Challenges and Synergies with Future Gravitational Wave Observatories
A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Astroinformatics and Astrostatistics".
Deadline for manuscript submissions: 30 November 2024 | Viewed by 73
Special Issue Editors
Interests: LISA; gravitational waves; experimental gravity; small force experiments; gravitational waves data analysis
2. INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, 20126 Milan, Italy
3. Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT, UK
Interests: relativistic astrophysics; gravitational-wave astronomy
Special Issue Information
Dear Colleagues,
The recent adoption of LISA by the European Space Agency, together with advancements in third-generation detectors such as the Einstein Telescope in Europe and Cosmic Explorer in the US, and possibly rapid progress regarding a similar Chinese space mission, present an intriguing opportunity to discuss possible synergies in terms of both data analysis and scientific exploitation. With this Special Issue, we would like to cover the scientific and data analysis challenges and opportunities that high-SNR, high-dimensionality data sets from planned or potential future gravitational observatories will create. These problems and opportunities will include the global fit challenge, stochastic background detection, and multi-frequency GW source characterization—to mention but a few.
Dr. Vetrugno Daniele
Dr. Riccardo Buscicchio
Guest Editors
Manuscript Submission Information
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Keywords
- gravitational waves
- LISA
- ET
- einstein telescope
- cosmic explorer
- global fit
- stochastic gravitational waves background
- multifrequency GW observation
- GW observatories synergies
- GW data analysis
