Relevant bibliographies by topics / Black hole physics

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Black hole physics'

Author: Grafiati
Published: 4 June 2021
Last updated: 25 July 2025

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Journal articles on the topic "Black hole physics"

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Zakharov, Aleksandr F. "Black hole physics." Physics-Uspekhi 42, no. 9 (1999): 947–51. http://dx.doi.org/10.1070/pu1999v042n09abeh000651.

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Zakharov, A. F. "Black hole physics." Uspekhi Fizicheskih Nauk 169, no. 9 (1999): 1041. http://dx.doi.org/10.3367/ufnr.0169.199909h.1041.

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Carballo-Rubio, Raúl, Francesco Di Filippo, Stefano Liberati, et al. "Towards a non-singular paradigm of black hole physics." Journal of Cosmology and Astroparticle Physics 2025, no. 05 (2025): 003. https://doi.org/10.1088/1475-7516/2025/05/003.

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Abstract The study of regular black holes and black hole mimickers as alternatives to standard black holes has recently gained significant attention, driven both by the need to extend general relativity to describe black hole interiors, and by recent advances in observational technologies. Despite considerable progress in this field, significant challenges remain in identifying and characterizing physically well-motivated classes of regular black holes and black hole mimickers. This paper provides an overview of these challenges, and outlines some of the promising research directions — as disc
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Voss, D. "PHYSICS: Black Hole Encryption." Science 311, no. 5767 (2006): 1525a. http://dx.doi.org/10.1126/science.311.5767.1525a.

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VISSER, MATT. "HAWKING RADIATION: A PARTICLE PHYSICS PERSPECTIVE." Modern Physics Letters A 08, no. 18 (1993): 1661–70. http://dx.doi.org/10.1142/s0217732393001409.

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It has recently become fashionable to regard black holes as elementary particles. By taking this suggestion reasonably seriously it is possible to cobble together an elementary particle physics based on estimate for the decay rate (black hole) i → (black hole) f+ (massless quantum) . This estimate of the spontaneous emission rate contains two free parameters which may be fixed by demanding that the high energy end of the spectrum of emitted quanta match a black body spectrum at the Hawking temperature. The calculation, though technically trivial, has important conceptual implications: (1) The
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Abramovsky. "Abramovsky—Gribov—Kancheli Theorem in the Physics of Black Holes." Physics 1, no. 2 (2019): 253–70. http://dx.doi.org/10.3390/physics1020020.

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The proof of the Abramovsky—Gribov—Kancheli (AGK) theorem for black hole physics is given. Based on the AGK relations, a formula for the luminosity of a black hole as a function of the mass of the black hole is derived. The correspondence to experimental data is considered. It is shown that the black holes of the galaxies NGC3842 and NGC4889 do not differ from those of the other galaxies.
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Sims, Christopher. "Analogous Black Holes in Type-III Dirac Semimetal Ni3In2X2 (X = S, Se)." Crystals 13, no. 5 (2023): 847. http://dx.doi.org/10.3390/cryst13050847.

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Black holes are objects that have a large mass and curve space time, characterized by their event horizon and singularity. Recently, an interesting concept of analogous black holes has emerged in the field of condensed matter physics. In this work, the possibility of realizing analogous black holes in topological material is Ni3In2X2 (X = S, Se) discussed. This work shows that the type-III Dirac cones of the material can lead to the emergence of an event horizon and the formation of a black hole-like region near the Dirac point. In addition, the possible experimental signatures of such a syste
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Nasution, Budiman, Winsyahputra Ritonga, Ruben Cornelius Siagian, et al. "Physics Visualization of Schwarzschild Black Hole through Graphic Representation of the Regge-Wheeler Equation using R-Studio Approach." Sainmatika: Jurnal Ilmiah Matematika dan Ilmu Pengetahuan Alam 20, no. 1 (2023): 8–24. http://dx.doi.org/10.31851/sainmatika.v20i1.11845.

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This study aims to visualize the vibrations of black holes using the Regge-Wheeler equation in Cartesian coordinates. Black holes are astrophysical objects with extremely strong gravity, and understanding the vibrations around them provides insights into the nature and structure of black holes. The Regge-Wheeler equation is used to model these vibrations. In this study, the goal is to generate visual images that visualize the vibrations of black holes, including their frequencies, amplitudes, and possible vibration modes. Complex mathematical and computational methods were employed to create t
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Altas, E., and B. Tekin. "Basics of Apparent horizons in black hole physics." Journal of Physics: Conference Series 2191, no. 1 (2022): 012002. http://dx.doi.org/10.1088/1742-6596/2191/1/012002.

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Abstract 1Event Horizon, a null hypersurface defining the boundary of the black hole region of a spacetime, is not particularly useful for evolving black holes since it is non-local in time. Instead, one uses the more tangible concept of Apparent Horizon for dynamical black holes out there in the sky that do all sorts of things: evolve, merge and feed on the environment. Event Horizon, being a gauge-independent, global property of the total spacetime is easy to define and locate in the stationary case; on the other hand, Apparent Horizon depends on the embedding of the surface in spacetime and
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Aste, Andreas, and Dirk Trautmann. "Radial fall of a test particle onto an evaporating black hole." Canadian Journal of Physics 83, no. 10 (2005): 1001–6. http://dx.doi.org/10.1139/p05-058.

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A test particle falling onto a classical black hole crosses the event horizon and ends up in the singularity within finite eigentime. In the "more realistic" case of a "classical" evaporating black hole, an observer falling onto a black hole observes a sudden evaporation of the hole. This illustrates the fact that the discussion of the classical process, commonly found in the literature, may become obsolete when the black hole has a finite lifetime. The situation is basically the same for more complex cases, for example, where a particle collides with two merging black holes. It should be poin
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Dissertations / Theses on the topic "Black hole physics"

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Ahmadi, Morteza, and University of Lethbridge Faculty of Arts and Science. "Aspects of black hole physics." Thesis, Lethbridge, Alta. : University of Lethbridge, Faculty of Arts and Science, 2006, 2006. http://hdl.handle.net/10133/386.

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In this thesis, aspects of the physics of black holes are reviewed and new results in black hole thermodynamics are presented. First, general black hole solutions of Einstein’s equations of general relativity are mentioned and a proof of conservation law of energy and momentum in general relativity is presented. Aspects of the laws of black hole mechanics and Hawking radiation are then studied. Two proposals which attempt to explain the origin of black hole entropy (the brick wall model and entanglement entropy) are then discussed. Finally, some recent work related to the possible production a
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Chung, Hyeyoun. "Exploring Black Hole Dynamics." Thesis, Harvard University, 2014. http://nrs.harvard.edu/urn-3:HUL.InstRepos:14226081.

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This thesis explores the evolution of different types of black holes, and the ways in which black hole dynamics can be used to answer questions about other physical systems. We first investigate the differences in observable gravitational effects between a four-dimensional Randall-Sundrum (RS) braneworld universe compared to a universe without the extra dimension, by considering a black hole solution to the braneworld model that is localized on the brane. When the brane has a negative cosmological constant, then for a certain range of parameters for the black hole, the intersection of the bl
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Luna, Raimon. "New Strategies for Black Hole Physics." Doctoral thesis, Universitat de Barcelona, 2020. http://hdl.handle.net/10803/669583.

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In this thesis we apply new approaches and develop new techniques to address various issues related to fundamental aspects of modern gravitational theory and black holes. We study the behavior of black branes in the large D approximation, that is, we consider a space with a very large number of dimensions. This approach allows us to obtain a set of very simple equations that capture many of the physical phenomena of gravity. This technique uses the fact that the gravitational field around a massive object decays faster the higher the dimension, so when you take the very large D limit it bec
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Pidokrajt, Narit. "Information geometries in black hole physics." Doctoral thesis, Stockholms universitet, Fysikum, 2009. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-29365.

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In this thesis we aim to develop new perspectives on the statistical mechanics of black holes using an information geometric approach (Ruppeiner and Weinhold geometry). The Ruppeiner metric is defined as a Hessian matrix on a Gibbs surface, and provides a geometric description of thermodynamic systems in equilibrium. This Ruppeiner geometry exhibits physically suggestive features; a flat Ruppeiner metric for systems with no interactions i.e. the ideal gas, and curvature singularities signaling critical behavior(s) of the system. We construct a flatness theorem based on the scaling property of
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Chambers, Chris M. "Classical aspects of black hole physics." Thesis, University of Newcastle Upon Tyne, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.294892.

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Zhu, Yucong. "The Bright Side of Black Holes: Radiation From Black Hole Accretion Disks." Thesis, Harvard University, 2015. http://nrs.harvard.edu/urn-3:HUL.InstRepos:17463143.

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An understanding of radiation is paramount for connecting observations of accretion disks with the theory of black holes. In this thesis, we explore via radiative transfer postprocessing calculations the observational signatures of black holes. We investigate disk spectra by analyzing general relativistic magnetohydrodynamic (GRMHD) simulations of accretion disks. For the most part there are no surprises -- the resulting GRMHD spectrum is very close to the analytic Novikov & Thorne (1973) prediction from decades past, except for a small modification in the case of spinning black holes, whic
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O'Sullivan, Stephen Gerard. "Making better binary models and modeling distorted black holes using black hole perturbation theory." Thesis, Massachusetts Institute of Technology, 2015. http://hdl.handle.net/1721.1/99297.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Physics, 2015.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references.<br>In this thesis, I discuss the application and development of black hole perturbation theory both from an observational standpoint via gravitational waves and also tidal distortions of black hole horizons. The promise of gravitational wave astronomy depends on our ability to accurately model gravitational wave signals from astrophysical sources. This requires large numbers of accurate theoretical template waveforms spanning large
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Sung, Shih-Ta. "Black hole entropy and models." Thesis, Durham University, 1997. http://etheses.dur.ac.uk/4677/.

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No universally accepted statistical explanation of black hole entropy exists up to now, therefore, it is worth another try. Admittedly, black hole entropy does not have to have a statistical origin. If the "black hole entropy" is called "black hole index" instead, someone might be lured to give it an economic explanation. Nonetheless, the only way to justify one's claim about the statistical origin of black hole entropy is to compute it statistically. This is the motivation for the construction of black hole models. In chapter 1, I first review the four laws of classical black hole mechanics w
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Kolishetty, Kiran. "Quantum properties of black hole." Thesis, Lancaster University, 2014. http://eprints.lancs.ac.uk/71783/.

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In this research report I would like to present some of the results obtained based on the published research, it is on the analogue model of Bose Einstein condensate of gravitons. In my investigation with different approach I could reach similar conclusion for Schwarzschild radius which is derived for Bose Einstein condensate of N-gravitons . I could calculate the pressure inside the condensed black hole. It is found that the Bogoliubov dispersion relation for the elementary excitations of the weakly-interacting N-gravitons is shown to hold for the case of the weakly-interacting Graviton gas o
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Sidhu, Steve. "Conformal field theory and black hole physics." Thesis, Lethbridge, Alta. : University of Lethbridge, Dept. of Physics and Astronomy, c2012, 2012. http://hdl.handle.net/10133/3109.

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This thesis reviews the use of 2-dimensional conformal field theory applied to gravity, specifically calculating Bekenstein-Hawking entropy of black holes in (2+1) dimensions. A brief review of general relativity, Conformal Field Theory, energy extraction from black holes, and black hole thermodynamics will be given. The Cardy formula, which calculates the entropy of a black hole from the AdS/CFT duality, will be shown to calculate the correct Bekenstein-Hawking entropy of the static and rotating BTZ black holes. The first law of black hole thermodynamics of the static, rotating, and charged-r
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Books on the topic "Black hole physics"

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Venzo, De Sabbata, Zhang Zhenjiu, North Atlantic Treaty Organization. Scientific Affairs Division., and NATO Advanced Study Institute on Black Hole Physics (1991 : Erice, Italy), eds. Black hole physics. Kluwer Academic Publishers, 1992.

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Frolov, Valeri P., and Igor D. Novikov. Black Hole Physics. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5139-9.

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Sabbata, Venzo, and Zhenjiu Zhang, eds. Black Hole Physics. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2420-1.

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Grumiller, Daniel, and Mohammad Mehdi Sheikh-Jabbari. Black Hole Physics. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-10343-8.

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Sabbata, Venzo. Black Hole Physics. Springer Netherlands, 1992.

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service), SpringerLink (Online, ed. Black Hole Gravitohydromagnetics. Springer-Verlag Berlin Heidelberg, 2009.

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Punsly, Brian. Black Hole Gravitohydromagnetics. Springer Berlin Heidelberg, 2001.

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Andrei, Zelnikov, ed. Introduction to black hole physics. Oxford University Press, USA, 2011.

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D, Novikov I., ed. Black hole physics: Basic concepts and new developments. Kluwer, 1998.

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1966-, Falcke Heino, and Hehl F. W. 1937-, eds. The Galactic black hole: Lectures on general relativity and astrophysics. Institute of Physics Pub., 2003.

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Book chapters on the topic "Black hole physics"

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Romero, Gustavo E., and Gabriela S. Vila. "Black Hole Physics." In Introduction to Black Hole Astrophysics. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-39596-3_3.

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Lüst, Dieter, and Ward Vleeshouwers. "Rotating Black Holes and Black Hole Mechanics." In SpringerBriefs in Physics. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-10919-6_10.

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Lüst, Dieter, and Ward Vleeshouwers. "Black Hole Thermodynamics." In SpringerBriefs in Physics. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-10919-6_12.

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Novikov, Igor D., and Valery P. Frolov. "Rotating Black Hole." In Physics of Black Holes. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-017-2651-1_4.

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Novikov, Igor D., and Valery P. Frolov. "Black-Hole Electrodynamics." In Physics of Black Holes. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-017-2651-1_7.

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Frolov, Valeri P., and Igor D. Novikov. "Black hole Perturbations." In Fundamental Theories of Physics. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5139-9_4.

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Frolov, Valeri P., and Igor D. Novikov. "Black Hole Electrodynamics." In Fundamental Theories of Physics. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5139-9_8.

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Zhang, Zhenjiu. "Physics of Black Holes: Classical, Quantum and Astrophysical." In Black Hole Physics. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2420-1_1.

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Ching, Chengrui, Tsohsiu Ho, Yiren Wang, and Jing Yao. "Possible Multi-Explosions of Supernovae and Induced Gravitational Collapse." In Black Hole Physics. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2420-1_10.

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Bergmann, Peter G. "Concluding Remarks." In Black Hole Physics. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2420-1_11.

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Conference papers on the topic "Black hole physics"

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Mammadova, Tunzala. "Prognosing How Time Passes in a Black Hole: A Study in Physics and Cosmology." In IAF Microgravity Sciences and Processes Symposium, Held at the 75th International Astronautical Congress (IAC 2024). International Astronautical Federation (IAF), 2024. https://doi.org/10.52202/078356-0007.

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Bilic, Neven. "Black-Hole Phenomenology." In School on Particle Physics, Gravity and Cosmology. Sissa Medialab, 2007. http://dx.doi.org/10.22323/1.034.0004.

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Matzner, Richard A. "Designing a 2 black hole code." In Computational quantum physics. AIP, 1992. http://dx.doi.org/10.1063/1.42616.

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Ben Achour, Jibril, and Karim Noui. "Analytical continuation of black hole entropy in Loop Quantum Gravity: Lessons from black hole thermodynamics." In Frontiers of Fundamental Physics 14. Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.224.0158.

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Lambert, Pierre-Henry. "Introduction to Black Hole evaporation." In Ninth Modave Summer School in Mathematical Physics. Sissa Medialab, 2014. http://dx.doi.org/10.22323/1.201.0001.

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Tejeiro-Sarmiento, Juan Manuel. "Black Hole Entanglement Entropy." In A CENTURY OF RELATIVITY PHYSICS: ERE 2005; XXVIII Spanish Relativity Meeting. AIP, 2006. http://dx.doi.org/10.1063/1.2218196.

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Bianchi, Eugenio. "Last gasps of a black hole." In Frontiers of Fundamental Physics 14. Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.224.0035.

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Lemos, José P. S., Vilson T. Zanchin, Carlos Herdeiro, and Roger Picken. "New regular black hole solutions." In XIX INTERNATIONAL FALL WORKSHOP ON GEOMETRY AND PHYSICS. AIP, 2011. http://dx.doi.org/10.1063/1.3599140.

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Hooft, Gerard 't. "THE BLACK HOLE INFORMATION PROBLEM." In Proceedings of the International School of Subnuclear Physics. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812708427_0008.

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Marrani, Alessio. "Non-Linear Invariance of Black Hole Entropy." In The European Physical Society Conference on High Energy Physics. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.314.0543.

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Reports on the topic "Black hole physics"

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Balachandran, A. P., A. Momen, and L. Chandar. Edge states in gravity and black hole physics. Office of Scientific and Technical Information (OSTI), 1995. http://dx.doi.org/10.2172/176797.

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