The Analysis of Large Order Bessel Functions in Gravitational Wave Signals from Pulsars
Chishtie, F. A. ; Valluri, S. R. ; Rao, K. M. ; Sikorski, D. ; Williams, T.
arXiv, 0503037 / Harvested from arXiv
Text on arXiv
In this work, we present the analytic treatment of the large order Bessel functions that arise in the Fourier Transform (FT) of the Gravitational Wave (GW) signal from a pulsar. We outline several strategies which employ asymptotic expansions in evaluation of such Bessel functions which also happen to have large argument. Large order Bessel functions also arise in the Peters-Mathews model of binary inspiralling stars emitting GW and several problems in potential scattering theory. Other applications also arise in a variety of problems in Applied Mathematics as well as in the Natural Sciences and present a challenge for High Performance Computing(HPC).
Publié le : 2005-03-15
Classification:  Mathematical Physics,  Astrophysics,  Physics - Computational Physics 
@article{0503037,
     author = {Chishtie, F. A. and Valluri, S. R. and Rao, K. M. and Sikorski, D. and Williams, T.},
     title = {The Analysis of Large Order Bessel Functions in Gravitational Wave
  Signals from Pulsars},
     journal = {arXiv},
     volume = {2005},
     number = {0},
     year = {2005},
     language = {en},
     url = {http://dml.mathdoc.fr/item/0503037}
}

Chishtie, F. A.; Valluri, S. R.; Rao, K. M.; Sikorski, D.; Williams, T. The Analysis of Large Order Bessel Functions in Gravitational Wave
  Signals from Pulsars. arXiv, Tome 2005 (2005) no. 0, . http://gdmltest.u-ga.fr/item/0503037/