Global Magnetosphere Theory and Simulation | ||
Chair: Alice Harding | ||
9:15 | Welcome | |
9:30 | Spitkovsky | Numerical modeling of pulsar magnetospheres: from force-free to particles |
10:05 | Philippov | How do pulsars shine? |
10:40 | Discussion | |
11:00 | Break | |
11:30 | Contopoulos | The Aristotelian Equatorial Current Sheet |
12:05 | Discussion | |
12:30 | Lunch | |
Chair: Demos Kazanas | ||
2:00 | Timokhin | How much plasma can a pulsar make? |
2:35 | Belyaev | Pulsar Polar Cap and Y-point in PIC Simulations |
3:10 | Discussion | |
3:30 | Break | |
4:00 | Kalapotharakos | Towards the Understanding of the Gamma-ray Emission in Pulsar Magnetospheres: Models vs Fermi |
4:35 | Brambilla | Developing a specialized Particle-In-Cell code to study Pulsar Magnetospheres |
5:10 | Discussion |
Mode Changing and Variability | ||
Chair: Andrey Timokhin | ||
9:00 | Rankin | Radio pulsar phenomenology I : Geometry, Emission Heights and Identification of X and O modes |
9:35 | Mitra | Radio pulsar phenomenology II : Drifting Subpulses |
10:10 | Discussion | |
10:30 | Break | |
11:00 | Melkidze | Coherent Radio emission, PSG model and Drifting subpulses |
11:35 | Hermsen | The mystery of simultaneous pulsar moding in the X-ray and radio bands |
12:10 | Discussion | |
12:30 | Lunch | |
Chair: Wim Hermsen | ||
2:00 | Van Leeuwen | Pulsar mode changes and subpulse drift |
2:15 | Szary | A physically justified model of drifting subpulses. |
2:30 | Discussion | |
2:45 | Kargaltsev | Is there a useful connection between the pulsar magnetosphere geometry and PWN morphology? |
3:05 | Break | |
3:35 | Harding | Pulsar Variability and the Global Magnetosphere |
4:10 | Wadiasingh | Magnetar polarization |
4:25 | Arons | Ultra High Energy Cosmic Rays from Magnetars |
5:00 | Discussion | |
7:00 | Workshop Dinner | Siri's Chef's Secret, Greenbelt |
Emission Modeling and Magnetic Fields | ||
Chair: Kostas Kalapotharakos | ||
9:00 | Venter | Insights from Pulsar Light Curve Modeling |
9:10 | Seyffert | Toward a more rigorous statistical goodness of fit test for concurrent light curve fitting |
9:20 | Barnard | High-Energy Light Curves in an Offset Polar Cap B-Field Geometry |
9:30 | Discussion | |
9:45 | Shibata | X-ray and rotational luminosity correlation and magnetic heating of the radio pulsars |
10:15 | Discussion | |
10:25 | Break | |
10:55 | Hirotani | Leptonic acceleration in pulsar and black hole magnetospheres |
11:30 | Petri | Multipolar fields in neutron stars |
12:05 | Kazanas | Crab GeV Flares: Too much ado about not too much? |
12:20 | Discussion | |
12:30 | Lunch | |
2:00 | Gonthier | Magnetic field decay and unification of young and millisecond pulsar populations |
2:30 | Grenier | Phase-Resolved Spectroscopy of Millisecond Pulsars |
2:45 | Discussion | |
Present and Future Missions | ||
3:00 | Johnson | Pulsar Observations with Fermi |
3:35 | Break | |
4:05 | Arzoumanian | An X-ray Astrophysics Mission Dedicated to Neutron Stars: Capabilities and Status of NICER |
4:35 | Hunter | Measurement of Gamma-ray Polarization |
4:55 | Hays | ComPair/AMEGO |
5:15 | Discussion |