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Proof of a Null Penrose Conjecture U...
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ProQuest Information and Learning Co.
Proof of a Null Penrose Conjecture Using a New Quasi-local Mass.
Record Type:
Language materials, manuscript : Monograph/item
Title/Author:
Proof of a Null Penrose Conjecture Using a New Quasi-local Mass./
Author:
Roesch, Henri P.
Description:
1 online resource (172 pages)
Notes:
Source: Dissertation Abstracts International, Volume: 78-09(E), Section: B.
Contained By:
Dissertation Abstracts International78-09B(E).
Subject:
Mathematics. -
Online resource:
click for full text (PQDT)
ISBN:
9781369725384
Proof of a Null Penrose Conjecture Using a New Quasi-local Mass.
Roesch, Henri P.
Proof of a Null Penrose Conjecture Using a New Quasi-local Mass.
- 1 online resource (172 pages)
Source: Dissertation Abstracts International, Volume: 78-09(E), Section: B.
Thesis (Ph.D.)
Includes bibliographical references
In the theory of general relativity, the Penrose conjecture claims a lower bound for the mass of a spacetime in terms of the area of an outermost horizon, if one exists. In physical terms, this conjecture is a geometric formulation of the statement that the total mass of a spacetime is at least the mass of any black holes that are present, assuming non-negative energy density. For the geometry of light-rays emanating off of a black hole horizon (called a nullcone) the Penrose conjecture can be reformulated to the so-called Null Penrose Conjecture (NPC). In this thesis, we define an explicit quasi-local mass functional that is non-decreasing along all foliations (satisfying a convexity assumption) of nullcones. We use this new functional to prove the NPC under fairly generic conditions.
Electronic reproduction.
Ann Arbor, Mich. :
ProQuest,
2018
Mode of access: World Wide Web
ISBN: 9781369725384Subjects--Topical Terms:
527692
Mathematics.
Index Terms--Genre/Form:
554714
Electronic books.
Proof of a Null Penrose Conjecture Using a New Quasi-local Mass.
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Proof of a Null Penrose Conjecture Using a New Quasi-local Mass.
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In the theory of general relativity, the Penrose conjecture claims a lower bound for the mass of a spacetime in terms of the area of an outermost horizon, if one exists. In physical terms, this conjecture is a geometric formulation of the statement that the total mass of a spacetime is at least the mass of any black holes that are present, assuming non-negative energy density. For the geometry of light-rays emanating off of a black hole horizon (called a nullcone) the Penrose conjecture can be reformulated to the so-called Null Penrose Conjecture (NPC). In this thesis, we define an explicit quasi-local mass functional that is non-decreasing along all foliations (satisfying a convexity assumption) of nullcones. We use this new functional to prove the NPC under fairly generic conditions.
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2018
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click for full text (PQDT)
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