Black Holes, Lasers and Data Analysis: Contributions to Gravitational Wave Searches with the ExcessPower Pipeline

Autores/as

  • Sydney J. Chamberlin Department of Physics University of Wisconsin-Milwaukee Milwaukee, WI

DOI:

https://doi.org/10.17307/wsc.v1i1.102

Palabras clave:

LIGO, laser interferometry, gravitational waves

Resumen

Gravitational waves (GWs) are tiny perturbations to the spacetime structure of the universe that propagate freely as wavelike solutions to the Einstein equations. The direct detection of GWs is currently a major goal in experimental physics, and a number of large scale efforts to detect them are currently underway.

Citas

A. Abramovici, W. E. Althouse, R. W. Drever, Y. Gursel, S. Kawamura, et al., Science 256, 325 (1992).

http://dx.doi.org/10.1126/science.256.5055.325

W. G. Anderson, P. R. Brady, J. D. Creighton, and E. E. Flanagan, Phys. Rev. D 63, 042003 (2001), arXiv:gr-qc/0008066.

http://dx.doi.org/10.1103/PhysRevD.63.042003

P. Brady, D. Brown, K. Cannon, and S. Ray-Majumder, Excess Power, https://dcc.ligo.org/LIGO-T1200125 (2007), lIGO Document T1200125.

J. D. E. Creighton and W. G. Anderson, Gravitational-wave Physics and Astronomy (Wiley-VCH, 2011).

http://dx.doi.org/10.1002/9783527636037

C. Pankow, ExcessPower: A Status Report, https://dcc.ligo.org/cgi-bin/private/DocDB/ShowDocument?docid=97802 (2012), lIGO Document G1201140-v1.

Descargas

Publicado

2015-01-01

Cómo citar

Chamberlin, S. J. (2015). Black Holes, Lasers and Data Analysis: Contributions to Gravitational Wave Searches with the ExcessPower Pipeline. Proceedings of the Wisconsin Space Conference, 1(1). https://doi.org/10.17307/wsc.v1i1.102

Número

2014: Commercial Space

Sección

Astronomy and Cosmology

Licencia

Creative Commons License
This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.