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Proc. Neutrino Astrophysics - MPP Theory Group

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Preface<br />

This was the fourth workshop in our series of annual “retreats” of the Sonderforschungsbereich<br />

Astroteilchenphysik (Special Research Center for Astroparticle Physics), or SFB for<br />

short, to the Ringberg Castle above Lake Tegernsee in the foothills of the Alps. These<br />

meetings are meant to bring together the members of the SFB which are dispersed between<br />

four institutions in the Munich area, the Technical University Munich (TUM), the Ludwig-<br />

Maximilians-University (LMU), and the Max-Planck-Institute for Physics (<strong>MPP</strong>) and that<br />

for <strong>Astrophysics</strong> (MPA). We always invite a number of external speakers, including visitors<br />

at our institutions, to complement the scientific program and to further the exchange of ideas<br />

with the international community.<br />

This year’s topic was “<strong>Neutrino</strong> <strong>Astrophysics</strong>” which undoubtedly is one of the central<br />

pillars of astroparticle physics. We focused on the astrophysical and observational aspects<br />

of this field, deliberately leaving out theoretical particle physics and laboratory experiments<br />

from the agenda. Each day of the workshop was dedicated to a specific sub-topic, ranging<br />

from solar, supernova and atmospheric neutrinos over high-energy cosmic rays to the early<br />

universe. A session on future prospects served to conclude the workshop and provide an<br />

outlook on the field in the next decade and beyond. We started every topical session with one<br />

or two introductory talks, reviewing the status of theory and experiment and to providing<br />

some background for the non-experts.<br />

For the entire program we interpreted “neutrino astrophysics” in a broad sense, including,<br />

for example, the physics of γ-ray bursts or the recent observations of TeV γ-rays by the<br />

imaging air-Cherenkov technique. Some of the after-dinner-talks went significantly beyond a<br />

narrow interpretation of the field! From our perspective the profile of neutrino astrophysics<br />

as defined by our program worked very well, even better than we had hoped. We are proud<br />

that the main complaint of the participants seemed to be that they did not get enough<br />

mountain-hiking done because the sessions were too interesting to miss.<br />

Besides regular SFB resources this workshop was made possible by a direct grant from<br />

the Max-Planck-Society and additional funds from the Max-Planck-Institute for <strong>Astrophysics</strong>.<br />

Special thanks go to the SFB secretary, Maria Depner, for her smooth and skillful management<br />

of all practical matters related to the workshop.<br />

We thank the participants for their high-level contributions and for being extremely cooperative<br />

in submitting the “extended abstracts” of their talks on time and in a format that<br />

allowed us to produce these proceedings in electronic form. Anyone interested in a printed<br />

version should write to the SFB secretary at the address given on the previous page. We<br />

hope that you will find this booklet a useful and up-to-date resource for the exciting and<br />

fast-developing field of neutrino astrophysics.<br />

Michael Altmann, Wolfgang Hillebrandt, Hans-Thomas Janka and Georg Raffelt<br />

Munich, January 1998<br />

iii

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