AbstractIt has been shown in [G.A. Vilkovisky, hep-th/0511182] that the metric in the semiclassical region of the collapse spacetime is expressed purely kinematically through the Bondi charges. Here the Bondi charges are expressed through this metric by calculating the vacuum radiation against its background. The result is closed equations for the metric and the Bondi charges. Notably, there is a nonvanishing flux of the vacuum-induced matter charge
International audienceWe present an exact solution of the Maxwell-Einstein equations, which describe...
Abstract. I revisit a known solution of the Einstein field equations to show that it describes the f...
In this letter we show that an uncharged black hole moving superluminally in a transparent dielectri...
AbstractIt has been shown in [G.A. Vilkovisky, hep-th/0511182] that the metric in the semiclassical ...
The correspondence principle and causality divide the spacetime of a macroscopic collapsing mass int...
The following research contributes to the understanding of how electric charge influences the unwrap...
© 2018. The American Astronomical Society. All rights reserved.. In many astrophysically relevant si...
Classically, if two highly boosted particles collide head-on, a black hole is expected to form whose...
Black holes create a vacuum matter charge to protect themselves from the quantum evaporation. A sphe...
We study the Bondi-Sachs rockets with nonzero cosmological constant. We observe that the acceleratio...
The dynamical properties of an electron--positron--photon plasma created by the vacuum polarization ...
Considered is the class of metrics which can be obtained from nonextreme black holes by expanding ne...
Abstract. In this note, we study energy estimates for Einstein vacuum equations in order to prove th...
AbstractBlack holes create a vacuum matter charge to protect themselves from the quantum evaporation...
The results of various calculations of the Casimir effect and of the effect of particle creation by ...
International audienceWe present an exact solution of the Maxwell-Einstein equations, which describe...
Abstract. I revisit a known solution of the Einstein field equations to show that it describes the f...
In this letter we show that an uncharged black hole moving superluminally in a transparent dielectri...
AbstractIt has been shown in [G.A. Vilkovisky, hep-th/0511182] that the metric in the semiclassical ...
The correspondence principle and causality divide the spacetime of a macroscopic collapsing mass int...
The following research contributes to the understanding of how electric charge influences the unwrap...
© 2018. The American Astronomical Society. All rights reserved.. In many astrophysically relevant si...
Classically, if two highly boosted particles collide head-on, a black hole is expected to form whose...
Black holes create a vacuum matter charge to protect themselves from the quantum evaporation. A sphe...
We study the Bondi-Sachs rockets with nonzero cosmological constant. We observe that the acceleratio...
The dynamical properties of an electron--positron--photon plasma created by the vacuum polarization ...
Considered is the class of metrics which can be obtained from nonextreme black holes by expanding ne...
Abstract. In this note, we study energy estimates for Einstein vacuum equations in order to prove th...
AbstractBlack holes create a vacuum matter charge to protect themselves from the quantum evaporation...
The results of various calculations of the Casimir effect and of the effect of particle creation by ...
International audienceWe present an exact solution of the Maxwell-Einstein equations, which describe...
Abstract. I revisit a known solution of the Einstein field equations to show that it describes the f...
In this letter we show that an uncharged black hole moving superluminally in a transparent dielectri...
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