Abstract
| Lingua originale | English |
|---|---|
| Titolo della pubblicazione ospite | AIP Conference Proceedings |
| Pagine | 214-214 |
| Numero di pagine | 1 |
| Stato di pubblicazione | Published - 2005 |
Serie di pubblicazioni
| Nome | AIP CONFERENCE PROCEEDINGS |
|---|
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Constraining the Equation of State of Neutron Stars with Genral Relativity. / Di Salvo, Tiziana; Robba, Natale; Iaria, Rosario; D'Antona, Fabio; Lavagetto, Giuseppe.
AIP Conference Proceedings. 2005. pag. 214-214 (AIP CONFERENCE PROCEEDINGS).Risultato della ricerca: Chapter
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TY - CHAP
T1 - Constraining the Equation of State of Neutron Stars with Genral Relativity
AU - Di Salvo, Tiziana
AU - Robba, Natale
AU - Iaria, Rosario
AU - D'Antona, Fabio
AU - Lavagetto, Giuseppe
PY - 2005
Y1 - 2005
N2 - When a radio pulsar breakes down by virtue of magnetodipole emission, its gravitational mass decreases accordingly. If the pulsar in hosted in a binary system, this mass loss will increase the orbital period of the system. We show that this relativistic effect can be indeed observable if the NS is fast and magnetized enough and that, if observed, it will help to put tight constraints on the equation of state of ultradense matter.
AB - When a radio pulsar breakes down by virtue of magnetodipole emission, its gravitational mass decreases accordingly. If the pulsar in hosted in a binary system, this mass loss will increase the orbital period of the system. We show that this relativistic effect can be indeed observable if the NS is fast and magnetized enough and that, if observed, it will help to put tight constraints on the equation of state of ultradense matter.
UR - http://hdl.handle.net/10447/22900
M3 - Chapter
T3 - AIP CONFERENCE PROCEEDINGS
SP - 214
EP - 214
BT - AIP Conference Proceedings
ER -