Speaker
Prasanta Bera (Open University of Israel)
Date & Time
Thu, 05 October 2023, 15:30 to 17:00
Venue
Emmy Noether Seminar Room & Online
Resources
Abstract
Compact stars are the dense, final stage of normal stars. Due to their small size and large mass, compact stars have a strong gravitational pull. They can also rotate very quickly and have powerful magnetic fields. These extreme properties allow compact stars to emit high-energy radiation. Finding the stable structure of a compact star with a strong magnetic field and rotation is a difficult task. This talk will discuss the numerical methods used to model compact stars and the astrophysical importance of these models.
Zoom link: https://icts-res-in.zoom.us/j/82882003877?pwd=IUw5evOKAYvwj3XHWQ2bKCou8mzsB3.1
Meeting ID: 828 8200 3877
Passcode: 088327