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Probing gravitation with pulsars

Published online by Cambridge University Press:  20 March 2013

Michael Kramer
Michael Kramer*
Affiliation:
MPI für Radioastronomy, Auf dem Hügel 69, 53121 Bonn, Germany email: [email protected] Jodrell Bank Centre for Astrophysics, University of ManchesterOxford Road, Manchester M13 9PL, UK email: [email protected]
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Abstract

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Radio pulsars are fascinating and extremely useful objects. Despite our on-going difficulties in understanding the details of their emission physics, they can be used as precise cosmic clocks in a wide-range of experiments – in particular for probing gravitational physics. While the reader should consult the contributions to these proceedings to learn more about this exciting field of discovering, exploiting and understanding pulsars, we will concentrate here on on the usage of pulsars as gravity labs.

Keywords

gravitationtechniques:radio astronomystars:neutronpulsars:general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 19 - 26
Copyright
Copyright © International Astronomical Union 2013

References

Börner, G., Ehlers, J. & Rudolph, E., 1975, A&A, 44, 417Google Scholar
Breton, R. P., et al., 2008, Science, 321, 104Google Scholar
Burgay, M., et al., 2003, Nature, 426, 531Google Scholar
Burgay, M., et al., 2005, ApJ, 624, L113CrossRefGoogle Scholar
Damour, T. & Deruelle, N., 1986, Ann. Inst. H. Poincaré (Physique Théorique), 44, 263Google Scholar
Damour, T. & Esposito-Farèse, G., 1996, Phys. Rev. D, 54, 1474Google Scholar
Damour, T. & Ruffini, R., 1974, Acad. des Sci. Paris Comptes Rendus Ser. Scie. Math., 279, 971Google Scholar
Damour, T. & Taylor, J. H., 1992, Phys. Rev. D, 45, 1840Google Scholar
Ferdman, R. D., et al., 2012, submittedGoogle Scholar
Freire, P. C. C., et al., 2012, MNRAS, 423, 3328Google Scholar
Hulse, R. A. & Taylor, J. H., 1975, ApJ, 195, L51Google Scholar
Kramer, M. & Stairs, I. H., 2008, Ann. Rev. Astr. Ap., 46, 541Google Scholar
Kramer, M. & Wex, N., 2009, Classical and Quantum Gravity, 26 (7), 073001CrossRefGoogle Scholar
Kramer, M., et al., 2006, Science, 314, 97Google Scholar
Liu, K., Wex, N., Kramer, M., Cordes, J. M., & Lazio, T. J. W., 2012, ApJ, 747, 1CrossRefGoogle Scholar
Lorimer, D. R. & Kramer, M., 2005, Handbook of Pulsar Astronomy. Cambridge University PressGoogle Scholar
Lyne, A. G., et al., 2004, Science, 303, 1153Google Scholar
Perera, B., et al., 2010, ApJ, 721, 1193CrossRefGoogle Scholar
Weisberg, J. M., Nice, D. J. & Taylor, J. H., 2010, ApJ, 722, 1030CrossRefGoogle Scholar
Will, C., 2006, Living Reviews in Relativity, 9, 1Google Scholar