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The first scientific runs of kilometer scale laser interferometric detectors like LIGO are underway. Data from these detectors will be used to look for signatures of gravitational waves (GW) from astrophysical objects like inspiraling…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Anand S. Sengupta , Sanjeev Dhurandhar , Albert Lazzarini

It is well known that matched filtering techniques cannot be applied for searching extensive parameter space volumes for continuous gravitational wave signals. This is the reason why alternative strategies are being pursued. Hierarchical…

广义相对论与量子宇宙学 · 物理学 2007-05-23 M. A. Papa , B. F. Schutz , A. M. Sintes

It has long been known that the search for gravitational waves from inspiraling binaries must be aided by signal processing methods, and that the technique of matched filtering is the most likely to be used for the detection of inspiral…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Benjamin J. Owen

Nearly all template-based gravitational wave (GW) searches only include the quasi-circular quadrupolar modes of the signals in their templates. Including additional degrees of freedom in the GW templates corresponding to higher-order…

广义相对论与量子宇宙学 · 物理学 2024-09-10 Digvijay Wadekar , Tejaswi Venumadhav , Javier Roulet , Ajit Kumar Mehta , Barak Zackay , Jonathan Mushkin , Matias Zaldarriaga

Future space-based laser interferometric detectors, such as LISA, will be able to detect gravitational waves (GWs) generated during the inspiral phase of stellar-mass binary black holes (SmBBHs). The detection and characterization of GWs…

天体物理仪器与方法 · 物理学 2025-02-04 Yao Fu , Yan Wang , Soumya D. Mohanty

Astrophysical compact binary systems consisting of neutron stars and blackholes are an important class of gravitational wave (GW) sources for advanced LIGO detectors. Accurate theoretical waveform models from the inspiral, merger and…

广义相对论与量子宇宙学 · 物理学 2017-11-15 Soumen Roy , Anand S. Sengupta , Nilay Thakor

The detection of gravitational waves from coalescing compact binaries would be a computationally intensive process if a single bank of template wave forms (i.e., a one step search) is used. In an earlier paper we had presented a detection…

广义相对论与量子宇宙学 · 物理学 2009-12-30 Soumya D. Mohanty

We present a novel gravitational wave detection algorithm that conducts a matched filter search stochastically across the compact binary parameter space rather than relying on a fixed bank of template waveforms. This technique is…

We discuss a method to analyze data from interferometric gravitational wave detectors focusing on the technique of hierarchical search to detect gravitational waves from inspiraling binaries. For this purpose, we propose new coordinates to…

广义相对论与量子宇宙学 · 物理学 2009-12-30 Takahiro Tanaka , Hideyuki Tagoshi

Matched filtering is a common method for detecting gravitational waves. However, the computational costs of searching large template banks limit the efficiency of classical algorithms when searching for massive black hole binary (MBHB)…

天体物理仪器与方法 · 物理学 2025-10-20 Fangzhou Guo , Jibo He

Searching for gravitational waves from compact binary coalescence (CBC) is performed by matched filtering the observed strain data from gravitational-wave observatories against a discrete set of waveform templates designed to accurately…

天体物理仪器与方法 · 物理学 2022-05-12 Rahul Dhurkunde , Henning Fehrmann , Alexander H. Nitz

The detection of gravitational waves (GWs) from coalescing compact binaries has become routine with ground-based detectors like LIGO and Virgo. However, beyond standard sources such as binary black holes and neutron stars and neutron star…

广义相对论与量子宇宙学 · 物理学 2024-12-30 Kanchan Soni , Alexander H. Nitz

Matched filtering is used to search for gravitational waves emitted by inspiralling compact binaries in data from the ground-based interferometers. One of the key aspects of the detection process is the design of a template bank that covers…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Thomas Cokelaer

Electromagnetic (EM) follow-up observations of gravitational wave (GW) events will help shed light on the nature of the sources, and more can be learned if the EM follow-ups can start as soon as the GW event becomes observable. In this…

广义相对论与量子宇宙学 · 物理学 2015-05-30 Jing Luan , Shaun Hooper , Linqing Wen , Yanbei Chen

Recent discoveries of gravitational wave (GW) signals from astrophysical compact binary systems of neutron stars and black holes have firmly established them as prime sources for advanced GW detectors. Theoretical templates of expected…

广义相对论与量子宇宙学 · 物理学 2019-02-04 Soumen Roy , Anand S. Sengupta , Parameswaran Ajith

When looking for gravitational wave signals from known pulsars, targets have been treated using independent searches. Here we use a hierarchical Bayesian framework to combine observations from individual sources for two purposes: to produce…

天体物理仪器与方法 · 物理学 2018-09-12 M. Pitkin , C. Messenger , X. Fan

Searches for gravitational wave events use models, or templates, for the signals of interest. The templates used in current searches in the LIGO-Virgo-Kagra (LVK) data model the dominant quadrupole mode $(\ell,|m|)=(2,2)$ of the signals,…

广义相对论与量子宇宙学 · 物理学 2024-10-18 Digvijay Wadekar , Tejaswi Venumadhav , Ajit Kumar Mehta , Javier Roulet , Seth Olsen , Jonathan Mushkin , Barak Zackay , Matias Zaldarriaga

Gravitational wave searches rely on a combination of methods, including matched filtering, coherent analyses, and more recent machine learning based pipelines. For compact binary coalescences, where signals originate from the relativistic…

广义相对论与量子宇宙学 · 物理学 2026-03-11 Lorenzo Mobilia , Tito Dal Canton , Gianluca Maria Guidi

Searching for a signal depending on unknown parameters in a noisy background with matched filtering techniques always requires an analysis of the data with several templates in parallel in order to ensure a proper match between the filter…

The prior knowledge of the gravitational waveform from compact binary systems makes matched filtering an attractive detection strategy. This detection method involves the filtering of the detector output with a set of theoretical waveforms…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Edward K. Porter
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