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学術論文

The Performance of Random Template Banks

MPS-Authors
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Allen,  Bruce
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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フルテキスト (公開)

2203.02759.pdf
(プレプリント), 616KB

PhysRevD.105.102003.pdf
(出版社版), 425KB

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引用

Allen, B. (2022). The Performance of Random Template Banks. Physical Review D, 105(10):. doi:10.1103/PhysRevD.105.102003.


引用: https://hdl.handle.net/21.11116/0000-000A-1944-E
要旨
When searching for new gravitational-wave or electromagnetic sources, the $n$
signal parameters (masses, sky location, frequencies,...) are unknown. In
practice, one hunts for signals at a discrete set of points in parameter space,
called a template bank. These may be constructed systematically as a lattice,
or alternatively, by placing templates at randomly selected points in parameter
space. Here, we calculate the fraction of signals lost by an $n$-dimensional
random template bank (compared to a very finely spaced bank). This fraction is
compared to the corresponding loss fraction for the best possible lattice-based
template banks containing the same number of grid points. For dimensions $n<4$
the lattice-based template banks significantly outperform the random ones.
However, remarkably, for dimensions $n>8$, the difference is negligible. In
high dimensions, random template banks outperform the best known lattices.