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SKA-Japan Pulsar Science with the Square Kilometre Array

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arxiv 1603.01951 v1 pith:2UEV5WSH submitted 2016-03-07 astro-ph.IM astro-ph.COastro-ph.HE

SKA-Japan Pulsar Science with the Square Kilometre Array

classification astro-ph.IM astro-ph.COastro-ph.HE
keywords pulsarpulsarsarrayblackkilometrescienceska-japansquare
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Square Kilometre Array will revolutionize pulsar studies with its wide field-of-view, wide-band observation and high sensitivity, increasing the number of observable pulsars by more than an order of magnitude. Pulsars are of interest not only for the study of neutron stars themselves but for their usage as tools for probing fundamental physics such as general relativity, gravitational waves and nuclear interaction. In this article, we summarize the activity and interests of SKA-Japan Pulsar Science Working Group, focusing on an investigation of modified gravity theory with the supermassive black hole in the Galactic Centre, gravitational-wave detection from cosmic strings and binary supermassive black holes, a study of the physical state of plasma close to pulsars using giant radio pulses and determination of magnetic field structure of Galaxy with pulsar pairs.

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