| Athens/Institutional login |
|
| 
| 
|
|
|
|
|||
| Journals Home | Journals List | EJs Extra | This Journal | Search | Authors | Referees | Librarians | User Options | Help | | ||||
|
||||
|
|
| | |
|
||||
2009 Class. Quantum Grav. 26 225012 (9pp) doi: 10.1088/0264-9381/26/22/225012
 |
 |
 |
||
|
||||
 |
|
 |
Abstract. This paper reports the investigation of a potential source of noise in the Laser Interferometer Space Antenna (LISA). The effect, not yet discussed in the literature, is a phase noise due to the presence of interplanetary dust along the path of LISA laser beams. The investigated source of noise has been found to be negligible in all the analyzed scenarios. We have estimated that the phase noise induced by the interplanetary dust complex is about 11 orders of magnitude below the best LISA sensitivity. A modest increase in the noise level has been found when dust fluctuations due to dust streams or nearby-passing comets are taken into account.
PACS numbers: 04.80.Nn, 42.25.Bs, 96.30.Vb
Print publication: Issue 22 (21 November 2009) |
Post to CiteUlike | | Post to Connotea | | Post to Bibsonomy |
|
|
|
|
| | |
|
|
|
|
|
|
Journals Home | Journals List | EJs Extra | This Journal | Search | Authors | Referees | Librarians | User Options | Help | Recommend this journal EndNote, ProCite ® and Reference Manager ® are registered trademarks of ISI Researchsoft. Copyright © Institute of Physics and IOP Publishing Limited 2009. Use of this service is subject to compliance with the Terms and Conditions of use. In particular, reselling and systematic downloading of files is prohibited. Help: Cookies | Data Protection. Privacy policy Disclaimer |
|
| |
