Neutron Star Theory- Madrid

from Thursday, 10 October 2019 (08:30) to Friday, 11 October 2019 (15:00)
Facultad de Ciencias Fisicas UCM (Sala de Grados (1st floor))

        : Sessions
    /     : Talks
        : Breaks
10 Oct 2019
11 Oct 2019
08:35 --- Registration and welcome ---
09:05 Numerical simulations of neutron star mergers - Dr. Kastaun Wolfgang (Max Planck Institute for Gravitational Physics Hanover)   (Sala de Grados (1st floor))
09:45 Quasinormal modes of neutron stars with scalar hair - Dr. Jose Luis Blázquez-Salcedo   (Sala de Grados (1st floor))
10:25 Gravitational wave echoes from strange stars - Massimo Mannarelli (INFN-LNGS)   (Sala de Grados (1st floor))
10:50 --- Coffee Break ---
11:20 Mixed configurations of tensor-multi-scalar solitons and neutron stars - Stoytcho Yazadjiev (Sofia University)   (Sala de Grados (1st floor))
11:45 Thermodynamically consistent equation of state for an accreted crust - Mikhail Gusakov (Ioffe Institute)   (Sala de Grados (1st floor))
09:15 Resumming the fermionic in-medium ladder diagrams to all orders (Russian-Iberian congress) by Jose Antonio Oller   (Aula M2 (ground floor))
09:55 Study of the core-crust transition in neutron stars with finite-range interactions: the dynamical method (Russian-Iberian Congress) by Xavier Viñas   (Aula M2 (ground floor))
10:35 Gravitation wave driven CFS instability of neutron stars and current observational constraints (Russian-Iberian Congress) by Andrey Chugunov   (Aula M2 (ground floor))
11:00 --- Coffee Break ---
11:30 Constraints in Neutron Stars Properties - Morgane Fortin (CAMK PAN)   (Aula M2 (ground floor))
12:25 EoS in neutron stars - recent results on cooling and tidal deformabilities - Laura Tolos   (Sala de Grados (1st floor))
12:50 Bulk viscosity of baryonic matter with trapped neutrinos and its application to neutron star mergers - Dr. Arus Harutyunyan (Byurakan Astrophysical Observatory, Yerevan State University)   (Sala de Grados (1st floor))
13:30 --- Lunch break ---
15:05 nEoS: Neutron Star Equation of State from hadron physics alone - Eva Lope Oter (Universidad Complutense de Madrid)   (Sala de Grados (1st floor))
15:30 An universal upper limit for shear modulus of neutron star crust - Dr. Andrey Chugunov (Ioffe Institute)   (Sala de Grados (1st floor))
15:55 The crust of accreting neutron stars within simplified reaction network - Nikolay Shchechilin (Ioffe Institute)   (Sala de Grados (1st floor))
16:50 Heat transport in neutron stars - Dr. Alexander Potekhin (Ioffe Institute)   (Sala de Grados (1st floor))
17:30 Generation of strong magnetic fields in neutron stars driven by the permanent mean spin source - Maxim Dvornikov (Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation)   (Sala de Grados (1st floor))
17:55 A second look to the Polyakov Loop Nambu-Jona-Lasinio model at finite baryonic density - Dr. O. Ivanitskyi / M. Angeles Pérez García   (Sala de Grados (1st floor))
12:10 Neutron stars in modified theories of gravity - models, astrophysical implications and gravitational wave emission - Daniela Doneva (University of Tuebingen)   (Aula M2 (ground floor))
12:50 Measuring H_0 in PTA with gravitational waves (Russian-Iberian congress) - Domenec Espriu   (Aula M2 (ground floor))
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