There are many logically and computationally distinct characterizations of the surface gravity of a horizon, just as there are many logically rather distinct notions of horizon. Fortunately, in standard general relativity, for stationary horizons, most of these characterizations are degenerate. However, in modified gravity, or in analogue spacetimes, horizons may be non-Killing or even non-null, and hence these degeneracies can be lifted. We present a brief overview of the key issues, specifically focusing on horizons in analogue spacetimes and universal horizons in modified gravity
This is a contribution to MG9 session BHT4. Certain geometrically distinguished frame on a non-expan...
For distant observers black holes are trapped spacetime domains bounded by apparent horizons. We rev...
We discuss different kinds of Killing horizons possible in static, spherically symmetric configurati...
There are many logically and computationally distinct characterizations of the surface gravity of a ...
This thesis explores two avenues into understanding the physics of black holes and horizons beyond g...
This thesis explores two avenues into understanding the physics of black holes and horizons beyond g...
This thesis explores two avenues into understanding the physics of black holes and horizons beyond g...
Doctoral Degree. University of KwaZulu-Natal, Durban.Abstract available in PDF.Some text in red
Since the 1970s, it has been known that black-hole (and other) horizons are truly thermodynamic. Mor...
The persistence of a suitable notion of black hole thermodynamics in Lorentz breaking theories of g...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
This is a contribution to MG9 session BHT4. Certain geometrically distinguished frame on a non-expan...
For distant observers black holes are trapped spacetime domains bounded by apparent horizons. We rev...
We discuss different kinds of Killing horizons possible in static, spherically symmetric configurati...
There are many logically and computationally distinct characterizations of the surface gravity of a ...
This thesis explores two avenues into understanding the physics of black holes and horizons beyond g...
This thesis explores two avenues into understanding the physics of black holes and horizons beyond g...
This thesis explores two avenues into understanding the physics of black holes and horizons beyond g...
Doctoral Degree. University of KwaZulu-Natal, Durban.Abstract available in PDF.Some text in red
Since the 1970s, it has been known that black-hole (and other) horizons are truly thermodynamic. Mor...
The persistence of a suitable notion of black hole thermodynamics in Lorentz breaking theories of g...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
We study the extent of quantum gravitational effects in the internal region of non-singular, Hayward...
This is a contribution to MG9 session BHT4. Certain geometrically distinguished frame on a non-expan...
For distant observers black holes are trapped spacetime domains bounded by apparent horizons. We rev...
We discuss different kinds of Killing horizons possible in static, spherically symmetric configurati...