scholarly journals Semiparametric approach to the detection of non-Gaussian gravitational wave stochastic backgrounds

2014 ◽  
Vol 89 (12) ◽  
Author(s):  
Lionel Martellini ◽  
Tania Regimbau
Keyword(s):  
Gravitational Wave ◽  
Semiparametric Approach ◽  
Non Gaussian ◽  
Stochastic Backgrounds

scholarly journals Constraining Modified Theories of Gravity with Gravitational-Wave Stochastic Backgrounds

2016 ◽  
Vol 117 (9) ◽  
Author(s):  
Andrea Maselli ◽  
Stefania Marassi ◽  
Valeria Ferrari ◽  
Kostas Kokkotas ◽  
Raffaella Schneider
Keyword(s):  
Gravitational Wave ◽  
Modified Theories Of Gravity ◽  
Theories Of Gravity ◽  
Stochastic Backgrounds

scholarly journals Probing non-Gaussian stochastic gravitational wave backgrounds with LISA

2018 ◽  
Vol 2018 (11) ◽  
pp. 034-034 ◽  
Author(s):  
Nicola Bartolo ◽  
Valerie Domcke ◽  
Daniel G. Figueroa ◽  
Juan Garcia-Bellido ◽  
Marco Peloso ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Non Gaussian

NON-GAUSSIAN NOISE IN GRAVITATIONAL WAVE RESONANT DETECTORS: EXPLORER AND NAUTILUS REPORT

2000 ◽  
Vol 09 (03) ◽  
pp. 257-261 ◽  
Author(s):  
PAOLO BONIFAZI
Keyword(s):  
Gravitational Wave ◽  
Gaussian Noise ◽  
Stationary Noise ◽  
Wave Event ◽  
Non Gaussian

The problem of the non-Gaussian and non-stationary noise in the data of the International Gravitational Wave Event Collaboration (IGEC) is investigated for the two detectors Explorer and Nautilus. We report simple tests that show how part of the IGEC events belong to non-Gaussian and non-stationary noise.

scholarly journals Estimating the Chirp Mass of Eccentric Inspiraling Binary Systems from Time-Frequency Representations of their Gravitational Radiation

2021 ◽  
Vol 2081 (1) ◽  
pp. 012008
Author(s):  
Innocenzo M Pinto
Keyword(s):  
Binary System ◽  
Gravitational Wave ◽  
Gravitational Radiation ◽  
Binary Systems ◽  
Estimation Algorithm ◽  
Orbital Eccentricity ◽  
Reference Time ◽  
Time Frequency ◽  
Compact Binary ◽  
Non Gaussian

Abstract Using the simplest yet meaningful Peters-Mathews model describing the orbital damping of a compact binary system under the emission of gravitatonal radiation, we show that the chirp-mass of an eccentric inspiraling binary, and its (Keplerian) orbital eccentricity at some reference time, can be estimated from the time-frequency skeleton of its gravitational wave signal. The estimation algorithm is nicely simple, and is robust against the non-ideal (non Gaussian, non stationary) features of detector noise.

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