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Continuous Gravitational Waves from Isolated Galactic Neutron Stars in the Advanced Detector Era

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons1452

Knispel,  Benjamin
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons40518

Allen,  Bruce
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Volltexte (frei zugänglich)

1209.2971
(Preprint), 627KB

PRD86_124011.pdf
(beliebiger Volltext), 555KB

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Zitation

Wade, L., Siemens, X., Kaplan, D. L., Knispel, B., & Allen, B. (2012). Continuous Gravitational Waves from Isolated Galactic Neutron Stars in the Advanced Detector Era. Physical Review D, 86: 124011. doi:10.1103/PhysRevD.86.124011.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-B311-3
Zusammenfassung
We consider a simulated population of isolated Galactic neutron stars. The rotational frequency of each neutron star evolves through a combination of electromagnetic and gravitational wave emission. The magnetic field strength dictates the dipolar emission, and the ellipticity (a measure of a neutron star's deformation) dictates the gravitational wave emission. Through both analytic and numerical means, we assess the detectability of the Galactic neutron star population and bound the magnetic field strength and ellipticity parameter space of Galactic neutron stars with or without a direct gravitational wave detection. While our simulated population is primitive, this work establishes a framework by which future efforts can be conducted.