Importance of constraining the dense matter Equation of State in pulsar astrophysics (original) (raw)

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PSR J1847-0130: A Radio Pulsar with Magnetar Spin Characteristics Cover Page

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X‐Ray Observations of the High Magnetic Field Radio Pulsar PSR J1814−1744 Cover Page

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Modelling of the surface magnetic field in neutron stars: Application to radio pulsars Cover Page

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Pulsar Physics without Magnetars Cover Page

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Non-corotating models for pulsar magnetospheres Cover Page

Radio emission from a pulsar’s magnetic pole revealed by general relativity

Science, 2019

Binary pulsars are affected by general relativity (GR), causing the spin axis of each pulsar to precess. We present polarimetric radio observations of the pulsar PSR J1906+0746 that demonstrate the validity of the geometrical model of pulsar polarization. We reconstruct the (sky-projected) polarization emission map over the pulsar’s magnetic pole and predict the disappearance of the detectable emission by 2028. Two tests of GR are performed using this system, including the spin precession for strongly self-gravitating bodies. We constrain the relativistic treatment of the pulsar polarization model and measure the pulsar beaming fraction, with implications for the population of neutron stars and the expected rate of neutron star mergers.

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Radio emission from a pulsar’s magnetic pole revealed by general relativity Cover Page

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Discovery of Two High Magnetic Field Radio Pulsars Cover Page

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VLT / NACO observations of the high-magnetic field radio pulsar PSR J1119-6127 Cover Page

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Pulsar magnetospheres in general relativity Cover Page

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Origin of pulsar radio emission. I. High frequency data Cover Page