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Advances in High Energy Physics
Volume 2017, Article ID 1273931, 11 pages
Review Article

Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma

Experimental High Energy Physics and Applications Group, Variable Energy Cyclotron Center, 1/AF Bidhannagar, Kolkata 700 064, India

Correspondence should be addressed to Souvik Priyam Adhya; moc.liamg@7002ayhdakivuos

Received 20 July 2016; Revised 31 December 2016; Accepted 19 February 2017; Published 16 March 2017

Academic Editor: Sally Seidel

Copyright © 2017 Souvik Priyam Adhya. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP3.


The cardinal focus of the present review is to explore the role of neutrinos originating from the ultradense core of neutron stars composed of quark gluon plasma in the astrophysical scenario. The collective excitations of the quarks involving the neutrinos through the different kinematical processes have been studied. The cooling of the neutron stars as well as pulsar kicks due to asymmetric neutrino emission has been discussed in detail. Results involving calculation of relevant physical quantities like neutrino mean free path and emissivity have been presented in the framework of non-Fermi liquid behavior as applicable to ultradegenerate plasma.