Gravitational radiation from a rotating magnetic dipole

Authors

  • S. Hacyan

DOI:

https://doi.org/10.31349/RevMexFis.63.5.466

Keywords:

Gravitational waves, neutron stars

Abstract

The gravitational radiation emitted by a rotating magnetic dipole is calculated. Formulas for the polarization amplitudes and the radiated power are obtained in closed forms. A comparison is made with other sources of gravitational and electromagnetic radiation, particularly neutron stars with extremely powerful magnetic fields.

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Published

2017-01-01

How to Cite

[1]
S. Hacyan, “Gravitational radiation from a rotating magnetic dipole”, Rev. Mex. Fís., vol. 63, no. 5, pp. 466–468, Jan. 2017.

Issue

Vol. 63 No. 5 (2017): Revista Mexicana de Física

Section

Articles

License

Copyright (c) 2018 Revista Mexicana de Física

Creative Commons License

This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.

Authors retain copyright and grant the Revista Mexicana de Física right of first publication with the work simultaneously licensed under a CC BY-NC-ND 4.0 that allows others to share the work with an acknowledgement of the work's authorship and initial publication in this journal.

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