A review is given of the theory and phenomenology of neutrino electromagnetic interactions,
which provide powerful tools to probe the physics beyond the standard model. After a …

The microscopic quantum nature of elementary particles, chirality, leads to macroscopic
phenomena like the chiral anomaly, chiral magnetic effect, and chiral plasma instability. We …

We show that a sterile neutrino with a mass in the 1–20 keV range and a small mixing with
the electron neutrino can simultaneously explain the origin of the pulsar motions and the …

Based on the recently formulated chiral radiation transport theory for left-handed neutrinos,
we study the chiral transport of neutrinos near thermal equilibrium in core-collapse …

The origin of pulsar kicks is reviewed in the framework of the spin-flip conversion of
neutrinos propagating in the gravitational field of a magnetized protoneutron star. We find …

Aims. We critically discuss a pulsar acceleration mechanism based on asymmetric neutrino
emission from the direct quark Urca process in the interior of proto neutron stars. Methods …

Neutrinos have no electric charge, but a magnetic field can indirectly affect neutrino
properties and interactions through its effect on charged particles. After a brief field-theoretic …

It has been suggested that the observed pulsar velocities are caused by an asymmetric
neutrino emission from a hot neutron star during the first seconds after the supernova …

We study the neutrino interaction rates in hot matter at high densities in the presence of a
uniform magnetic field. The neutrino cross sections involving both the charged current …

In this work we calculate the pulsar kick velocity of a magnetized neutron star (NS)
composed of a degenerate quark matter core with non-Fermi liquid (NFL) correction. Both …