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Gravitational Waves from a Core-Collapse Supernova: Perspectives with Detectors in the Late 2020s and Early 2030s
| Content Provider | MDPI |
|---|---|
| Author | Marek, Szczepańczyk Zanolin, Michele |
| Copyright Year | 2022 |
| Description | We studied the detectability and reconstruction of gravitational waves from core-collapse supernova multidimensional models using simulated data from detectors predicted to operate in the late 2020s and early 2030s. We found that the detection range will improve by a factor of around two with respect to the second-generation gravitational-wave detectors, and the sky localization will significantly improve. We analyzed the reconstruction accuracy for the lower frequency and higher frequency portion of supernova signals with a 250 Hz cutoff. Since the waveform’s peak frequencies are usually at high frequencies, the gravitational-wave signals in this frequency band were reconstructed more accurately. |
| Starting Page | 70 |
| e-ISSN | 20754434 |
| DOI | 10.3390/galaxies10030070 |
| Journal | Galaxies |
| Issue Number | 3 |
| Volume Number | 10 |
| Language | English |
| Publisher | MDPI |
| Publisher Date | 2022-05-23 |
| Access Restriction | Open |
| Subject Keyword | Galaxies Gravitational Waves Core-collapse Supernova Future Detectors |
| Content Type | Text |
| Resource Type | Article |
