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SPACE-BASED GRAVITATIONAL WAVE OBSERVATIONS IN THE MID-BAND FREQUENCY REGION

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Autor(es):
Tinto, Massimo
Número total de Autores: 1
Tipo de documento: Artigo Científico
Fonte: ACTA PHYSICA POLONICA B PROCEEDINGS SUPPLEMENT; v. 13, n. 2, p. 10-pg., 2020-01-01.
Resumo

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. (AU)

Processo FAPESP: 19/07131-0 - Astronomia de ondas gravitacionais com detetores espaciais
Beneficiário:Oswaldo Duarte Miranda
Modalidade de apoio: Auxílio à Pesquisa - Pesquisador Visitante - Internacional