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Participant |
Cipolletta, Federico | |||||||
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Institution |
Università di Roma, "Sapienza" - Piazzale Aldo Moro, 5 - Roma - - Italy | |||||||
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Session |
NS1 |
Accepted |
No |
Order |
4 |
Time |
15:35 | 20' |
|
Talk |
Oral abstract |
Title |
Structure And Stability For Realistic Rapidly Rotating NS: Full GR Treatment | |||||
| Coauthors | C. Cherubini, S. Filippi, J. A. Rueda and R. Ruffini | |||||||
|
Abstract |
I will present a full general relativistic treatment for the problem of equilibrium of rapidly rotating realistic Neutron Stars, taking into account some peculiar limits to define a "stability region" in which numerical models exists. I will focus on three realistic Equations of State, showing how this kind of problem is approached and some numerical results describing the structure of such compact objects. I will also discuss characteristics of spacetime external to the NS (e.g. quadrupole mass moment) and universal (EOS-independent) relations. |
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Pdf file |
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Session |
NS2 |
Accepted |
Yes |
Order |
4 |
Time |
16:30 | 30' |
|
Talk |
Oral abstract |
Title |
Structure And Stability For Realistic Rapidly Rotating NS: Full GR Treatment | |||||
| Coauthors | C. Cherubini, S. Filippi, J. A. Rueda and R. Ruffini | |||||||
|
Abstract |
I will present a full general relativistic treatment for the problem of equilibrium of rapidly rotating realistic Neutron Stars, taking into account some peculiar limits to define a "stability region" in which numerical models exists. I will focus on three realistic Equations of State, showing how this kind of problem is approached and some numerical results describing the structure of such compact objects. I will also discuss characteristics of spacetime external to the NS (e.g. quadrupole mass moment) and universal (EOS-independent) relations. |
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Pdf file |
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