We will have online presentations June 30 - July 2, 2020 using the Zoom video conference software. Remote connection information will be sent to accepted participants a few days prior to the start of the program.
Please note that all times are in Eastern Daylight Savings Time
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Tuesday, 30 June, 2020 |
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Time |
Session |
Speaker |
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9:00 AM - 9:30 AM |
Connect via Zoom - Online |
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9:30 AM - 9:40 AM |
Welcome |
Thomas Glasmacher Jorge Piekarewicz |
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9:40 AM - 10:50 AM |
Introduction to modeling the core of neutron stars – Part 1 |
V. Dexheimer |
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10:50 AM - 12:00 PM |
Introduction to modeling the core of neutron stars – Part 2 |
V. Dexheimer |
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12:00 PM - 1:30 PM |
Break |
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1:30 PM - 2:30 PM |
The physics of supernova explosions and neutron star mergers – Part 1 |
L. Roberts |
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2:30 PM - 3:30 PM |
The physics of supernova explosions and neutron star mergers – Part 2 |
L. Roberts |
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3:30 PM – 3:50 PM |
Break |
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3:50 PM - 5:00 PM |
Laboratory constraints for the equation of state of neutron stars – Part 1 |
P. Danielewicz |
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Wednesday, 1 July, 2020 |
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Time |
Session |
Speaker |
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9:40 AM - 10:50 AM |
Laboratory constraints for the equation of state of neutron stars – Part 2 |
P. Danielewicz |
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10:50 AM - 12:00 PM |
Deconfined quarks and phase transitions in the core of neutron stars – Part 1 |
T. Klähn |
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12:00 PM - 1:30 PM |
Break |
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1:30 PM - 2:30 PM |
Deconfined quarks and phase transitions in the core of neutron stars – Part 2 |
T. Klähn |
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2:30 PM - 3:30 PM |
General relativity (including the formalism to describe stellar rotation and magnetic fields) and stellar cooling - Part 1 |
R. Negreiros |
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3:30 PM – 3:50 PM |
Break |
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3:50 PM – 5:10 PM 3:50 PM – 4:40 PM 4:40 PM – 5:10 PM |
Interactive activities Graduate students only Everyone |
R. Negreiros P. Danielewicz T. Klähn |
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Thursday, 2 July, 2020 |
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Time |
Session |
Speaker |
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9:40 AM - 10:50 AM |
General relativity (including the formalism to describe stellar rotation and magnetic fields) and stellar cooling – Part 2 |
R. Negreiros |
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10:50 AM - 12:00 PM |
General relativity (including the formalism to describe stellar rotation and magnetic fields) and stellar cooling – Part 3 |
R. Negreiros |
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12:00 PM - 1:30 PM |
Break |
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1:30 PM - 2:30 PM |
Deconfined quarks and phase transitions in the core of neutron stars – Part 3 |
T. Klähn |
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2:30 PM - 3:30 PM 2:30 PM – 3:00 PM 3:00 PM - 3:30 PM |
Interactive activities Graduate students only Everyone |
V. Dexheimer P. Danielewicz R. Negreiros |
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3:30 PM – 3:50 PM |
Break |
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3:50 PM - 5:00 PM |
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5:00 PM |
Adjourn |
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