Neutrino Emission from Ungapped Quark Matter

Details Neutrino Emission from Ungapped Quark Matter Neutrino Emission from Ungapped Quark Matter

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jhw..confe..30s&link_type=abstract

Proceedings of the 29th Johns Hopkins Workshop on current problems in particle theory: strong matter in the heavens. 1-3 August,

Computer Science

Scientific paper

We study the cooling of compact star cores due to neutrino emission from ungapped quark modes within an effective theory for magnetic interactions at high density. As shown recently the rele- vant low energy dynamics is semi-perturbative even for realistic couplings of order one due to a systematic expansion scheme in (ω/m)1/3 , where ω is the energy and m the screening scale. We find that the characteristic T 6 behavior of the neutrino emissivity remains valid even when the strong coupling is not small. In the weak coupling limit the results shows a non-Fermi liquid low temperature enhancement.

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