Abstract
The analysis of the data of the COMPTON observatory [BATSE Burst catalog] indicates the existence of dipole asymmetry with amplitude a=0.036 in the direction b=-22°, l=30°. The observational data are shown to agree qualitatively with the giant dark matter halo (GDMH) model of Gurevich et al. [Phys. Lett. A 175 (1993) 397]. The method of observational verification of the GDHM model is suggested.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
