| Full text | |
| Author(s): |
Tinto, Massimo
Total Authors: 1
|
| Document type: | Journal article |
| Source: | ACTA PHYSICA POLONICA B PROCEEDINGS SUPPLEMENT; v. 13, n. 2, p. 10-pg., 2020-01-01. |
| 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. (AU) | |
| FAPESP's process: | 19/07131-0 - Space-based gravitational wave astronomy |
| Grantee: | Oswaldo Duarte Miranda |
| Support Opportunities: | Research Grants - Visiting Researcher Grant - International |