@Article{TintoAraúAguiAlve:2013:SeGrWa,
               author = "Tinto, Massimo and Ara{\'u}jo, Jose Carlos Neves de and Aguiar, 
                         Odylio Denys de and Alves, M. E. S.",
          affiliation = "Divis{\~a}o de Astrof{\'{\i}}sica, Instituto Nacional de 
                         Pesquisas Espaciais, S. J. Campos, SP 12227-010, Brazil; Jet 
                         Propulsion Laboratory, California Institute of Technology, 
                         Pasadena, CA 91109, United States and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)} and Instituto de F{\'{\i}}sica e 
                         Qu{\'{\i}}mica, Universidade Federal de Itajub{\'a}, 
                         Itajub{\'a}, MG 37500-903, Brazil",
                title = "Searching for gravitational waves with a geostationary 
                         interferometer",
              journal = "Astroparticle Physics",
                 year = "2013",
               volume = "48",
                pages = "50--60",
             keywords = "Black holes, Black holes physics, Gravitational wave detectors, 
                         Gravitational wave interferometers, Laser interferometer space 
                         antenna, Frequency bands, Gravitational effects, Interferometers, 
                         Laser interferometry, Stars, Gravity waves.",
             abstract = "We analyze the sensitivities of a geostationary gravitational wave 
                         interferometer mission operating in the sub-Hertz band. Because of 
                         its smaller armlength, in the lower part of its accessible 
                         frequency band (10 -4-2×10-2 Hz) our proposed Earth-orbiting 
                         detector will be less sensitive, by a factor of about seventy, 
                         than the Laser Interferometer Space Antenna (LISA) mission. In the 
                         higher part of its band instead (2×10-2-10 Hz), our proposed 
                         interferometer will have the capability of observing super-massive 
                         black holes (SMBHs) with masses smaller than <106 M{\^a}`{"}. 
                         With good event rates for these systems, a geostationary 
                         interferometer will be able to accurately probe the astrophysical 
                         scenarios that account for their formation. © 2013 Elsevier B.V. 
                         All rights reserved.",
                  doi = "10.1016/j.astropartphys.2013.07.001",
                  url = "http://dx.doi.org/10.1016/j.astropartphys.2013.07.001",
                 issn = "0927-6505",
                label = "scopus 2013-11",
             language = "en",
        urlaccessdate = "04 maio 2024"
}