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Neutrino interactions in neutron matter

Cipollone, A (2012) Neutrino interactions in neutron matter

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Abstract

Neutrino flow is the dominant mechanism of energy transfer in the latest stages of supernovae explosions and in compact stars. The Standard Model of particle physics and accelerator data, provide a satisfactory description of neutrino physics in vacuum up to TeV scale. Nevertheless modeling the dynamics of neutrino interaction in the nuclear environment involves severe difficulties. This thesis in mainly aimed at obtaining the weak response of infinite matter, using both the Correlated Basis Function theory and Landau Theory of Fermi liquid to take into account properly nucleon-nucleon hard core potential and long range correlation (quasi-particle, collective modes, ecc.)

Item Type: Article
Authors :
NameEmailORCID
Cipollone, Aandrea.cipollone@surrey.ac.ukUNSPECIFIED
Date : 20 December 2012
Uncontrolled Keywords : astro-ph.SR, astro-ph.SR, nucl-th
Related URLs :
Depositing User : Symplectic Elements
Date Deposited : 17 May 2017 12:39
Last Modified : 17 May 2017 12:39
URI: http://epubs.surrey.ac.uk/id/eprint/836225

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