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Surface tension of highly magnetized degenerate quark matter

Nuclear Theory 2017-01-25 v2 High Energy Astrophysical Phenomena High Energy Physics - Phenomenology

Abstract

We study the surface tension of highly magnetized three flavor quark matter within the formalism of multiple reflection expansion (MRE). Quark matter is described as a mixture of free Fermi gases composed by quarks uu, dd, ss and electrons, in chemical equilibrium under weak interactions. Due to the presence of strong magnetic fields the particles' transverse motion is quantized into Landau levels, and the surface tension has a different value in the parallel and transverse directions with respect to the magnetic field. We calculate the transverse and longitudinal surface tension for different values of the magnetic field and for quark matter drops with different sizes, from a few fm to the bulk limit. For baryon number densities between 2102-10 times the nuclear saturation density, the surface tension falls in the range 2202 - 20 MeV /fm2^{2}. The largest contribution comes from strange quarks which have a surface tension an order of magnitude larger than the one for uu or dd quarks and more than two orders of magnitude larger than for electrons. Our results show that the total surface tension is quite insensitive to the size of the drop. We also find that the surface tensions in the transverse and parallel directions are almost unaffected by the magnetic field if eBeB is below 5×103\sim 5 \times 10^{-3} GeV2^2. Nevertheless, for higher values of eBeB, there is a significant increase in the parallel surface tension and a significant decrease in the transverse one with respect to the unmagnetized case.

Keywords

Cite

@article{arxiv.1610.05875,
  title  = {Surface tension of highly magnetized degenerate quark matter},
  author = {G. Lugones and A. G. Grunfeld},
  journal= {arXiv preprint arXiv:1610.05875},
  year   = {2017}
}

Comments

version to appear in Physical Review C