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Search for Antideuterons of Cosmic Origin Using the BESS-Polar II Magnetic-Rigidity Spectrometer.
K Sakai1,2, H Fuke3, K Yoshimura4
1NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, Maryland 20771, USA.
Researchers found no antideuterons (d[over ¯]s) in cosmic rays, setting a new flux limit. This result improves upon previous experiments and provides crucial data for theoretical predictions.
Area of Science:
- * Particle astrophysics and cosmology
- * Cosmic ray physics
Background:
- * Cosmic rays contain various particles, including potential antimatter components.
- * Antideuterons (d[over ¯]s) are predicted by some theories, such as supersymmetry, and their detection could indicate new physics.
- * Previous experiments have searched for antideuterons, but with limited sensitivity.
Purpose of the Study:
- * To search for antideuterons (d[over ¯]s) in cosmic ray data.
- * To establish an upper limit on the antideuteron flux.
- * To test theoretical predictions for antideuteron production in the galaxy.
Main Methods:
- * Analysis of 4.7×10⁹ cosmic-ray events collected during the BESS-Polar II flight (2007-2008) at solar minimum.
- * Utilized a sensitive detector to identify and distinguish antideuterons from other cosmic ray particles.
- * Calculated a 95% confidence level (C.L.) upper limit on the antideuteron flux.
Main Results:
- * No antideuteron candidates were detected in the observed cosmic ray events.
- * A 95% C.L. upper limit on the antideuteron flux was determined to be 6.7×10⁻⁵ (m² s sr GeV/n)⁻¹ for energies between 0.163 and 1.100 GeV/n.
- * This limit represents a significant improvement, over 14 times lower than previous limits from the BESS97 experiment.
Conclusions:
- * The BESS-Polar II experiment sets the most stringent upper limit on the antideuteron flux to date.
- * This result achieves the sensitivity required to constrain current theoretical models of antideuteron production.
- * The lack of detected antideuterons places constraints on theories predicting their abundance in cosmic rays.
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