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astro-ph2000
Superfluidity in relativistic neutron stars
David Langlois
The purpose of these notes is to give a brief review of superfluidity in neutron stars. After a short presentation explaining why and how superfluidity is expected in the crust and…
astro-ph2000
Centrifugal buoyancy as a mechanism for neutron star glitches
Brandon Carter, David Langlois, David M. Sedrakian
The frequent glitches (sudden increases of the apparent angular velocity) observed in certain pulsars are generally believed to be attributable to discontinuous angular momentum tr…
astro-ph2000
Correlated mixtures of adiabatic and isocurvature cosmological perturbations
Alain Riazuelo, David Langlois
The Cosmic Microwave Background (CMB) anisotropies measurements can provide many clues about the Universe. Although the common belief is that they will allow a very precise measure…