Handbook of nanoHz gravitational wave astronomy

Author:   Bhal Chandra Joshi (Tata Institute of Fundamental Research (India))
Publisher:   Institute of Physics Publishing
ISBN:  

9780750363686


Publication Date:   30 November 2025
Format:   Hardback
Availability:   In Print   Availability explained
This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us.

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Handbook of nanoHz gravitational wave astronomy


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Author:   Bhal Chandra Joshi (Tata Institute of Fundamental Research (India))
Publisher:   Institute of Physics Publishing
Imprint:   Institute of Physics Publishing
ISBN:  

9780750363686


ISBN 10:   0750363681
Publication Date:   30 November 2025
Audience:   Professional and scholarly ,  Professional & Vocational
Format:   Hardback
Publisher's Status:   Active
Availability:   In Print   Availability explained
This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us.

Table of Contents

A. Review of concepts related to PTA material 1 Introduction – Overview of the book 2 Gravitational Waves – Historical prelude, GW theory, GW sources 3 Radio Pulsars – Brief overview of radio pulsars and phenomenology 4 Frequentist and Bayesian Analysis of data B. Analysis Technique for PTA experiments 5 Pulsar Timing technique – Concepts and tools (TEMPO2, PINT, TEMPONEST, ENTERPRISE) 6 Noise modeling – Bayesian modeling of single pulsar achromatic and chromatic noise sources 7 Optimal Statistic for Gravitational Wave background search 8 Bayesian models for Gravitational Wave background search C. Pulsar Timing Array experiments 9 Pulsar Timing Array – Historical prelude, theory and practice of pulsat timing array experiments 10 Current pulsar timing array experiments and International Pulsar Timing Array 11 Search for Gravitational Wave background – recent results 12 Continuous source search – recent results 13 Future and conclusions

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NOV RG 20252

 

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