Add to ORKGThis article provides a concise review of the problem of neutrino radiation from dense matter. The subjects addressed include quantum kinetic equations for neutrino transport, collision integrals describing neutrino radiation through charged and neutral current interactions, radiation rates from pair-correlated baryonic and color superconducting quark matter
Neutrinos are copiously emitted by neutron star mergers, due to the high temperatures reached by den...
The thermal conductivity of the color-flavor locked phase of dense quark matter is calculated. The d...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...
A brief review is given of neutrino emission processes in dense matter, with particular emphasis on ...
Several relevant issues in computing neutrino emissivity in Urca processes in color superconducting ...
We calculate the neutrino mean free path in color superconducting quark matter, and employ it to stu...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...
The aim of these lectures is to introduce basic processes responsible for cooling of neutron stars ...
This review demonstrates that neutrino emission from dense hadronic component in neutron stars is su...
We calculate neutrino emissivities from the decay and scattering of Goldstone bosons in the color-fl...
AbstractDense matter in compact stars cools efficiently by neutrino emission via the direct Urca pro...
It is now firmly established that neutrinos, which are copiously produced in the hot and dense core ...
The subject of this dissertation is the evolution of neutrino distributions in hot, dense astrophysi...
We discuss specific heat and neutrino emissivity due to direct Urca processes for quark matter in th...
A (toy) model for cold and luke-warm strongly-coupled nuclear matter at finite baryon density is use...
Neutrinos are copiously emitted by neutron star mergers, due to the high temperatures reached by den...
The thermal conductivity of the color-flavor locked phase of dense quark matter is calculated. The d...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...
A brief review is given of neutrino emission processes in dense matter, with particular emphasis on ...
Several relevant issues in computing neutrino emissivity in Urca processes in color superconducting ...
We calculate the neutrino mean free path in color superconducting quark matter, and employ it to stu...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...
The aim of these lectures is to introduce basic processes responsible for cooling of neutron stars ...
This review demonstrates that neutrino emission from dense hadronic component in neutron stars is su...
We calculate neutrino emissivities from the decay and scattering of Goldstone bosons in the color-fl...
AbstractDense matter in compact stars cools efficiently by neutrino emission via the direct Urca pro...
It is now firmly established that neutrinos, which are copiously produced in the hot and dense core ...
The subject of this dissertation is the evolution of neutrino distributions in hot, dense astrophysi...
We discuss specific heat and neutrino emissivity due to direct Urca processes for quark matter in th...
A (toy) model for cold and luke-warm strongly-coupled nuclear matter at finite baryon density is use...
Neutrinos are copiously emitted by neutron star mergers, due to the high temperatures reached by den...
The thermal conductivity of the color-flavor locked phase of dense quark matter is calculated. The d...
We calculate the rate of energy radiation by bremsstrahlung of neutrino pairs by baryons in neutron ...