Scientific Background

In astroparticle physics, a number of complementary detection techniques are employed to measure cosmic particles of the highest energies. Cosmic rays are measured with ground-based particle detector arrays and air fluorescence telescopes. High energy neutrinos are detected via optical Cherenkov emission from muons induced by neutrino interactions in ice or water. However, these measurement techniques have limitations, be it with regard to uncertainties of hadronic interaction models, the number of detectors needed to instrument a given volume or the duty cycle with which a detector can be operated.

Radio detection of cosmic particles in both air and dense media has a high potential to suit as an alternative or complement to the well-established techniques. In air, radio measurements are viable with ~95% duty cycle. In dense media, radio detectors allow for a very sparse spacing of detectors. Using radio techniques, even the moon can be used as a target to measure cosmic rays and neutrinos of extremely high energies.

The field of radio detection in astroparticle physics has experienced a period of very vivid research over the past few years, and has matured to a state of making the transition from small-scale prototype experiments to large scale application in cosmic ray and neutrino detection. Consequently, the time is right for a review of the field and of its ambitious plans for the future.

Goals of the Seminar

The seminar will give a detailed overview of the field of radio detection of cosmic particles, both in air and dense media. Additionally, overlap with adjoining fields of research such as the acoustic detection of neutrinos in dense media and the physics of thunderstorms and their connection with radio detection techniques will be reviewed.

The format of the seminar, consisting of detailed 40-minutes lectures complemented with ample time for discussions for a limited number of only ~65 participants, will ensure very intense scientific exchange in particular for PhD students and young postdocs.

In addition to the lectures, the participants will be given an opportunity to present their own work with scientific posters, the best three of which will be awarded a prize.

Application

The total number of participants is limited. Full consideration will be given to applications received until July 31st, 2011 using the provided application form. We will notify the succesful candidates within two weeks after the end of the application deadline together with further information concerning accommodation, travel plans, etc.

Due to the generous support by the Wilhelm and Else Heraeus-Foundation, participation in the meeting, including meals and accommodation will be free of charge for all participants.