Constraining the Equation of State of Neutron Stars with Genral Relativity

Tiziana Di Salvo; Natale Robba; Rosario Iaria; Fabio D'Antona; Giuseppe Lavagetto

Constraining the Equation of State of Neutron Stars with Genral Relativity

Tiziana Di Salvo, Natale Robba, Rosario Iaria, Fabio D'Antona, Giuseppe Lavagetto

Fisica e Chimica - Emilio Segrè

Risultato della ricerca: Chapter

Abstract

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.

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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Di Salvo, T., Robba, N., Iaria, R., D'Antona, F., & Lavagetto, G. (2005). Constraining the Equation of State of Neutron Stars with Genral Relativity. In AIP Conference Proceedings (pagg. 214-214). (AIP CONFERENCE PROCEEDINGS).

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abstract = "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.",

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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

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