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arxiv: 1705.02525 · v1 · pith:DCSIO5DPnew · submitted 2017-05-06 · ⚛️ nucl-th · astro-ph.HE· cond-mat.quant-gas· cond-mat.supr-con

Composition of nuclear matter with light clusters and Bose-Einstein condensation of α particles

classification ⚛️ nucl-th astro-ph.HEcond-mat.quant-gascond-mat.supr-con
keywords matteralphaclusterscondensationbose-einsteincompositionisotopelight
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The Bose-Einstein condensation of $\alpha$ partciles in the multicomponent environment of dilute, warm nuclear matter is studied. We consider the cases of matter composed of light clusters with mass numbers $A\leq 4$ and matter that in addition these clusters contains $\isotope[56]{Fe}$ nuclei. We apply the quasiparticle gas model which treats clusters as bound states with infinite life-time and binding energies independent of temperature and density. We show that the $\alpha$ particles can form a condensate at low temperature $T\le 2$ MeV in such matter in the first case. When the $\isotope[56]{Fe}$ nucleus is added to the composition the cluster abundances are strongly modified at low temperatures, with an important implication that the $\alpha$ condensation at these temperatures is suppressed.

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