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.

Recent developments in perturbative QCD

(2006)

ΔI=1/2 rule in holographic QCD

Physical Review D - Particles, Fields, Gravitation and Cosmology 74:2 (2006)

Authors:

T Hambye, B Hassanain, J March-Russell, M Schvellinger

Abstract:

We study the ΔI=1/2 rule for kaon decays and the BK parameter for K0-K̄0 mixing in a dual 5-dimensional holographic QCD model. We perform, in the chiral limit, computations of the relevant four-point current-current correlators, which depend upon self-interactions among the 5D bulk fields. Spontaneous chiral symmetry breaking (χSB) is realized through boundary conditions on the bulk fields. Numerical results are analyzed in comparison with QCD, chiral perturbation theory (χPT) and data, finding reasonable agreement with the experimental values of the g8 and g27 parameters describing the ΔI=1/2, 3/2 decay channels. © 2006 The American Physical Society.

Seeing the Invisible Axion in the Sparticle Spectrum

ArXiv hep-ph/0607138 (2006)

Abstract:

I describe how under favourable circumstances the invisible axion may manifest its existence at the LHC through the sparticle spectrum; in particular through a gluino \sim \ln (M_P/m_{3/2}) times heavier than other gauginos.

Seeing the Invisible Axion in the Sparticle Spectrum

(2006)