Time-frequency analysis of simulated binary pulsar signals

The science that deals with the study of celestial objects, the physics, chemistry and evolution of such objects is called Astronomy and the branch of Astronomy that deals with the behavior and dynamic processes of the celestial objects is called Astrophysics. This dissertation discusses one such di...

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Main Author: Nandhini Ganesan
Other Authors: Saman S Abeysekera
Format: Theses and Dissertations
Language:English
Published: 2013
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Online Access:http://hdl.handle.net/10356/55201
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Institution: Nanyang Technological University
Language: English
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spelling sg-ntu-dr.10356-552012023-07-04T16:04:33Z Time-frequency analysis of simulated binary pulsar signals Nandhini Ganesan Saman S Abeysekera School of Electrical and Electronic Engineering DRNTU::Engineering::Electrical and electronic engineering The science that deals with the study of celestial objects, the physics, chemistry and evolution of such objects is called Astronomy and the branch of Astronomy that deals with the behavior and dynamic processes of the celestial objects is called Astrophysics. This dissertation discusses one such discoveries of the modem astronomy, Pulsars. Pulsar, from the time it was discovered in 1967 has been a curious and exciting topic for the entire astrophysicist. They are perhaps the most extraordinary Physics laboratory in the Universe. With its discovery by Jocelyn Bell Burnell and Antony Hewish, who received Nobel Prize in 1974, it got the attention of many astrophysicists. Pulsars are used to detect gravitational waves and they earned another Nobel Prize in 1993 for a prediction related to the same. In order to search pulsars, many methods have been employed. One common method used to detect the Binary pulsar is called sideband search. Sideband search employs Two-stage Fourier Analysis for the detection. This dissertation aims to use Autocorrelation method instead of Two-stage Fourier analysis for the detection of Orbital period of the pulsar. The performance of both the methods is compared using different Signal to Noise Ratio (SNR) values and is shown to be similar. Time frequency analysis is done on the pulsar signal to estimate the Instantaneous Frequency. From Instantaneous Frequency (IF), the pulsar velocity and acceleration are estimated. It is used to characterize the pulsar and extract two relevant orbital parameters in circular orbit. Thus the study of pulsars enables us to understand the origin of our Universe, test the theory of Einstein's relativity. Because of pulsars our timing standard has improved and our understanding for cosmological objects like neutron star, black hole has increased. Master of Science (Signal Processing) 2013-12-30T03:25:46Z 2013-12-30T03:25:46Z 2013 2013 Thesis http://hdl.handle.net/10356/55201 en 57 p. application/pdf
institution Nanyang Technological University
building NTU Library
continent Asia
country Singapore
Singapore
content_provider NTU Library
collection DR-NTU
language English
topic DRNTU::Engineering::Electrical and electronic engineering
spellingShingle DRNTU::Engineering::Electrical and electronic engineering
Nandhini Ganesan
Time-frequency analysis of simulated binary pulsar signals
description The science that deals with the study of celestial objects, the physics, chemistry and evolution of such objects is called Astronomy and the branch of Astronomy that deals with the behavior and dynamic processes of the celestial objects is called Astrophysics. This dissertation discusses one such discoveries of the modem astronomy, Pulsars. Pulsar, from the time it was discovered in 1967 has been a curious and exciting topic for the entire astrophysicist. They are perhaps the most extraordinary Physics laboratory in the Universe. With its discovery by Jocelyn Bell Burnell and Antony Hewish, who received Nobel Prize in 1974, it got the attention of many astrophysicists. Pulsars are used to detect gravitational waves and they earned another Nobel Prize in 1993 for a prediction related to the same. In order to search pulsars, many methods have been employed. One common method used to detect the Binary pulsar is called sideband search. Sideband search employs Two-stage Fourier Analysis for the detection. This dissertation aims to use Autocorrelation method instead of Two-stage Fourier analysis for the detection of Orbital period of the pulsar. The performance of both the methods is compared using different Signal to Noise Ratio (SNR) values and is shown to be similar. Time frequency analysis is done on the pulsar signal to estimate the Instantaneous Frequency. From Instantaneous Frequency (IF), the pulsar velocity and acceleration are estimated. It is used to characterize the pulsar and extract two relevant orbital parameters in circular orbit. Thus the study of pulsars enables us to understand the origin of our Universe, test the theory of Einstein's relativity. Because of pulsars our timing standard has improved and our understanding for cosmological objects like neutron star, black hole has increased.
author2 Saman S Abeysekera
author_facet Saman S Abeysekera
Nandhini Ganesan
format Theses and Dissertations
author Nandhini Ganesan
author_sort Nandhini Ganesan
title Time-frequency analysis of simulated binary pulsar signals
title_short Time-frequency analysis of simulated binary pulsar signals
title_full Time-frequency analysis of simulated binary pulsar signals
title_fullStr Time-frequency analysis of simulated binary pulsar signals
title_full_unstemmed Time-frequency analysis of simulated binary pulsar signals
title_sort time-frequency analysis of simulated binary pulsar signals
publishDate 2013
url http://hdl.handle.net/10356/55201
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