We report on an all-sky search for periodic gravitational waves in the frequency band 50-800Hz and with the frequency time derivative in the range of 0 through -6×10-9Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10× increase in computational efficiency, we have searched in two years of data collected during LIGO's fifth science run and have obtained the most sensitive all-sky upper limits on gravitational-wave strain to date. Near 150Hz our upper limit on worst-case linearly polarized strain amplitude h0 is 1×10-24, while at the high end of our frequency range we achieve a worst-case upper limit of 3.8×10-24 for all polarizations and sky locations. These results constitute a factor of 2 improvement upon previously published data. A new detection pipeline utilizing a loosely coherent algorithm was able to follow up weaker outliers, increasing the volume of space where signals can be detected by a factor of 10, but has not revealed any gravitational-wave signals. The pipeline has been tested for robustness with respect to deviations from the model of an isolated neutron star, such as caused by a low-mass or long-period binary companion. © 2012 American Physical Society.

All-sky search for periodic gravitational waves in the full S5 LIGO data / Abadie, J., Abbott, B., Abbott, R., Abbott, T., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Affeldt, C., Ajith, P., Allen, B., Allen, G., Amador Ceron, E., Amariutei, D., Amin, R., Anderson, S., Anderson, W., Arai, K., Arain, M., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 85:2(2012). [10.1103/physrevd.85.022001]

All-sky search for periodic gravitational waves in the full S5 LIGO data

ASTONE, PIA;COLLA, ALBERTO;COLOMBINI, MARZIA;CONTE, ANDREA;CORSI, ALESSANDRA;I. Di Palma;M. Drago;FRASCA, Sergio;E. Majorana;NATICCHIONI, LUCA;PALOMBA, Cristiano;RAPAGNANI, Piero;RICCI, Fulvio;F. Salemi;
2012

Abstract

We report on an all-sky search for periodic gravitational waves in the frequency band 50-800Hz and with the frequency time derivative in the range of 0 through -6×10-9Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10× increase in computational efficiency, we have searched in two years of data collected during LIGO's fifth science run and have obtained the most sensitive all-sky upper limits on gravitational-wave strain to date. Near 150Hz our upper limit on worst-case linearly polarized strain amplitude h0 is 1×10-24, while at the high end of our frequency range we achieve a worst-case upper limit of 3.8×10-24 for all polarizations and sky locations. These results constitute a factor of 2 improvement upon previously published data. A new detection pipeline utilizing a loosely coherent algorithm was able to follow up weaker outliers, increasing the volume of space where signals can be detected by a factor of 10, but has not revealed any gravitational-wave signals. The pipeline has been tested for robustness with respect to deviations from the model of an isolated neutron star, such as caused by a low-mass or long-period binary companion. © 2012 American Physical Society.
2012
01 Pubblicazione su rivista::01a Articolo in rivista
All-sky search for periodic gravitational waves in the full S5 LIGO data / Abadie, J., Abbott, B., Abbott, R., Abbott, T., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Affeldt, C., Ajith, P., Allen, B., Allen, G., Amador Ceron, E., Amariutei, D., Amin, R., Anderson, S., Anderson, W., Arai, K., Arain, M., et al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 85:2(2012). [10.1103/physrevd.85.022001]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/456033
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