Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/48827
Citations | ||
Scopus | Web of Science® | Altmetric |
---|---|---|
?
|
?
|
Type: | Journal article |
Title: | Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors |
Author: | Abbott, B. Abbott, R. Adhikari, R. Ageev, A. Allen, B. Amin, R. Anderson, S. Anderson, W. Araya, M. Armandula, H. Asiri, F. Aufmuth, P. Aulbert, C. Babak, S. Balasubramanian, R. Ballmer, S. Barish, B. Barker, C. Barker, D. Barnes, M. et al. |
Citation: | Physical Review D: Particles, Fields, Gravitation and Cosmology, 2004; 69(8):082004-1-082004-16 |
Publisher: | American Physical Soc |
Issue Date: | 2004 |
ISSN: | 1550-7998 1550-2368 |
Statement of Responsibility: | B. Allen...C.J. Killow...C. Kim...D. Ottaway...et al. |
Abstract: | Data collected by the GEO 600 and LIGO interferometric gravitational wave detectors during their first observational science run were searched for continuous gravitational waves from the pulsar J1939+2134 at twice its rotation frequency. Two independent analysis methods were used and are demonstrated in this paper: a frequency domain method and a time domain method. Both achieve consistent null results, placing new upper limits on the strength of the pulsar’s gravitational wave emission. A model emission mechanism is used to interpret the limits as a constraint on the pulsar’s equatorial ellipticity. |
Rights: | ©2004 American Physical Society |
DOI: | 10.1103/PhysRevD.69.082004 |
Published version: | http://dx.doi.org/10.1103/physrevd.69.082004 |
Appears in Collections: | Aurora harvest Physics publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
hdl_48827.pdf | Published version | 790.43 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.