[PDF] Top 20 Sor Juana Inés de la Cruz y el espejo de los enigmas
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Frequency of Hawking Radiation of Black Holes
... In quantum physics, the empty space is not empty at all. In it there are always particles flashing into existence and disappear again. They always come in pairs; one particle and one anti-particle, like an electron and a ... See full document
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Hawking Radiation from Higher-Dimensional Black Holes
... that Hawking radiation from higher-dimensional black holes is more complicated than from four-dimensional black holes, with many fea- tures depending on the number of extra ... See full document
6
Hawking radiation from rotating brane black holes
... In this brief review we have considered the Hawking radiation of rotating brane black holes, as may be produced at the LHC. In references [1, 2, 3] we have studied in detail the fluxes of ... See full document
7
Low frequency analogue Hawking radiation: The Bogoliubov de Gennes model
... Our first result is the general low-frequency dependence of all scattering coefficients. In particular, the spectrum of emitted phonons increases like the inverse power of the frequency (see equation ... See full document
329
Low frequency analogue Hawking radiation: the Korteweg–de Vries model
... analogue Hawking radiation in a general weak-dispersive ...the Hawking one only when the dispersive length scale is much smaller than the flow gradient ... See full document
158
THE CASE STUDY OF BLACK HOLES?
... A hypothesis of general relativity predicts that an adequately minimized mass can disfigure spacetime to shape a dark opening. The limit of the locale from which no escape is conceivable is known as the occasion skyline. ... See full document
9
Black Holes—Information Models
... of black holes distribution by mass one can calculate the intensity of aggregated distri- bution of black holes radiation by frequencies and com- pare them with the experiment ... See full document
59
Upper Limit of Radiation from Coalescence of Rotating Hayward Black Holes
... Colliding black holes have been an expected source of gravitational ...gravitational radiation thermally allowed under the collision of two Hayward black ...holes[4]. Black hole ... See full document
6
Hawking radiation in dispersive media
... the Hawking prediction remains valid for low frequencies in the adiabatic ...regime, Hawking radiation behaves as it does in the dispersionless ...entire frequency range has never been found; ... See full document
25
Effect of Quintessential and Magnetic Field on GUP Modified Hawking Radiation
... the black holes (BHs) evaporation as a result of Hawking radiation [1] is one of the important ...of radiation process the researchers try to combine the gravitation within BH ... See full document
68
Binary Black Holes in the Inspiral Regime: The Effect of Spins and Eccentricity on Spacetime Dynamics and Gravitational Radiation
... The regime of final inspiral to plunge and merger can only be modeled by numerical relativity (Pretorius, 2005; Campanelli et al., 2006a; Baker et al., 2006; Campanelli et al., 2006b, 2007a,b; Lousto and Healy, 2015c,b). ... See full document
140
Black holes, TeV-scale gravity and the LHC
... The radiation of Standard Model particles on the brane in both the spin-down [26] and Schwarzschild phases [27] is studied using a gener- alization of Teukolsky’s formalism ...the radiation of scalar ... See full document
30
Analytical theory of Hawking radiation in dispersive media
... (angular) frequency ω ...one black-hole horizon, for simplicity. In a co-moving frame, the frequency is Doppler-shifted to ω − uk and equals ck for waves propagating against the ... See full document
22
Information Loss Paradox Resolved by Nonsingular Hyperbolic Spacetime
... and Hawking both agree that as a star collapses under its own gravity, it produces Hawking ...this radiation, the star also sheds ...a black hole. Before a black hole can form, the ... See full document
8
Massive photons propagation in gravitational field
... – Black holes represent the ultimate state that heavy stars can end their ...first black hole solution was obtained by Schwarzschild in 1916 employing Einstein’s general relativity field ...the ... See full document
8
Micro black holes in the laboratory
... a black hole emits quantum thermal radiation like a black body at a temperature proportional to the inverse of its mass, T ∝ 1/M ...as black hole evaporation since Hawking’s early work6, tells ... See full document
112
Topological black holes in su(N) Einstein Yang Mills theory with a negative cosmological constant
... topological black holes in su (N) EYM in adS was proven [31], but in that paper the solutions shown to exist are such that all the gauge field functions have no zeros (including at infinity), which are not ... See full document
31
Binary Black Holes Algorithm
... adapt black holes optimization algorithms for binary discrete search spaces by applying a sigmoid transformation to the gravity and electrical ...binary black hole and after calculating the gravity ... See full document
49
Topological black holes in su(N) Einstein-Yang-Mills theory with a negative cosmological constant
... topological black hole solutions of su( 3 ) EYM for k = − ...20. Black hole solutions exist in the region bounded by the axes and the solid ...topological black hole solutions are labelled according ... See full document
11
Preons, Gravity and Black Holes
... for non-singular black hole formation. Near and above Planck scale the particle interactions due to curvature of general relativity are assumed to be compara- tively small, but the essence of GR to spacetime ... See full document
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