PIRSA:11060017

An effective theory for the neutron star inner crust

Sharma, R. (2011). An effective theory for the neutron star inner crust. Perimeter Institute. https://pirsa.org/11060017

Sharma, Rishi. An effective theory for the neutron star inner crust. Perimeter Institute, Jun. 20, 2011, https://pirsa.org/11060017 

          @misc{ pirsa_PIRSA:11060017,
            doi = {10.48660/11060017},
            url = {https://pirsa.org/11060017},
            author = {Sharma, Rishi},
            keywords = {Particle Physics},
            language = {en},
            title = {An effective theory for the neutron star inner crust},
            publisher = {Perimeter Institute},
            year = {2011},
            month = {jun},
            note = {PIRSA:11060017 see, \url{https://pirsa.org}}
          }

Rishi Sharma

TRIUMF (Canada's National Laboratory for Particle and Nuclear Physics)

Talk number
PIRSA:11060017
Collection
Talk Type
Subject
Abstract
The inner crust of neutron stars has a remarkable property that it is crystalline as well as superfluid. I will describe the low energy theory of systems with this property in general, and describe how to relate the low energy constants of the theory to derivatives of the free energy with respect to lattice shape and chemical potentials. As an application, I will discuss the mixing of lattice and superfluid modes in the neutron star inner crust.