activity
19942003
most citedLow Scale String Unification and the Highest Energy Cosmic Rays

1 citations · 1 across the 2 of their papers we have counts for

collaborators

7 papers

hep-ph2003

What Can we learn from Cosmic Rays?

S. Kovesi-Domokos, G. Domokos

Ultra high energy cosmic rays (UHECR) pose a problem either for particle physics or for astrophysics (or for both) by the unexpectedly high number of cosmic ray showers observed wi…

hep-ph20021 cited

Low Scale String Unification and the Highest Energy Cosmic Rays

William S. Burgett, G. Domokos, S. Kovesi-Domokos

String unification at a scale of a few tens of TeV explains the existence of cosmic ray interactions beyond the Greisen-Zatsepin-Kuzmin (GZK) cutoff. Trans-GZK cosmic rays are neut…

hep-ph2000

Ultrahigh Energy Neutrinos and the Highest Energy Cosmic Rays

G. Domokos, S. Kovesi-Domokos, Paul T. Mikulski

It has been suggested that the characteristic energy of string models may be considerably lower than the observed Planck mass. In such schemes, the unification of interactions take…

hep-ph1999

Energy Loss of Ultrahigh Energy Protons in Strong Magnetic Fields

G. Domokos, S. Kovesi-Domokos

Ultrahigh energy protons in magnetic fields produce pions and thus lose energy. The mean free path of such a process is worked out for Gaussian random fields. Two cases are conside…

hep-ph1998

Observation of Ultrahigh Energy Neutrino Interactions by Orbiting Detectors

G. Domokos, S. Kovesi-Domokos

Orbiting detectors will be able to observe showers initiated by neutrinos penetrating the Earth and interacting close to their exit point. There is a correlation between the impact…

hep-ph1998

Neutrinos in Random Magnetic Fields: The Problem of Measuring Magnetic Moments

G. Domokos, S. Kovesi-Domokos

The existence of magnetic moments of neutrinos points to physics beyond the standard model. Given current upper limits, terrestrial measurements are difficult or completely unfeasi…