The Structure and Signals of Neutron Stars, from Birth to Death

Speaker List

• Michalis Agathos
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    Probing the neutron star equation of state with second-generation gravitational wave detectors

• Deborah Aguilera (Deutsches Zentrum fuer Luft- und Raumfahrt e.V., Bremen, Germany)
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    Quiescent thermal emission of neutron stars in LMXBs

• Mark Alford (Washington University in St. Louis, USA)
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    Hybrid stars: how can we identify them ?

• Robert Archibald
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    Repeated, Delayed Torque Instabilities Following Flux Enhancement in the Magnetar 1E 1048.1 5937

• Zaven Arzoumanian (C)
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    The Neutron Star Interior Composition Explorer: An X-ray Astrophysics Facility Dedicated to Neutron Star Science

• François Aymard (LPC Caen, France)
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    Surface properties of nuclei embedded in a nucleon gas in the framework of the Extended Thomas-Fermi theory

• Andreas Bauswein (Department of Physics, Aristotle University of Thessaloniki)
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    Equation-of-state dependence of neutron-star mergers

• Andrei Beloborodov (Columbia University)
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    Magnetic energy dissipation and emission from magnetars

• Edo Berger (Harvard, USA)
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    Neutron Star Binary Mergers as the Progenitors of Short GRBs

• Federico Bernardini (w)
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    The tormented quiescence of the transient neutron star low mass X-ray binary Centaurus X-4

• Mohsen Bigdeli (University of Zanjan)
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    LOCV approach and core-crust transition in neutron stars

• Anton Biryukov
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    The effects of a neutron star translational and rotational motion in observable timing and evolution of radiopulsars

• David Blaschke (University of Wroclaw)
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    Symmetry energy and neutron star radii

• Alfio Bonanno (INAF-Catania)
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    The neutron star in Cassiopeia A: equation of state, superfluidity, and Joule heating

• M. Bronzato de Avellar (IAG in San Paulo, Brasil)
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    New results of the time lags in the QPO's of 4U 1636-53

• Niccolò Bucciantini (INAF Osservatorio di Arcetri)
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    GRB central engines

• Rudiney Casali (Institut de Physique Nucléaire de Lyon)
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    Stellar compact objects under strong magnetic fields

• Deepto Chakrabarty (M)
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    Probing the neutron star equation of state through X-ray timing

• Manoneeta Chakraborty (Tata Institute of Fundamental Research)
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    X-ray Bursts from Accreting Neutron star LMXBs

• Nicolas Chamel (Universitè Libre de Bruxelles, Belgium)
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    Vela Pulsar Glitches and Nuclear Superfluidity

• Maria Chernyakova (D)
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    Multiwavelength properties of gamma-ray loud binaries.

• Cecilia Chirenti (UFABC)
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    Magnetic fields and r-modes in slowly rotating relativistic neutron stars

• Andrey Chugunov (I)
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    New possible class of rapidly rotating neutron stars

• Rafael C. R. de Lima (Universidade do Estado de Santa Catarina)
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    Effect of strong magnetic fields on the nuclear “pasta” phase structure

• Pawel Danielewicz (East Lansing, MSU (USA))
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    Constraints on the Equation of State of Nuclear Matter from Heavy-Ion Collisions and from Structure

• Nathalie Degenaar (University of Michigan)
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    Probing the crusts of transiently accreting neutron stars

• M. De Pasquale (Mullard Space Science Laboratory - University College London)
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    GRB 130831A: The Birth and Death of a Magnetar at z=0.5

• Veronica Dexheimer (Kent State University)
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    Equation of State for Hybrid Compact Stars

• Jason Dexter (UC Berkeley)
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    Spectral signatures of super-luminous supernovae powered by magnetars and black holes

• Jaroslaw Dyks (Nicolaus Copernicus Astronomical Center)
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    Azimuthally-structured radio beams of pulsars

• Khaled Elshamouty (University of Alberta)
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    Testing the Impact of Surface Temperature Inhomogeneities on Quiescent Neutron Star Mass/Radius Determinations

• Cristobal Espinoza (P)
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    The glitch activity of the Crab pulsar

• Anthea Fantina (Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles)
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    Unified equations of state of dense matter: nuclear-matter properties …..

• Sofie Fehlmann (University of Basel)
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    Simulations of X-ray Bursts and Superbursts

• Plamen Fiziev (Foundation of Theoretical and Computational Physics and Astrophysics (TCPA) Sofia University)
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    Compact static stars in minimal dilatonic gravity

• Luca Franci (Università di Parma)
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    Numerical studies of the dynamical bar-mode instability in rapidly rotating relativistic stars

• Paulo Freire (MPI Bonn)
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    Direct formation of millisecond pulsars from rotationally delayed accretion-induced collapse of massive white dwarfs

• Kenji Fukukawa (INFN Sezione di Catania)
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    Quark-Model Baryon-Baryon Interaction and Its Prospects in the Nuclear Matter Physics

• Michael Gabler (MPA Garching)
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    Superfluid magneto-elastic oscillations in Magnetars

• Ulrich Geppert (DLR and University of Zielona Gora)
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    Radio pulsar emission and crustal field evolution

• Bruno Giacomazzo
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    Magnetic Field Effects in the Merger of Binary Neutron Stars

• Janusz Gil (University of Zielona Gora)
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    Radio pulsar emission and crustal field evolution

• Ramandeep Gill (CITA (University of Toronto))
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    Statistical ages and the cooling rate of X-ray dim isolated neutron stars

• Kostas Glampedakis
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    Three evolutionary paths for magnetar oscillations

• Stefan Gmuca (Institute of Physics, Slovak Academy of Sciences)
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    Dirac density functional for dense matter

• Peter Gonthier (Hope College)
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    Compton Scattering Cross Sections in Strong Magnetic Fields: Advances for Neutron Star Applications

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    Population synthesis of radio and gamma-ray normal, isolated pulsars using Markov Chain Monte Carlo

• Leonardo Gualtieri (Rome University "La Sapienza", Italy)
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    On the gravitational signal from tidally deformed neutron stars in coalescing binaries

• Sebastien Guillot (M)
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    The neutron star radius and the dense-matter equation of state

• Miguel Gullón (University of Alicante)
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    Population synthesis of Isolated Neutron Stars

• Francesca Gulminelli (LPC and Univ.of Caen)
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    Phase diagram of nuclear matter in the stellar medium

• Mikhail Gusakov
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    Instability windows and evolution of rapidly rotating neutron stars

• Pawel Haensel (Nicholaus Copernicus Astronomical Centre, Warsaw, Poland)
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    Neutron stars with hyperon cores: stellar radii and EOS near nuclear density

• Alice Harding (NASA Goddard Space Flight Center)
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    Studying Pulsars with the Fermi Gamma-Ray Space Telescope

• Craig Heinke (University of Alberta)
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    Probing the neutron star equation of state through X-ray spectroscopy

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    Probing the neutron star equation of state through X-ray spectroscopy

• Matthias Hempel (B)
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    Effects of the symmetry energy in core-collapse supernovae

• Ricardo Heras (University College London)
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    Energy transformations in the birth of neutron stars

• Tanja Hinderer (Caltech, USA)
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    Extracting information on the neutron star equation of state via gravitational waves from binary inspirals

• Wynn Ho (U)
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    Tests of the nuclear equation of state and superfluid and superconducting gaps using the Cassiopeia A neutron star

• Jorge Horvath (I)
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    Evolution of relativistic binary systems

• Igor Iosilevskiy (Joint Institute for High Temperature (Russian Academy of Science), Moscow Institute of Physics and Technology (State University))
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    Enthalpic and entropic phase transitions in high energy density nuclear matter

• Hans Thomas Janka (MPI Garching)
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    Review talk on numerical modelling of neutron star coalesence and their remnants.

• Elena Kantor
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    g-modes in superfluid neutron stars

• David Keitel (Albert Einstein Institute)
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    Searching for pulsars with Einstein@Home

• Aida Kirichenko (Ioffe Physical Technical Institute)
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    New multiwavelength observations of two gamma-ray pulsars J0357+3205 and J1357-6429

• Paul Lasky (School of Physics, melbourne University)
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    Nuclear equation of state from observations of short gamma-ray burst remnants

• Manuel Linares (I)
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    Neutron star metamorphosis: from sub-luminous accretion to rotation-powered quiescence

• Jerome Margueron (IPN Lyon, France)
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    Role of superfluidity close to the neutron drip line

• Toshiki Maruyama (Japan Atomic Energy Agency)
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    Inhomogeneous structures of neutron star crust and mechanical properties

• Tomoyuki Maruyama (Nihon University)
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    Rapid Spin-Deceleration through Asymmetric Neutrino Emission in Magnetized Proto-Neutron Stars

• Andrew Melatos (University of Melbourne, Australia)
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    Superfluidity and superconductivity in neutron stars

• Gogi Melikidze (University of Zielona Gora)
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    What makes magnetars (as well as normal pulsars) radio laud?

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    Radio pulsar emission and crustal field evolution

• Debora Menezes (Universidade Federal de Santa Catarina)
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    SU(3) symmetric hypernuclear matter and related stellar properties

• Roberto Mignani (INAF/IASF)
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    X-ray observations of gamma-ray pulsars detected by Fermi

• Sergey Moiseenko (Space Research Institute)
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    Neutron star formation on magnetorotational supernova explosion

• Hamidreza Moshfegh (University of Tehran)
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    Obtaining the neutron star gravitational mass limit in the frame work of the LOCV method

• Toshio Nakano (University of tokyo)
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    Clues to the formation and evolution of magnetars from X-ray observations of the associated supernova remnants

• Lubos Neslusan (Astronomical Institute, Slovak Academy of Sciences)
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    Linkup of non-rotating neutron-star and outer-Schwarzschild metrics

• Ralph Neuhaeuser (U Jena)
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    Kinematics, ages, and Equation-of-State of nearby Neutron Stars

• Tsuneo Noda (Kurume Institute of Technology)
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    Thermal Evolution of Compact Stars with Color Superconducting Quark Matter

• Ken'ichi Nomoto
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    Formation of Neutron Stars from the ONeMg Core of Super-­‐AGB Stars

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    Formation of Neutron Stars from the ONeMg Core of Super-AGB Stars

• Felipe Olivares E. (Universidad Andrés Bello)
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    Multiwavelength analysis of three GRB-associated SNe in the context of the full GRB-SN sample

• Christian Ott (Caltech, USA)
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    Gravitational Waves from Core-Collapse Supernovae

• Benjamin Owen (Penn State, USA)
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    Continuous gravitational waves and neutron star microphysics

• Giuseppe Pagliara
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    The birth of quark stars

• Giulia Pagliaroli (INFN - LNGS)
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    Electromagnetic signals from bare strange stars

• Helena Pais (University of Coimbra)
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    Nuclear pasta phase in core-collapse supernova matter

• Cristina Pallanca
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    Optical companions to binary Millisecond Pulsars in Globular Clusters: the case of IGR J18245-2452/PSR J1824-2452I

• Cristiano Palomba (INFN Roma)
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    Results of the search for continuous gravitational wave signals from known pulsars

• Andrea Passamonti (INAF-Observatory of Rome)
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    Superfluid and superconducting magnetars and QPO spectrum

• Alessandro Pastore (ULB)
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    Neutrino mean free path in asymmetric nuclear matter

• Albino Perego (TU Darmstadt, Institut für Kernphysik Theoriezentrum)
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    Neutrino-driven wind from the aftermath of binary neutron star mergers

• M. A. Perez-Garcia (University of Salamanca and IUFFyM)
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    Finite temperature effects in the crust of neutron stars

• Kristian Petrik (Institute of Physics, Slovak Academy of Sciences)
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    New approach to an effective density dependence within an advanced relativistic mean-field theory.

• Elena Pian (INAF, Italy)
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    The connection between core-collapse supernovae and Gamma-Ray Bursts

• Carlotta Pittori (ASDC and INAF-OAR)
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    Gamma-ray emission and variability of the Crab Nebula above 100 MeV: theoretically challenging AGILE observations

• Jose Pons (University of Alicante, Spain)
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    Towards the great unification of neutron stars

• Sergei Popov (SAI Moscow)
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    Origin and evolution of magnetars

• Constança Providência (University of Coimbra)
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    The symmetry energy and neutron star properties

• Adriana Raduta (IFIN-HH)
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    Clusterized nuclear matter in the (proto-)neutron star crust and the symmetry energy

• Scott Ransom (National Radio Astronomy Observatory)
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    Nuclear Physics at Two Kiloparsecs with Millisecond Pulsars

• Massimiliano Razzano
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    The first variable gamma-ray pulsar: challenging the models of high-energy magnetospheric emission

• Nanda Rea (nstitute of Space Sciences (CSIC-IEEC), Barcelona, ES)
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    The extreme activity of strong and low magnetic magnetars

• Sanjay Reddy (U)
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    The thermal and electrical conductivity of neutron star matter

• Luciano Rezzolla (AEI)
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    MAGNETIC FIELDS IN RELATIVISTIC COMPACT-OBJECT BINARIES

• Arnau Rios Huguet (University of Surrey)
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    The equation of state from chiral forces in the Green's functions approach

• Dirk Rischke (Institut für Theoretische Physik Johann Wolfgang Goethe-Universität)
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    Inhomogeneous phases in dense strongly interacting matter - a generic phenomenon?

• Friedrich Roepke (MPA Garching)
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    Combustion processes in compact objects

• Juergen Schaffner-Bielich (Institut fuer Theoretische Physik, Goethe Universitaet, Frankfurt)
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    Strangeness in Compact Stars

• Andreas Schmitt (Vienna University of Technology)
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    Sound modes and instabilities in a relativistic superfluid

• Paul Scholz (McGill University)
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    The long-term post-outburst spin down of low magnetic field magnetar Swift J1822.3-1606

• Stefan Schramm (Frankfurt Institute for Advanced Studies Johann Wolfgang Goethe Universität)
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    Compact stars and general constraints on exotic phases

• Hans-Josef Schulze (INFN Sezione di Catania)
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    The Equation of State of Neutron Star Matter

• Armen Sedrakian (Frankfurt University)
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    Effects of superfluidity on cooling of compact stars

• Roshan Sellahewa (University of Surrey)
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    Properties of Infinite Nuclear Matter and Neutron Star Matter with the Gogny Interaction

• Peter Senger (GSI Helmholtzzentrum für Schwerionenforschung)
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    Exploring dense nuclear matter with heavy-ion collisions

• Miroslav Shaltev (Albert Einstein Institute, Hannover)
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    Follow-up searches for continuous gravitational waves

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    Semicoherent search optimization using real detector data

• Peter Shternin
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    Transport coefficients of nuclear matter in neutron star cores in the BHF framework

• Hajime SOTANI (Kyoto University)
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    Neutron stars and nuclear matter parameters

• Rodrigo Souza (IAG - USP Sao Paulo)
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    Statistical measure of complexity in compact stars with global charge neutrality

• Luigi Stella (INAF - OAR)
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    Measuring the Mass-Radius Relation of Neutron Stars with the Large Observatory for X-ray Timing (LOFT)

• Holger Stiele (Shanghai Astronomical Observatory)
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    Millihertz Quasi-periodic Oscillations in 4U 1636-536: Pulse Profile and Energy Spectrum

• Kohsuke Sumiyoshi (Numazu College of Technology, Japan)
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    Data sets of equation of state for core-collapse supernovae: their impact on dynamics and signals

• Andrzej Szary (Kepler Institute of Astronomy, Univ. Zielona Gora, Poland)
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    Partially Screened Gap in Pulsars

• Adam Szmagliński (Institute of Physics, Cracow University of Technology)
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    PROPERTIES OF LOCALIZED PROTONS IN NEUTRON STAR MATTER AT FINITE TEMPERATURES

• Ali Taani (Al-Balqa' Applied University- Aqaba University College)
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    Formation and evolution of pulsars via the accretion induced collapse of white dwarfs

• Shuta Tanaka (Institute for Cosmic Ray Research, The University of Tokyo)
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    Constraint of Pulsar Wind Properties from Induced Compton Scattering off Radio Pulses

• Gabriele Taranto (INFN)
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    Nucleon effective masses within the Brueckner-Hartree-Fock theory: Impact on stellar neutrino emission

• Thomas Tauris (MPIfR Bonn)
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    Ultra-stripped Type Ic supernovae from close binary evolution

• Laura Tolos (ICE (CSIC-IEEC))
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    Transport coefficients in superfluid neutron stars

• Chris Van Den Broeck (Nikhef)
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    Testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing binary neutron stars

• Daniele Viganò
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    Physics of isolated neutron stars from their X-ray emission

• Xavier Vinas (Universitat de Barcelona)
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    Equation of State for Neutron Stars based on a microscopic energy density functional : from the outer crust to the core

• Dmitry Yakovlev (IOFFE Institute)
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    Theory of cooling neutron stars

• Nobutoshi Yasutake (Chiba Institute of Technology)
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    Pasta structures in quark-hadron phase transition by non-local NJL model

• Dario Zappalà (INFN Cezione di Catania)
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    Constraining the Field Correlator Method by Neutron Star observations

• Sergey Zharikov
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    Radiation efficiencies of the pulsars (current update).