A (toy) model for cold and luke-warm strongly-coupled nuclear matter at finite baryon density is used to study neutrino transport. The complete charged current two-point correlators are computed in the strongly-coupled medium and their impact on neutrino transport is analyzed. The full result is compared with various approximations for the current correlators and the distributions, including the degenerate approximation, the hydrodynamic approximation as well as the diffusive approximation and we comment on their successes. Further improvements are discussed.Comment: 67 pages + Appendix; 27 figures. Accepted for publication in JHEP. The treatment of isospin asymmetry was not correct in the previous version, so the isospin chemical poten...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
We develop a first-principles formalism to compute the distortion to the relic neutrino density fiel...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...
International audienceA (toy) model for cold and luke-warm strongly-coupled nuclear matter at finite...
Neutrinos are copiously emitted by neutron star mergers, due to the high temperatures reached by den...
This article provides a concise review of the problem of neutrino radiation from dense matter. The s...
Gravitational waves and electromagnetic signals from merging neutron star binaries provide valuable ...
Gravitational waves and electromagnetic signals from merging neutron star binaries provide valuable ...
The early evolution of a protoneutron star depends both on the equation of state and neutrino intera...
We have recently proposed an explanation for the birth velocities of pulsars based on neutrino oscil...
We apply the idea of landscape (motivated by string theory) to study the statistical nature of param...
A variety of new physics scenarios allow for neutrinos to up-scatter into a heavy neutral lepton sta...
The mechanism driving core-collapse supernovae is sensitive to the interplay between matter and neut...
Neutrino-neutrino scattering could have a large secret component that would turn neutrinos within a ...
When hypothetical neutrino secret interactions ($\nu$SI) are large, they form a fluid in a supernova...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
We develop a first-principles formalism to compute the distortion to the relic neutrino density fiel...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...
International audienceA (toy) model for cold and luke-warm strongly-coupled nuclear matter at finite...
Neutrinos are copiously emitted by neutron star mergers, due to the high temperatures reached by den...
This article provides a concise review of the problem of neutrino radiation from dense matter. The s...
Gravitational waves and electromagnetic signals from merging neutron star binaries provide valuable ...
Gravitational waves and electromagnetic signals from merging neutron star binaries provide valuable ...
The early evolution of a protoneutron star depends both on the equation of state and neutrino intera...
We have recently proposed an explanation for the birth velocities of pulsars based on neutrino oscil...
We apply the idea of landscape (motivated by string theory) to study the statistical nature of param...
A variety of new physics scenarios allow for neutrinos to up-scatter into a heavy neutral lepton sta...
The mechanism driving core-collapse supernovae is sensitive to the interplay between matter and neut...
Neutrino-neutrino scattering could have a large secret component that would turn neutrinos within a ...
When hypothetical neutrino secret interactions ($\nu$SI) are large, they form a fluid in a supernova...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
We develop a first-principles formalism to compute the distortion to the relic neutrino density fiel...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...