Symmetry Breaking Based Detectors R.P. Croce', V. Matta", V. Pierro', I.M. Pinto' ' WavesGroup, University of Sannio at Benevento " DI^3E, University of Salerno Symmetry breaking based detectors are a wide and relatively unexplored class, which includes, among others, stochastic-resonance based detectors [1-3], and many more. In this communication we discuss a possible basic paradigm, where the observable is the distribution of (real) zeros of random polynomials whose coefficients are the time samples of a signal+noise mixture, and the signal, whose possible presence has to be detected, has a known adiabatically evolving angular frequency. Possible application to gravitational wave detection from pulsars and coalescing binaries is suggested and preliminarily discussed. [1] J.W.C. Robinson et al., Phys. Rev. Lett. 81 (1998) 2850 [2] V. Galdi, V. Pierro, I.M. Pinto, Phys. Rev. E57 (1998) 6470. [3] F. Chapeau-Blondeau, Phys. Rev. E66 (2002) 032101.

Symmetry Breaking Based Derectors

Pierro V;Pinto I. M.
2003-01-01

Abstract

Symmetry Breaking Based Detectors R.P. Croce', V. Matta", V. Pierro', I.M. Pinto' ' WavesGroup, University of Sannio at Benevento " DI^3E, University of Salerno Symmetry breaking based detectors are a wide and relatively unexplored class, which includes, among others, stochastic-resonance based detectors [1-3], and many more. In this communication we discuss a possible basic paradigm, where the observable is the distribution of (real) zeros of random polynomials whose coefficients are the time samples of a signal+noise mixture, and the signal, whose possible presence has to be detected, has a known adiabatically evolving angular frequency. Possible application to gravitational wave detection from pulsars and coalescing binaries is suggested and preliminarily discussed. [1] J.W.C. Robinson et al., Phys. Rev. Lett. 81 (1998) 2850 [2] V. Galdi, V. Pierro, I.M. Pinto, Phys. Rev. E57 (1998) 6470. [3] F. Chapeau-Blondeau, Phys. Rev. E66 (2002) 032101.
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.12070/15061
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
social impact