Modulating the experimental signature of a stochastic gravitational wave background

Physical Review D

Volumn 64, Issue 8, 2001, Pages

  Finn, Lee Samuel ^a   Lazzarini, Albert ^b  

^a PENNSYLVANIA STATE UNIVERSITY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; EXPERIMENT; GRAVITY; MEASUREMENT; RELIABILITY; STOCHASTIC MODEL; WAVEFORM;

EID: 4243207250     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.64.082002     Document Type: Article

References (30)

1. M. Maggiore, Phys. Rep. 331, 283 (2000).
2. W. O. Hamilton et al., in Omnidirectional Gravitational Radiation Observatory, edited by W. F. Velloso, Jr., O. D. Aguiar, and N. S. Magalhaes (World Scientific, Singapore, 1997), pp. 19-26.
3. M. Cerdonio et al., Class. Quantum Grav. 14, 1491 (1997).
4. P. Astone et al., in Omnidirectional Gravitational Radiation Observatory, edited by W. F. Velloso, Jr., O. D. Aguiar, and N. S. Magalhaes (Ref. [2]), pp. 39-50.
5. H. Lück et al., in Gravitational Waves, Proceedings of the Third Edoardo Amaldi Conference, edited by S. Meshkov, AIP Conf. Proc. No. 523 (AIP, Melville, NY, 2000), pp. 119-127.
6. M. Coles, in Gravitational Waves, Proceedings of the Third Edoardo Amaldi Conference, edited by S. Meshkov, AIP Conf. Proc. No. 523 (AIP, Melville, NY, 2000).
7. D. Blair, in Gravitational Waves, Proceedings of the Third Edoardo Amaldi Conference, edited by S. Meshkov, AIP Conf. Proc. No. 523 (AIP, Melville, NY, 2000).
8. F. Marion and The VIRGO Collaboration, in Gravitational Waves, Proceedings of the Third Edoardo Amaldi Conference, edited by S. Meshkov, AIP Conf. Proc. No. 523 (AIP, Melville, NY, 2000), pp. 110-118.
9. M. Ando and K. Tsubono, in Gravitational Waves, Proceedings of the Third Edoardo Amaldi Conference, S. Meshkov, AIP Conf. Proc. No. 523 (AIP, Melville, NY, 2000).
10. A. Abramovici et al., Science 256, 325 (1992).
11. N. Solomonson, W. O. Hamilton, W. Johnson, and B. Xu, Rev. Sci. Instrum. 65, 174 (1994).
12. E. Mauceli et al., Phys. Rev. D 54, 1264 (1996).
13. R. H. Dicke, Rev. Sci. Instrum. 17, 268 (1946).
14. A. group (private communiation).
15. P. F. Michelson, Mon. Not. R. Astron. Soc. 227, 933 (1987).
16. N. Christensen, Phys. Rev. D 46, 5250 (1992).
17. É. É. Flanagan, Phys. Rev. D 48, 2389 (1993).
18. B. Allen and J. D. Romano, Phys. Rev. D 59, 102001 (1999).
19. W. E. Althouse et al., Rev. Sci. Instrum. 72(7), 3086 (2001).
20. A. Lazzarini and R. Weiss, Technical Report No. LIGO-E950018-02-E, Laser Interferometer Gravitational Wave Observatory, internal working note.
21. The advanced LIGO noise curves are available from the LIGO II Concept Book, available at http://www.ligo.caltech.edu/ ~ligo2/scripts/noframedocs.html.
22. 0≈900 Hz were provided by K. Strain (private communication).
23. G. J. Feldman and R. D. Cousins, Phys. Rev. D 57, 3873 (1998).
24. J. Hough, J. R. Pugh, R. Bland, and R. W. Drever, Nature (London) 254, 498 (1975).
25. R. L. Zimmerman and R. W. Hollings, Astrophys. J. 241, 475 (1980).
26. K. Compton, D. Nicholson, and B. Schutz, Proceedings of the 7th Marcel Grossman Meeting on General Relativity (World Scientific, Singapore, 1994), p. 1078.
27. P. Astone, M. Bassan, and P. Bonifazi, Astron. Astrophys. 19, 343 (1999).
28. P. Astone et al., Astron. Astrophys. 351, 811 (1999).
29. P. Astone, V. Ferrari, M. Maggiore, and J. Romano, Int. J. Mod. Phys. D 9, 361 (2000).
30. J. S. Bendat and A. G. Piersol, Random Data Analysis and Measurement Procedures, 2nd ed. (Wiley, New York, 1986).