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Invitation to the seminar — The maximum gravitational mass and deformation of magnetized rotating strange quark stars
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Invitation to the seminar — The maximum gravitational mass and deformation of magnetized rotating strange quark stars
Invitation to the seminar — The maximum gravitational mass and deformation of magnetized rotating strange quark stars
The seminar will happen online. The more information in regards to the meeting link will be further known closer to the event itself.
More Details
| Date from | 29.06.2023 / 13:00 |
| Date to | 29.06.2023 / 14:00 |
| All day | No |
| For students | Yes |
| For the public | No |
| Invite only | Yes |
More Details
| Date from | 29.06.2023 / 13:00 |
| Date to | 29.06.2023 / 14:00 |
| All day | No |
| For students | Yes |
| For the public | No |
| Invite only | Yes |
Hosted by Fatima Kayanikhoo The abstract:
|
| Strange
quark stars (SQS) are a possible type of compact object that may be
created after the proto-neutron star state, through a second explosion.
The core magnetic field of the quark stars may reach magnetic fields of
10^{18} G. The other interesting property of compact objects which
affects the dynamic and configuration of the star is spin. Rotating
compact objects are supposed to be stable with larger maximum
gravitational masses compared to the non-rotating models. We studied the
structure of SQSs in the presence of strong magnetic fields with
different rotational frequencies. I will give an overview of SQS and
discuss the model we provided for the equation of state and structure of
SQS as well as remark on the impact of rotation and magnetic field on
the shape and gravitational mass limits of SQS. |
