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Pseudogap in electron-doped cuprates as a thermal precursor to magnetism. [PDF]
Nat CommunKokkinis EK, Chubukov AV.
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Generating polarized amplified spontaneous emission at high symmetry points of square lattices. [PDF]
Microsyst NanoengWang T +6 more
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2014
This chapter is devoted to some physical properties of black holes, including a discussion of their thermodynamics, black hole laws, quantum effects, black hole magnetospheres, interiors, and singularities. The chapter opens with a discussion on the formation of black holes in astrophysical environments.
Gustavo E. Romero, Gabriela S. Vila
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This chapter is devoted to some physical properties of black holes, including a discussion of their thermodynamics, black hole laws, quantum effects, black hole magnetospheres, interiors, and singularities. The chapter opens with a discussion on the formation of black holes in astrophysical environments.
Gustavo E. Romero, Gabriela S. Vila
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Superradiance in Black Hole Physics
2015As discussed in the previous section, superradiance requires dissipation. The latter can emerge in various forms, e.g. viscosity, friction, turbulence, radiative cooling, etc. All these forms of dissipation are associated with some medium or some matter field that provides the arena for superradiance.
Richard Brito, Vitor Cardoso, Paolo Pani
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Two-dimensional black hole physics
Physical Review D, 1992Two-dimensional black hole solutions of string-motivated two-dimensional (2D) gravity are studied. It is shown that the main results of 4D black hole physics (such as the uniqueness theorems, mass formulas, and thermodynamical analogy) have their counterparts in the 2D case. The existence of static solutions describing black holes with tachyon hairs is
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1992
Physics of Black Holes: Classical. Quantum and Astrophysical.- Black Holes and Thermodynamics.- Thermodynamics and Black Holes.- Thermodynamics and Internal Dynamics of Black Holes: some recent developments.- Black-Hole Thermodynamics, Mass-Inflation, and Evaporation.- The central role of Spin in Black Hole Evaporation.- Mechanics and Equilibrium ...
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Physics of Black Holes: Classical. Quantum and Astrophysical.- Black Holes and Thermodynamics.- Thermodynamics and Black Holes.- Thermodynamics and Internal Dynamics of Black Holes: some recent developments.- Black-Hole Thermodynamics, Mass-Inflation, and Evaporation.- The central role of Spin in Black Hole Evaporation.- Mechanics and Equilibrium ...
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2020
General relativity predicts the existence of Black Holes. A Black Hole (BH) is a region of space into which matter has collapsed and out of which not even light may escape and hence the term “black”. It partitions space into an inner region which is bounded by a surface, referred to as the event horizon, which acts as a one way surface for light going ...
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General relativity predicts the existence of Black Holes. A Black Hole (BH) is a region of space into which matter has collapsed and out of which not even light may escape and hence the term “black”. It partitions space into an inner region which is bounded by a surface, referred to as the event horizon, which acts as a one way surface for light going ...
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Near-horizon Black Hole Physics
2022This thesis studies the near-horizon black hole physics in depth from three perspectives. An important tool for studying perturbations of black hole spacetime is the linearized Einstein equations (LEE). In the Kerr spacetime, the variables in LEE do not separate, which poses a lot of difficulties to obtaining analytical solutions.
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2018
Abstract This chapter gives a brief description of Hawking radiation, which involves a combination of general relativity and quantum field theory and leads to a thermodynamical interpretation of the laws governing the evolution of black holes.
Nathalie Deruelle, Jean-Philippe Uzan
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Abstract This chapter gives a brief description of Hawking radiation, which involves a combination of general relativity and quantum field theory and leads to a thermodynamical interpretation of the laws governing the evolution of black holes.
Nathalie Deruelle, Jean-Philippe Uzan
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Quantum Physics of Black Holes
1998Quantum radiation from an isolated black hole reduces its mass, and hence its surface area. This “violation” of Hawking’s area theorem is explained by drawing the inevitable conclusion that the particle flux to infinity which carries away positive energy is accompanied by a flux of negative energy across the horizon into the black hole.
Valeri P. Frolov, Igor D. Novikov
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