COST Action MP1304 - Exploring fundamental physics with compact stars ( NewCompStar)
https://compstar.uni-frankfurt.de/
In this COST action Isaac Vidaña is a permanent member of the management committee, and Constança Providência a substitute member. Isaac Vidaña is a Topic Leader of the Working Group 2 and Constança Providência belongs to the Steering Committee as the coordinator of the Outreach. Renan Pereira maintains the outreach entrance.
Status: Running
Starting date: 25/Nov/2013
End date: 25/Nov/2017
Financing: Euros
Financing entity: ESF
Person*month: 0
Group person*month: 0
Members
- Constança Providência
- Isaac Vidaña Haro
- Silvia Chiacchiera
- Helena Sofia Pais
- Pedro Fernando Simões Costa
- Márcio Ferreira
- Renan Câmara Pereira
Articles
- Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars
- Light Clusters and Pasta Phases in Warm and Dense Nuclear Matter
- Neutron stars: From the inner crust to the core with the (extended) Nambu–Jona-Lasinio model
- Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness
- Two-solar-mass hybrid stars: a two model description with the Nambu-Jona-Lasinio quark model
- Neutrino diffusion in the pasta phase matter within the Thomas-Fermi approach
- Larger and more heterogeneous neutron star crusts: A result of strong magnetic fields
- Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
- The Vlasov formalism for extended relativistic mean field models: the crust-core transition and the stellar matter equation of state
- Spin polarization and color superconductivity in the Nambu Jona-Lasinio model at finite temperature
- Neutron star radii and crusts: uncertainties and unified equations of state
- Hyperons in neutron star matter within relativistic mean-field models
- Magnetic susceptibility and magnetization properties of asymmetric nuclear matter under a strong magnetic field
- Tensor force effects and high-momentum components in the nuclear symmetry energy
- Neutron matter under strong magnetic fields: a comparison of models
- Hyperons in neutron stars and supernova cores
- Quark matter nucleation in neutron stars and astrophysical implications
- Influence of the inverse magnetic catalysis and the vector interaction in the location of the critical end point
- Pasta phases in core-collapse supernova matter
- Anisotropy in the equation of state of magnetized quark matter
- Magnetic susceptibility and magnetization properties of asymmetric nuclear matter under a strong magnetic field
- Light clusters, pasta phases and phase transitions in core-collapse supernova matter
- Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars
