Probing low-x QCD with cosmic neutrinos at the Pierre Auger Observatory
Physical Review D - Particles, Fields, Gravitation and Cosmology 74:4 (2006)
Abstract:
The sources of the observed ultrahigh energy cosmic rays must also generate ultrahigh energy neutrinos. Deep inelastic scattering of these neutrinos with nucleons on Earth probe center-of-mass energies s∼100TeV, well beyond those attainable at terrestrial colliders. By comparing the rates for two classes of observable events, any departure from the benchmark (unscreened perturbative QCD) neutrino-nucleon cross section can be constrained. Using the projected sensitivity of the Pierre Auger Observatory to quasihorizontal showers and Earth-skimming tau neutrinos, we show that a "super-Auger" detector can thus provide an unique probe of strong interaction dynamics. © 2006 The American Physical Society.Erratum: Improved bounds on universal extra dimensions and consequences for Kaluza-Klein dark matter (Physical Review D - Particles, Fields, Gravitation and Cosmology (2006) 73, (095002))
Physical Review D Particles Fields Gravitation and Cosmology 74:1 (2006)
The intergalactic propagation of ultra-high energy cosmic ray nuclei
(2006)
Photon and dilepton production in supersymmetric Yang-Mills plasma
(2006)
The Ubiquitous Throat
ArXiv hep-th/0607120 (2006)