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The continuous wavelet derived by smoothing function and its application in cosmology
- Publication Year :
- 2021
- Publisher :
- arXiv, 2021.
-
Abstract
- The wavelet analysis technique is a powerful tool and is widely used in broad disciplines of engineering, technology, and sciences. In this work, we present a novel scheme of constructing continuous wavelet functions, in which the wavelet functions are obtained by taking the first derivative of smoothing functions with respect to the scale parameter. Due to this wavelet constructing scheme, the inverse transforms are only one-dimensional integrations with respect to the scale parameter, and hence the continuous wavelet transforms constructed in this way are more ready to use than the usual scheme. We then apply the Gaussian-derived wavelet constructed by our scheme to computations of the density power spectrum for dark matter, the velocity power spectrum and the kinetic energy spectrum for baryonic fluid. These computations exhibit the convenience and strength of the continuous wavelet transforms. The transforms are very easy to perform, and we believe that the simplicity of our wavelet scheme will make continuous wavelet transforms very useful in practice.<br />Comment: 9 Pages, 4 Figures, comments welcome
- Subjects :
- Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Physics and Astronomy (miscellaneous)
Computer science
Computation
ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION
Spectral density
FOS: Physical sciences
Function (mathematics)
Data_CODINGANDINFORMATIONTHEORY
Computational Physics (physics.comp-ph)
Wavelet
Continuous wavelet
Astrophysics - Instrumentation and Methods for Astrophysics
Algorithm
Scale parameter
Physics - Computational Physics
Instrumentation and Methods for Astrophysics (astro-ph.IM)
Smoothing
Continuous wavelet transform
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
Details
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....e1631cf8bbdbacd3398c017214949dc1
- Full Text :
- https://doi.org/10.48550/arxiv.2104.09505