Search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar

The physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mode oscillations in their parent neutron star that couple to gravitational-wave emission. In August 2006, a timing glitch was observed in the radio emission of PSR B0833-45, the Vela pulsar. At the time...

Full description

Bibliographic Details
Main Authors: Barsotti, Lisa (Contributor), Blackburn, Lindy L. (Contributor), Bodiya, Timothy Paul (Contributor), Cao, Jianshu (Contributor), Corbitt, Thomas R. (Contributor), Donovan, Frederick J. (Contributor), Duke, I. (Contributor), Evans, Matthew J. (Contributor), Foley, Stephany (Contributor), Fritschel, Peter K. (Contributor), Harry, Gregory (Contributor), Hughey, Barbara (Contributor), Katsavounidis, Erotokritos (Contributor), MacInnis, Myron E. (Contributor), Markowitz, Jared John (Contributor), Mason, Kenneth R. (Contributor), Matichard, Fabrice (Contributor), Mavalvala, Nergis (Contributor), Mittleman, Richard K. (Contributor), Sarin, P. (Contributor), Shapiro, B. (Contributor), Shoemaker, David H. (Contributor), Smith, N. D. (Contributor), Stein, Andrew J. (Contributor), Stein, Leo Chaim (Contributor), Waldman, Samuel J. (Contributor), Weiss, Rainer (Contributor), Wipf, Christopher C. (Contributor), Zucker, Michael E. (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Chemistry (Contributor), Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: American Physical Society, 2011-05-31T15:00:27Z.
Subjects:
Online Access:Get fulltext