Understanding pulsar magnetospheres with the SKA

A. Karastergiou; S. Johnston; N. Andersson; R. Breton; P. Brook; C. Gwinn; N. Lewandowska; E. Keane; M. Kramer; J. -P. Macquart; M. Serylak; R. Shannon; B. Stappers; J. van Leeuwen; J. P. W. Verbiest; P. Weltevrede; G. Wright

arXiv · 1501.00126

Understanding pulsar magnetospheres with the SKA

A. Karastergiou·S. Johnston·N. Andersson·R. Breton·P. Brook·C. Gwinn·N. Lewandowska·E. Keane·M. Kramer·J. -P. Macquart·M. Serylak·R. Shannon·B. Stappers·J. van Leeuwen·J. P. W. Verbiest·P. Weltevrede·G. Wright

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Abstract

The SKA will discover tens of thousands of pulsars and provide unprecedented data quality on these, as well as the currently known population, due to its unrivalled sensitivity. Here, we outline the state of the art of our understanding of magnetospheric radio emission from pulsars and how we will use the SKA to solve the open problems in pulsar magnetospheric physics.

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A. Karastergiou, S. Johnston, N. Andersson, R. Breton, P. Brook, C. Gwinn, N. Lewandowska, E. Keane, M. Kramer, J. -P. Macquart, M. Serylak, R. Shannon, B. Stappers, J. van Leeuwen, J. P. W. Verbiest, P. Weltevrede, G. Wright. 2014-12-31. Understanding pulsar magnetospheres with the SKA. https://arxiv.org/abs/1501.00126

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