The intergalactic propagation of ultra-high energy cosmic ray nuclei

(2006)

Authors:

Dan Hooper, Subir Sarkar, Andrew M Taylor

Photon and dilepton production in supersymmetric Yang-Mills plasma

(2006)

Authors:

Simon Caron-Huot, Pavel Kovtun, Guy Moore, Andrei Starinets, Laurence G Yaffe

The Ubiquitous Throat

ArXiv hep-th/0607120 (2006)

Authors:

A Hebecker, J March-Russell

Abstract:

We attempt to quantify the widely-held belief that large hierarchies induced by strongly-warped geometries are common in the string theory landscape. To this end, we focus on the arguably best-understood subset of vacua -- type IIB Calabi-Yau orientifolds with non-perturbative Kaehler stabilization and a SUSY-breaking uplift (the KKLT setup). Within this framework, vacua with a realistically small cosmological constant are expected to come from Calabi-Yaus with a large number of 3-cycles. For appropriate choices of flux numbers, many of these 3-cycles can, in general, shrink to produce near-conifold geometries. Thus, a simple statistical analysis in the spirit of Denef and Douglas allows us to estimate the expected number and length of Klebanov-Strassler throats in the given set of vacua. We find that throats capable of explaining the electroweak hierarchy are expected to be present in a large fraction of the landscape vacua while shorter throats are essentially unavoidable in a statistical sense.

The Ubiquitous Throat

(2006)

Authors:

A Hebecker, J March-Russell

Anisotropy studies around the galactic centre at EeV energies with the Auger Observatory

ArXiv astro-ph/0607382 (2006)

Abstract:

Data from the Pierre Auger Observatory are analyzed to search for anisotropies near the direction of the Galactic Centre at EeV energies. The exposure of the surface array in this part of the sky is already significantly larger than that of the fore-runner experiments. Our results do not support previous findings of localized excesses in the AGASA and SUGAR data. We set an upper bound on a point-like flux of cosmic rays arriving from the Galactic Centre which excludes several scenarios predicting sources of EeV neutrons from Sagittarius $A$. Also the events detected simultaneously by the surface and fluorescence detectors (the `hybrid' data set), which have better pointing accuracy but are less numerous than those of the surface array alone, do not show any significant localized excess from this direction.