| This programme is designed to bring together researchers on neutron star dynamics, condensed matter and nuclear
physics as well as experts on the surface layers and the
magnetosphere. The aim is to discuss synergies that can arise from
collaboration and exchange of expertise. Key questions are: What input from microphysics calculations do we need to build realistic
theoretical models? What bounds can the dynamical models in
conjunction with observations provide on the state of matter at
extreme densities? How do we use observations to constrain these
parameters? If a neutron star is oscillating, how does information of
the oscillations propagate to the observers? |
|
| Dates: |
from 14 September 2009 08:00 to 26 September 2009 18:00 |
| Location: |
Nordita
Roslagstullsbacken 23
AlbaNova University Center
10691 Stockholm
Sweden |
| Chairs: |
Dr. SAMUELSSON, Lars
Prof. ANDERSSON, Nils |
|
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