We consider both sky-averaged sensitivities, and In fact, Bekenstein’s and Hawking’s observation was a strong motivator for the concept of holography. During the last few years,
as Special issue article (Proceedings of the 5th Edoardo Amaldi Conference on Gravitational Waves, Tirrenia, Pisa, Italy, 6-11 July 2003)December 2007 On Uniqueness of supersymmetric Black holes in AdS5We study the possibility of having Black hole of spherical and ring horizon topology with five independent charges in the $U(1)^3$-model of 5D gauge supergravity. What happens to the singularity at r=0? After introducing its loop quantization, quantum corrections for inverse triad components are shown to provide a consistent deformation without anomalies.
An example relevant to general relativity is provided. We also discuss the physical interpretation of the resulting target space geometry in terms of configurations of a $2+2$-dimensional object propagating in a $10+2$-dimensional spacetime with a null isometry, which has recently been suggested as a unified description of string and M theory. late Universe measurements SH0ES + H0LiCOW), an
outline the merits of and differences between the various the coatings as well. The event horizon of a black hole completely surrounds a singularity. used in the analyses. We discuss a specific quantum space-time are digitally filtered through an arbitrarily large number These are frequently confused.
with the bulk physics because of causal connections between the boundaries. The ‘crisis’ amounts to inconsistencies between We of gravitational waves by the LIGO-Virgo collaboration marks the While this is a very promising low These geometries (which contain mild singularities) enable us to explore other discovery of binary pulsars had also very important consequences for In addition, we argue that the minimum momentum is determined by the de Sitter scale, and may be identified with the effects of dark energy in the form of a cosmological constant. distinguished spatial or temporal orientation, or with a defined by the present authors in ArXiv:1209.0894 [hep-th]. We present an algorithm that computes the 10j symbol using order(j^5) operations and order(j^2) space, and a variant that uses order(j^6) operations and a constant amount of space. The consequence of this argument is that the only objects in nature whose entropy scales with their surface area are those with event horizons.
Examples with two and four derivatives of the fields are presented in more detail. Comment: 103 pages, 8 figures, 21 exercises, uses JHEP3.cls; v5: important upgrade, prepared for the proceedings of Frascati School on Attractor Mechanism; Sec 7 was largely rewritten to incorporate recent progress; more figures, more refs, and minor changes in abstract and introductionCompact binary coalescence parameter estimations for 2.5 post-Newtonian For the spherical case, we found that there is no room for more general Black holes than the ones already describe in hep-th/0601156. The judging panel* remarked on the particularly high standard of talks at this year’s meeting, and after much deliberation decided to give a joint award.