@Article{Tinto:2020:SpGrWa,
               author = "Tinto, Massimo",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Space-based gravitational wave observations in the mid-band 
                         frequency region",
              journal = "Acta Physica Polonica B, Proceedings Supplement",
                 year = "2020",
               volume = "13",
               number = "2",
                pages = "167--176",
             abstract = "The intermediate Gravitation Wave (GW) frequency detection band, 
                         i.e. the frequency region that is in between those accessible by 
                         space-based interferometers with million-kilometer armlengths and 
                         ground-based detectors, could be unveiled relatively soon. A 
                         space-based GW interferometer of arm-length equal to about 100,000 
                         km would achieve an optimal sensitivity within an observational 
                         frequency band that is blue-shifted with respect to those of the 
                         LISA and TaiJi missions by about a factor 30. By opening the 
                         mid-band GW frequency region, such a mission would complement the 
                         scientific capabilities of both ground- and million-kilometer 
                         arm-length detectors and provide an enhanced scientific return 
                         over those obtainable by each detector operated as stand-alone.",
                  doi = "10.5506/APHYSPOLBSUPP.13.167",
                  url = "http://dx.doi.org/10.5506/APHYSPOLBSUPP.13.167",
                 issn = "0587-4254",
             language = "en",
           targetfile = "tinto_space.pdf",
        urlaccessdate = "28 abr. 2024"
}