Speaker
Prof.
Armen Sedrakian
Description
Relativistic density functionals based on baryon-meson Lagrangians can
be used to describe effectively dense matter in compact stars
including hyperonic and Delta-resonance degrees of
freedom. These can be supplemented with a first-order phase transition
to quark matter at high densities to describe hybrid compact stars.
I will discuss how the mass-radius and tidal deformability inferences
from electromagnetic and gravitational wave observations constrain the
current models of hypernuclear and hybrid stars. I will briefly review
recent results on the bulk viscosity of dense nucleonic matter in hot
compact stars, which emerged in recent years as the leading dissipative
channel in binary-neutron star merger simulations.
Details
I am the speaker
| Internet talk | No |
|---|---|
| Is this an abstract from experimental collaboration? | No |
| Name of experiment and experimental site | Not an experiment |
| Is the speaker for that presentation defined? | Yes |
Author
Prof.
Armen Sedrakian
