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Multifragmentation model for astrophysical strangelets

A model for the possible size distribution of astrophysical strangelets, that fragment out of the warm strange quark matter ejected during the merger of binary strange stars in the Galaxy, is presented here by invoking the statistical multifragmentation model. A simplified assumption of zero quark m...

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Bibliographic Details
Published in:Physics letters. B 2012-08, Vol.715 (1-3), p.30-34
Main Authors: Biswas, Sayan, De, J.N., Joarder, Partha S., Raha, Sibaji, Syam, Debapriyo
Format: Article
Language:English
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Summary:A model for the possible size distribution of astrophysical strangelets, that fragment out of the warm strange quark matter ejected during the merger of binary strange stars in the Galaxy, is presented here by invoking the statistical multifragmentation model. A simplified assumption of zero quark mass has been considered to obtain such mass-spectrum for the strangelets. An approximate estimate for the intensity of such strangelets in the galactic cosmic rays is also attempted by using a diffusion approximation.
ISSN:0370-2693
1873-2445
DOI:10.1016/j.physletb.2012.07.055