Astrophysical sources of the medium and low energy neutrinos

This is the list of the potentially interesting sources of the medium-energy neutrinos, available to study using methods developed for pre-supernova stars, i.e. objects transparent to neutrinos.

In limited range of the physical conditions, only temperature and electron chemical potential (or density and electron fraction) is required to compute neutrino spectrum. These objects are fully transparent to neutrinos, and total luminosities can be obtained with simple integration of the basic processes over volume of the object.

This is our list of worth of more detailed analysis (i.e. potentially detectable in the future) sources of the neutrinos:
We also provide some basic information on the well established other sources of the neutrinos. This gives intuitive comparison of the sources detected in the past to the sources we believe will be detected in not so far distant future.