Disassembly model for the production of astrophysical strangelets
High Energy Astrophysical Phenomena
2015-04-14 v2 Nuclear Theory
Abstract
Determination of the baryon number (or mass) distribution of the strangelets, that may fragment out of the warm and excited strange quark matter (SQM) ejected in the merger of strange stars (SSs) in compact binary stellar systems of the Galaxy, is attempted by using a statistical disassembly model (SMM). Finite mass of strange quarks is taken into account in the analysis. Strangelet charge and the resulting Coulomb correction are included to get a plausible mass distribution of galactic strangelets at their source.
Keywords
Cite
@article{arxiv.1405.2532,
title = {Disassembly model for the production of astrophysical strangelets},
author = {Sayan Biswas and J. N. De and Partha S. Joarder and Sibaji Raha and Debapriyo Syam},
journal= {arXiv preprint arXiv:1405.2532},
year = {2015}
}
Comments
10 pages, 2 figures