Evolution of Black Holes in Anti-de Sitter Spacetime and the Firewall Controversy PDF Download
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Author: Yen Chin Ong
Publisher: Springer
ISBN: 3662482703
Category : Science
Languages : en
Pages : 238
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Book Description
This thesis focuses on the recent firewall controversy surrounding evaporating black holes, and shows that in the best understood example concerning electrically charged black holes with a flat event horizon in anti-de Sitter (AdS) spacetime, the firewall does not arise. The firewall, which surrounds a sufficiently old black hole, threatens to develop into a huge crisis since it could occur even when spacetime curvature is small, which contradicts general relativity. However, the end state for asymptotically flat black holes is ill-understood since their curvature becomes unbounded. This issue is avoided by working with flat charged black holes in AdS. The presence of electrical charge is crucial since black holes inevitably pick up charges throughout their long lifetime. These black holes always evolve toward extremal limit, and are then destroyed by quantum gravitational effects. This happens sooner than the time required to decode Hawking radiation so that the firewall never sets in, as conjectured by Harlow and Hayden. Motivated by the information loss paradox, the author also investigates the possibility that “monster” configurations might exist, with an arbitrarily large interior bounded by a finite surface area. Investigating such an object in AdS shows that in the best understood case, such an object -- much like a firewall -- cannot exist.
Author: Yen Chin Ong
Publisher: Springer
ISBN: 3662482703
Category : Science
Languages : en
Pages : 238
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Book Description
This thesis focuses on the recent firewall controversy surrounding evaporating black holes, and shows that in the best understood example concerning electrically charged black holes with a flat event horizon in anti-de Sitter (AdS) spacetime, the firewall does not arise. The firewall, which surrounds a sufficiently old black hole, threatens to develop into a huge crisis since it could occur even when spacetime curvature is small, which contradicts general relativity. However, the end state for asymptotically flat black holes is ill-understood since their curvature becomes unbounded. This issue is avoided by working with flat charged black holes in AdS. The presence of electrical charge is crucial since black holes inevitably pick up charges throughout their long lifetime. These black holes always evolve toward extremal limit, and are then destroyed by quantum gravitational effects. This happens sooner than the time required to decode Hawking radiation so that the firewall never sets in, as conjectured by Harlow and Hayden. Motivated by the information loss paradox, the author also investigates the possibility that “monster” configurations might exist, with an arbitrarily large interior bounded by a finite surface area. Investigating such an object in AdS shows that in the best understood case, such an object -- much like a firewall -- cannot exist.
Author: Oleg Kupervasser
Publisher: Elsevier
ISBN: 012813318X
Category : Science
Languages : en
Pages : 308
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Book Description
Application of New Cybernetics in Physics describes the application of new cybernetics to physical problems and the resolution of basic physical paradoxes by considering external observer influence. This aids the reader in solving problems that were solved incorrectly or have not been solved. Three groups of problems of the new cybernetics are considered in the book: (a) Systems that can be calculated based on known physics of subsystems. This includes the external observer influence calculated from basic physical laws (ideal dynamics) and dynamics of a physical system influenced even by low noise (observable dynamics). (b) Emergent systems. This includes external noise from the observer by using the black box model (complex dynamics), external noise from the observer by using the observer’s intuition (unpredictable dynamics), defining boundaries of application of scientific methods for system behavior prediction, and the role of the observer’s intuition for unpredictable systems. (c) Methods for solution of basic physical paradoxes by using methods of the new cybernetics: the entropy increase paradox, Schrödinger’s cat paradox (wave package reduction in quantum mechanics), the black holes information paradox, and the time wormholes grandfather paradox. All of the above paradoxes have the same resolution based on the principles of new cybernetics. Indeed, even a small interaction of an observer with an observed system results in their time arrows’ alignment (synchronization) and results in the paradox resolution and appearance of the universal time arrow. Provides solutions to the basic physical paradoxes and demonstrates their practical actuality for modern physics Describes a wide class of molecular physics and kinetic problems to present semi-analytical and semi-qualitative calculations of solvation, flame propagation, and high-molecular formation Demonstrates the effectiveness in application to complex molecular systems and other many-component objects Includes numerous illustrations to support the text
Author: Robert B. Mann
Publisher: Springer
ISBN: 3319144960
Category : Science
Languages : en
Pages : 103
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Book Description
This book reflects the resurgence of interest in the quantum properties of black holes, culminating most recently in controversial discussions about firewalls. On the thermodynamic side, it describes how new developments allowed the inclusion of pressure/volume terms in the first law, leading to a new understanding of black holes as chemical systems, experiencing novel phenomena such as triple points and reentrant phase transitions. On the quantum-information side, the reader learns how basic arguments undergirding quantum complementarity have been shown to be flawed; and how this suggests that a black hole may surround itself with a firewall: a violent and chaotic region of highly excited states. In this thorough and pedagogical treatment, Robert Mann traces these new developments from their roots to our present-day understanding, highlighting their relationships and the challenges they present for quantum gravity.
Author: Uzair Hussain
Publisher:
ISBN:
Category :
Languages : en
Pages :
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Book Description
In this thesis we present projects that cover various topics in black hole physics. The central theme of the thesis is perturbation theory of black holes. The techniques developed to study the perturbations of spacetime allows us to explore and elucidate many other topics in gravitational physics. The recent discovery of gravitational waves provides strong evidence for the existence of black hole mergers. Using perturbation theory we study the problem of black hole mergers with an extreme mass ratio in an asymptotically at spacetime, and proceed to demonstrate how the event horizon and the apparent horizon of the larger black hole deform. In this thesis we also study problems concerning perturbation of black holes that are more theoretical in nature. In the context of the uid/gravity duality, we precisely establish the relationship between standard perturbation theory of spherically symmetric black holes i.e., the master equation, with near equilibrium dual uid perturbations on the boundary of asymptotically Anti de Sitter (AdS) black holes. By the use of this relationship and a numerical evolution of the master equation we argue for the existence of non-Newtonian uids in the uid/gravity duality. The last project concerns itself with a generalization of the first law of black hole mechanics to include five dimensional solutions of spacetime called solitons. We verify this law for spacetimes containing solitons.
Author: Hari Krishna Kunduri
Publisher:
ISBN:
Category : Black holes (Astronomy)
Languages : en
Pages : 518
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Book Description
Author: Henry Stoltenberg
Publisher:
ISBN: 9780355151992
Category :
Languages : en
Pages :
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Book Description
This dissertation covers work from three research projects relating to the physics before the start of inflation and information after the decay of a black hole. For the first project, we analyze the cosmological role of terminal vacua in the string theory landscape, and point out that existing work on this topic makes very strong assumptions about the properties of the terminal vacua. We explore the implications of relaxing these assumptions (by including "arrival'' as well as "departure'' terminals) and demonstrate that the results in earlier work are highly sensitive to their assumptionof no arrival terminals. We use our discussion to make some general points about tuning and initial conditions in cosmology. The second project is a discussion of the black hole information problem. Under certain conditions the black hole information puzzle and the (related) arguments that firewalls are a typical feature of blackholes can break down. We first review the arguments of Almheiri, Marolf, Polchinski and Sully (AMPS) favoring firewalls, focusing on entanglements in a simple toy model for a black hole and the Hawking radiation. By introducing a large and inaccessible system entangled with the black hole (representing perhaps a de Sitter stretched horizon or inaccessible part of a landscape) we show complementarity can be restored and firewalls can be avoided throughout the black hole's evolution. Under these conditions black holes do not have an "information problem''. We point out flaws in some of our earlier arguments that such entanglement might be generically present in some cosmological scenarios, and call out certain ways our picture may still be realized. The third project also examines the firewall argument. A fundamental limitation on the behavior of quantum entanglement known as "monogamy'' plays a key role in the AMPS argument. Our goal is to study and apply many-body entanglement theory to consider the entanglement among different parts of Hawking radiation and black holes. Using the multipartite entanglement measure called negativity, we identify an example which differs from the AMPS accounting of quantum entanglement and might eliminate the need for a firewall. Specifically, we constructed a toy model for black hole decay which has different entanglement behavior than that assumed by AMPS. We discuss the additional steps that would be needed to bring lessons from our toy model to our understanding of realistic black holes.
Author: M. Colpi
Publisher: CRC Press
ISBN: 1420012096
Category : Science
Languages : en
Pages : 482
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Book Description
Black holes are among the most mysterious objects that the human mind has been capable of imagining. As pure mathematical constructions, they are tools for exploiting the fundamental laws of physics. As astronomical sources, they are part of our cosmic landscape, warping space-time, coupled to the large-scale properties and life cycle of their host
Author: Paul V. Kreitler
Publisher: Nova Publishers
ISBN: 9781594544750
Category : Science
Languages : en
Pages : 198
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Book Description
A black hole is a point of extreme mass in spacetime with a radius, or event horizon, inside of which all electromagnetic radiation (including light) is trapped by gravity. A black hole is an extremely compact object, collapsed by gravity which has overcome electric and nuclear forces. It is believed that stars appreciably larger than the Sun, once they have exhausted all their nuclear fuel, collapse to form black holes: they are "black" because no light escapes their intense gravity. Material attracted to a black hole, though, gains enormous energy and can radiate part of it before being swallowed up. Some astronomers believe that enormously massive black holes exist in the centre of our galaxy and of other galaxies. This new book brings together leading research from throughout the world.
Author: Andrés Felipe Vargas Sánchez
Publisher:
ISBN:
Category :
Languages : en
Pages :
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Book Description
In this work, both extended phase space and holographic equipartition approaches are studied and employed to develop an exact Van der Waals description of nonrotating D = 4 SAdS black holes as an ensemble of spacetime atoms. After a possible micro- scopical interaction model is introduced, statistical mechanics techniques, with certain heuristic gravitational constraints, are used to derive the equation of state and the BekensteinHawking entropy. The procedure is generalized to the charged D = 4 SAdS black hole and to arbitrary D greater than or equal to 3 dimensions for the uncharged cases.
Author: Benjamin Lee Shepherd
Publisher:
ISBN:
Category :
Languages : en
Pages : 0
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