1–5 Aug 2011
AlbaNova University Center
Europe/Stockholm timezone

The search for TeV cosmic ray electrons with the CREST experiment

1 Aug 2011, 16:50
20m
The Oskar Klein Auditorium (AlbaNova University Center)

The Oskar Klein Auditorium

AlbaNova University Center

Speaker

Prof. Scott Nutter (Northern Kentucky University)

Description

The Cosmic Ray Electron Synchrotron Telescope (CREST) high-altitude balloon experiment is a pathfinding effort to detect multi-TeV cosmic-ray electrons. These electrons would be indicative of nearby cosmic accelerators, since energetic electrons from distant Galactic sources are depleted by radiative losses during interstellar transport. The electrons will be detected indirectly by the characteristic signature of their geomagnetic synchrotron losses: a group of collinear x-ray photons intersecting the instrument. Since the primary electron itself need not traverse the payload, an effective detection area is achieved that is several times the nominal 6.4 m^2 instrument. The payload is composed of an array of 1024 BaF2 crystals surrounded by a set of plastic scintillator detectors which veto through-going charged particles. A long-duration balloon flight in Antarctica is planned for the upcoming 2010-11 season.

Primary author

Prof. Scott Nutter (Northern Kentucky University)

Co-authors

C. Bower (Indiana University) D. Müller (University of Chicago) G. Tarlé (University of Michigan) J. Gennaro (University of Michigan) J. Musser (Indiana University) M. Geske (Pennsylvania State University) M. Schubnell (University of Michigan) N. H. Park (Indiana University) S. Coutu (Pennsylvania State University) S. Wakely (University of Chicago) Mr T. Anderson (Pennsylvania State University)

Presentation materials