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University of Birmingham > Talks@bham > Condensed Matter Physics Seminars > Neutron stars as superfluid laboratories
Neutron stars as superfluid laboratoriesAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Elizabeth Blackburn. Neutron stars are, at least in principle, laboratories for extreme physics. They are expected to contain superfluid components, the presence of which may affect their behaviour significantly. In this talk, I will discuss our current understanding of neutron-star superfluidity, how our models relate to laboratory systems (like superfluid helium) and give an overview of the observational evidence from pulsar glitches, free precession and magnetar oscillations. This talk is part of the Condensed Matter Physics Seminars series. This talk is included in these lists:
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