Speaker
Dr
M. A. Perez-Garcia
(University of Salamanca and IUFFyM)
Description
Using techniques of finite-temperature microscopic computational many-body modelling, we evaluate the microscopic structure of the neutron star crust at low nuclear densities for different isospin composition conditions focusing on temperature effects.
We will discuss about how the latter alter the inhomogenous pasta phases through the arising droplet configurations and, consequently, about the importance of this for the first stages of cooling compact stars.
Author
Dr
M. A. Perez-Garcia
(University of Salamanca and IUFFyM)
Co-author
Dr
C. Albertus
(University of Granada)
