de.mpg.escidoc.pubman.appbase.FacesBean
Deutsch
 
Hilfe Wegweiser Impressum Kontakt Einloggen
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT

Freigegeben

Konferenzbeitrag

Continuous Gravitational Wave Searches from Galactic Neutron Stars in the Advanced Detector Era

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

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

Externe Ressourcen
Es sind keine Externen Ressourcen verfügbar
Volltexte (frei zugänglich)
Es sind keine frei zugänglichen Volltexte verfügbar
Ergänzendes Material (frei zugänglich)
Es sind keine frei zugänglichen Ergänzenden Materialien verfügbar
Zitation

Wade, L., Siemens, X., Kaplan, D., Knispel, B., & Allen, B. (in preparation). Continuous Gravitational Wave Searches from Galactic Neutron Stars in the Advanced Detector Era.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-B342-6
Zusammenfassung
We consider a simulated population of galactic neutron stars. The rotational frequency of each neutron star evolves through a combination of electromagnetic and gravitational wave emission. The magnetic field strength determines the dipolar emission, and the ellipticity (a measure of a neutron star's deformation) determines the gravitational wave emission. We find the gravitational wave amplitude emitted by each star in the population and probe the areas of magnetic field strength and ellipticity parameter space that would result in a detection by Advanced LIGO. We show that in the absence of a detection, for fixed ellipticity, we can set lower bounds on the magnetic fields of young neutron stars.