Some issues about neutrino processes in color superconducting quark matter
Qun Wang
Abstract
Several relevant issues in computing neutrino emissivity in Urca processes in color superconducting quark matter are addressed. These include: (1) The constraint on u quark abundance is given from electric neutrality and the triangle relation among Fermi momenta for participants. (2) The phase space defined by Fermi momentum reduction of quarks is discussed in QCD and NJL model. (3) Fermi effective model of weak interaction is reviewed with special focus on its form in Nambu-Gorkov basis.
Create a lesson
Related papers
First-principle predictions of fragmentation functions via quantum computing
Juan J. Gálvez-Viruet, Felipe J. Llanes-Estrada, Nicolas M. Arenaza et al.
High energy thermal photons from chirally imbalanced QGP
Sourav Duari, Nilanjan Chaudhuri, Pradip Roy et al.
Spin-dependent fermion potentials from mixed tensor couplings of massive spin-1 and spin-2 bosons
D. Khadka, V. V. Flambaum
Building a Better Beta: Nucleation and Timescales in Cosmological Phase Transitions
William Searle, Csaba Balázs
Quantum Steering Geometry at High Energy Particle Colliders
Juan J. Mejia Alvarez, Andrew J. Wildridge, Angelo Arisi et al.
Quantum-statistical effects of bosonic warm dark matter in microscopic interacting dark sectors
Zhijian Zhang