by Dany Page, et al.
Publisher: arXiv 2013
Number of pages: 88
Neutron stars provide a fertile environment for exploring superfluidity under extreme conditions. It is not surprising that Cooper pairing occurs in dense matter since nucleon pairing is observed in nuclei as energy differences between even-even and odd-even nuclei. Since superfluids and superconductors in neutron stars profoundly affect neutrino emissivities and specific heats, their presence can be observed in the thermal evolution of neutron stars.
Home page url
Download or read it online for free here:
by Luis Alfredo Anchordoqui - arXiv
These lectures are aimed at graduate students in astrophysics/particle theory/particle experiment. We explain the important progress made in recent years towards understanding the experimental data on cosmic rays with energies higher than 10e8 GeV.
by P.K. Townsend - arXiv
Notes for a course taught in part III of the Cambridge University Mathematical Tripos: gravitational collapse, Schwarzschild black hole, charged black holes; rotating black holes; energy and angular momentum; black hole mechanics; Hawking radiation.
by Volker Springel - arXiv
These are lecture notes about high performance computing and numerical modelling in 43rd Saas Fee Advanced Course winter school, specifically covering the basics of numerically treating gravity and hydrodynamics in the context of galaxy evolution.
by Georg Raffelt - arXiv
The role of neutrinos in stars is introduced for students with little prior astrophysical exposure. We begin with neutrinos as an energy-loss channel in ordinary stars and how stars provide information on neutrinos and possible other particles.