Milli-Hertz Gravitational Waves: LISA and LISA PathFinder
Milli-Hertz Gravitational Waves: LISA and LISA PathFinder
About this item
Full title
Author / Creator
Araújo, H , Cañizares, P , Chmeissani, M , Conchillo, A , Díaz-Aguiló, M , García-Berro, E , Gesa, L , Gibert, F , Grimani, C , Hajdas, W , Hollington, D , Lloro, I , Lobo, A , Mateos, I , Nofrarias, M , Puigdengoles, C , Ramos-Castro, J , Sanjuán, J , Sopuerta, CF and Wass, P
Publisher
Bristol: IOP Publishing
Journal title
Language
English
Formats
Publication information
Publisher
Bristol: IOP Publishing
Subjects
More information
Scope and Contents
Contents
Ground based GW detectors are limited at their lower frequency band (1-10 Hz) by settlement gravity gradients and seismic noise, and their sensitivity peaks at around 100 Hz. Sources in this band are mostly short duration signals, and their rates uncertain. Going down to milli-Hertz frequencies significantly increases the number and types of availa...
Alternative Titles
Full title
Milli-Hertz Gravitational Waves: LISA and LISA PathFinder
Authors, Artists and Contributors
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_miscellaneous_1730055219
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1730055219
Other Identifiers
ISSN
1742-6596,1742-6588
E-ISSN
1742-6596
DOI
10.1088/1742-6596/314/1/012014