics
SU(n)
Hoop Conjecture
Black Rings
Ergoregions
Kerr-Newman
Melvin
spellingShingle Einstein metrics
SU(n)
Hoop Conjecture
Black Rings
Ergoregions
Kerr-Newman
Melvin
Mujtaba, Abid Hasan
Homogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole Spacetimes
description This Dissertation covers three aspects of General Relativity: inequivalent Einstein metrics on Lie Group Manifolds, proving the Hoop Conjecture for Black Rings, and investigating ergoregions in magnetised black hole spacetimes. A number of analytical and numerical techniques are employed to that end. It is known that every compact simple Lie Group admits a bi-invariant homogeneous Einstein metric. We use two ansatze to probe the existence of additional inequivalent Einstein metrics on the Lie Group SU (n). We provide an explicit construction of 2k + 1 and 2k inequivalent Einstein metrics on SU (2k) and SU (2k + 1) respectively. We prove the Hoop Conjecture for neutral and charged, singly and doubly rotating black rings. This allows one to determine whether a rotating mass distribution has an event horizon, that it is in fact a black ring. We investigate ergoregions in magnetised black hole spacetimes. We show that, in general, rotating charged black holes (Kerr-Newman) immersed in an external magnetic field have ergoregions that extend to infinity near the central axis unless we restrict the charge to q = amB and keep B below a maximal value. Additionally, we show that as B is increased from zero the ergoregion adjacent to the event horizon shrinks, vanishing altogether at a critical value, before reappearing and growing until it is no longer bounded as B becomes greater than the maximal value.
author2 Pope, Christopher N
author_facet Pope, Christopher N
Mujtaba, Abid Hasan
author Mujtaba, Abid Hasan
author_sort Mujtaba, Abid Hasan
title Homogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole Spacetimes
title_short Homogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole Spacetimes
title_full Homogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole Spacetimes
title_fullStr Homogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole Spacetimes
title_full_unstemmed Homogeneous Einstein Metrics on SU(n) Manifolds, Hoop Conjecture for Black Rings, and Ergoregions in Magnetised Black Hole Spacetimes
title_sort homogeneous einstein metrics on su(n) manifolds, hoop conjecture for black rings, and ergoregions in magnetised black hole spacetimes
publishDate 2013
url http://hdl.handle.net/1969.1/149262
work_keys_str_mv AT mujtabaabidhasan homogeneouseinsteinmetricsonsunmanifoldshoopconjectureforblackringsandergoregionsinmagnetisedblackholespacetimes
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