E-resources
-
Abbott, B. P; Abernathy, M; Arain, M. A; Babak, S; Ballmer, S; Barker, D; Barton, M. A; Bassiri, R; Beveridge, N; Blackburn, J. K; Brau, J. E; Brinkmann, M; Cao, J; Caride, S; Cavaglià, M; Clark, J; Clayton, J. H; Conte, R; Coyne, D. C; Creighton, J. D. E; DeRosa, R; Donovan, F; Dumas, J.-C; Eberle, T; Effler, A; Evans, T; Feldbaum, D; Foley, S; Frei, M; Fricke, T. T; Fulda, P; Fyffe, M; Garofoli, J. A; Gretarsson, A. M; Hammer, D; Hanna, C; Harry, G. M; Haughian, K; Hirose, E; Howell, E; Hoyland, D; Kopparapu, R; Kringel, V; Krishnamurthy, S; Krishnan, B; Lastzka, N; Lodhia, D; Lück, H; Lundgren, A; MacInnis, M; Mak, C; Matichard, F; McClelland, D. E; McIntyre, G; Mercer, R. A; Meshkov, S; Miller, J; Moe, B; Morioka, T; Newton, G; Nolting, D; O'Dell, J; O'Reilly, B; Osthelder, C; Pan, Y; Papa, M. A; Pedraza, M; Pekowsky, L; Pitkin, M; Price, L. R; Radkins, H; Robertson, N. A; Robinson, E. L; Ryan, K; Sakosky, M; Saulson, P. R; Savage, R; Scott, J; Sintes, A. M; Slutsky, J; Susmithan, S; Sutton, P. J; Tanner, D. B; Thrane, E; Torrie, C. I; Vahlbruch, H; Vaishnav, B; Vallisneri, M; van der Sluys, M. V; Vecchio, A; Villar, A; Wallace, L; Wen, L; Wessels, P; West, M; Whelan, J. T; Willems, P. A; Winkelmann, L; Yoshida, S; Zhao, C
Astrophysical journal/The Astrophysical journal, 10/2010, Volume: 722, Issue: 2Journal Article
We present a search for periodic gravitational waves from the neutron star in the supernova remnant Cassiopeia A. The search coherently analyzes data in a 12 day interval taken from the fifth science run of the Laser Interferometer Gravitational-Wave Observatory. It searches gravitational-wave frequencies from 100 to 300 Hz and covers a wide range of first and second frequency derivatives appropriate for the age of the remnant and for different spin-down mechanisms. No gravitational-wave signal was detected. Within the range of search frequencies, we set 95% confidence upper limits of (0.7-1.2) X 10--24 on the intrinsic gravitational-wave strain, (0.4-4) X 10--4 on the equatorial ellipticity of the neutron star, and 0.005-0.14 on the amplitude of r-mode oscillations of the neutron star. These direct upper limits beat indirect limits derived from energy conservation and enter the range of theoretical predictions involving crystalline exotic matter or runaway r-modes. This paper is also the first gravitational-wave search to present upper limits on the r-mode amplitude.
Author
Shelf entry
Permalink
- URL:
Impact factor
Access to the JCR database is permitted only to users from Slovenia. Your current IP address is not on the list of IP addresses with access permission, and authentication with the relevant AAI accout is required.
Year | Impact factor | Edition | Category | Classification | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Select the library membership card:
If the library membership card is not in the list,
add a new one.
DRS, in which the journal is indexed
Database name | Field | Year |
---|
Links to authors' personal bibliographies | Links to information on researchers in the SICRIS system |
---|
Source: Personal bibliographies
and: SICRIS
The material is available in full text. If you wish to order the material anyway, click the Continue button.