Autor: |
Sauter, Orion, Dergachev, Vladimir, Riles, Keith |
Rok vydání: |
2017 |
Předmět: |
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Zdroj: |
Phys. Rev. D 99, 044006 (2019) |
Druh dokumentu: |
Working Paper |
DOI: |
10.1103/PhysRevD.99.044006 |
Popis: |
Accurate determination of gravitational wave source parameters relies on transforming between the source and detector frames. All-sky searches for continuous wave sources are computationally expensive, in part, because of barycentering transformation of time delays to a solar system frame. This expense is exacerbated by the complicated modulation induced in signal templates. We investigate approximations for determining time delays of signals received by a gravitational wave detector with respect to the solar system barycenter. A highly non-linear conventional computation is transformed into one that has a pure linear sum in its innermost loop. We discuss application of these results to determination of the maximal useful integration time of continuous wave searches. |
Databáze: |
arXiv |
Externí odkaz: |
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