Hostname: page-component-78c5997874-fbnjt Total loading time: 0 Render date: 2024-11-01T02:40:44.408Z Has data issue: false hasContentIssue false

Gravitational wave radiation from white dwarf close encountersin globular clusters

Published online by Cambridge University Press:  30 September 2008

A.G. Pedemonte
Affiliation:
Departament de Física Aplicada, Universitat Politècnica de Catalunya, Escola Politécnica Superior de Castelldefels, Av. del Canal Olímpic, s/n, 08860 Castelldefels, Spain Institut d'Estudis Espacials de Catalunya, c/Gran Capità 2–4, 08034 Barcelona, Spain
P. Lorén-Aguilar
Affiliation:
Departament de Física Aplicada, Universitat Politècnica de Catalunya, Escola Politécnica Superior de Castelldefels, Av. del Canal Olímpic, s/n, 08860 Castelldefels, Spain Institut d'Estudis Espacials de Catalunya, c/Gran Capità 2–4, 08034 Barcelona, Spain
J. Isern
Affiliation:
Institut d'Estudis Espacials de Catalunya, c/Gran Capità 2–4, 08034 Barcelona, Spain
J.A. Lobo
Affiliation:
Institut d'Estudis Espacials de Catalunya, c/Gran Capità 2–4, 08034 Barcelona, Spain
E. García-Berro
Affiliation:
Departament de Física Aplicada, Universitat Politècnica de Catalunya, Escola Politécnica Superior de Castelldefels, Av. del Canal Olímpic, s/n, 08860 Castelldefels, Spain Institut d'Estudis Espacials de Catalunya, c/Gran Capità 2–4, 08034 Barcelona, Spain
Get access

Abstract

In the dense central regions of globular clusters close encounters oftwo white dwarfs are relatively frequent (one or more strongencounters per star in the lifetime of the cluster). Such encountersshould be potential sources of gravitational wave emission. Thus, itis foreseeable that these collisions could be either detected by LISAor they could contribute significantly to the background noise of thedetectors. We compute the gravitational wave pattern resulting fromthese encounters for a broad range of system parameters, which includethe masses and the relative distances of the white dwarfs involved inthe encounter.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2008

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Abramovici, A., et al., 1992, Science, 256, 325 CrossRef
Acernese, F., et al., 2004, Class. Quant. Grav., 21, S385 CrossRef
Bender, P.L., et al., 1998, “LISA: Laser Interferometer Space Antenna for the detection and observation of GW”, Pre-fase A Report (Garching: Max-Planck-Institut für Quantenoptik)
Bender, P.L., et al., 2000, “LISA: a conerstone mission for the observation of gravitational waves”, ESA-SCI(2000)11, System and Technology Study Report
Benz, W., 1990, in “The numerical modelling of Nonlinear stellar pulsations”, ed. J. Buchler (Dordrecht: Kluwer Academic Publishers), p. 269
Danzmann, K., & Rüdiger, A., 2003, Class. Quant. Grav., 20, S1 CrossRef
Gingold, R.A., & Monaghan, J.J., 1977, MNRAS, 181, 375 CrossRef
Guerrero, J., García–Berro, E., & Isern, J., 2004, A&A, 413, 257
Lorén-Aguilar, P., Guerrero, J., Isern, J., Lobo, J.A., & García–Berro, E., 2005, MNRAS, 356, 627 CrossRef
Hughes, S.A., 2006, in Laser Interferometer Space Antenna, ed. S.M. Merkowitz, & J.C. Livas (AIP Conf. Proc., 823 Melville: New York), 13
Lucy, L.B., 1977, AJ, 82, 1013 CrossRef
Misner, C.W., Thorne, K.S., & Wheeler, J.A., 1973, “Gravitation” (New York: W.H. Freeman)
Shara, M.M., & Hurley, J.R., 2002, ApJ, 571, 830 CrossRef
Takahashi, R., et al., 2004, Class. Quant. Grav., 21, S403 CrossRef
Willems, , et al., 2007, ApJ, 665, L59-L62 CrossRef
Willke, B., et al., 2004, Class. Quant. Grav., 21, S417 CrossRef