CaltechAUTHORS
  A Caltech Library Service

The science case for LIGO-India

Saleem, M. and Rana, Javed and Gayathri, V. and Vijaykumar, Aditya and Goyal, Srashti and Sachdev, Surabhi and Suresh, Jishnu and Sudhagar, S. and Mukherjee, Arunava and Gaur, Gurudatt and Sathyaprakash, Bangalore and Pai, Archana and Adhikari, Rana X. and Ajith, P. and Bose, Sukanta (2022) The science case for LIGO-India. Classical and Quantum Gravity, 39 (2). Art. No. 025004. ISSN 0264-9381. doi:10.1088/1361-6382/ac3b99. https://resolver.caltech.edu/CaltechAUTHORS:20220126-260834800

[img] PDF - Accepted Version
Creative Commons Public Domain Dedication.

1MB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20220126-260834800

Abstract

The global network of gravitational-wave detectors has completed three observing runs with ∼50 detections of merging compact binaries. A third LIGO detector, with comparable astrophysical reach, is to be built in India (LIGO-Aundha) and expected to be operational during the latter part of this decade. Such additions to the network increase the number of baselines and the network SNR of GW events. These enhancements help improve the sky-localization of those events. Multiple detectors simultaneously in operation will also increase the baseline duty factor, thereby, leading to an improvement in the detection rates and, hence, the completeness of surveys. In this paper, we quantify the improvements due to the expansion of the LIGO global network in the precision with which source properties will be measured. We also present examples of how this expansion will give a boost to tests of fundamental physics.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1088/1361-6382/ac3b99DOIArticle
https://arxiv.org/abs/2105.01716arXivDiscussion Paper
ORCID:
AuthorORCID
Saleem, M.0000-0002-3836-7751
Vijaykumar, Aditya0000-0002-4103-0666
Mukherjee, Arunava0000-0003-1274-5846
Sathyaprakash, Bangalore0000-0003-3845-7586
Adhikari, Rana X.0000-0002-5731-5076
Ajith, P.0000-0001-7519-2439
Bose, Sukanta0000-0002-4151-1347
Additional Information:© 2021 IOP Publishing Ltd. Received 9 June 2021; Revised 3 October 2021; Accepted 19 November 2021; Published 15 December 2021. We would like to thank our colleagues in the LIGO-India Scientific Collaboration and the LIGO-India Project for valuable inputs. We appreciate the several discussions we had with members of the various working groups in the LIGO-Virgo-KAGRA collaborations. In particular, we thank KG Arun, Bala Iyer, Shivaraj Kandhasamy, Jose Matthew, Fred Raab, Rory Smith, and Tarun Souradeep for valuable discussions and inputs. This work makes use of NumPy [153], SciPy [154], Matplotlib [155], AstroPy [156, 157], jupyter [158], dynesty [159], bilby [36] and PESummary [160] software packages. Thanks are also due to the Department of Science and Technology (DST) and the Department of Atomic Energy (DAE) of India. Specifically, MS acknowledges the support from the Infosys Foundation, the Swarnajayanti fellowship Grant DST/SJF/PSA-01/2017–18, and the support from the National Science Foundation with Grants PHY-1806630 and PHY-2010970, AP acknowledges support from the DST-SERB Matrics Grant MTR/2019/001096 and SERB-Power-fellowship Grant SPF/2021/000036, DST, India. AM acknowledges support from the DST-SERB Start-up Research Grant SRG/2020/001290, and PA, AV, and SG acknowledge support from DAE under Project No. RTI4001. PA's research was also supported by the Max Planck Society through a Max Planck Partner Group at ICTS-TIFR and by the Canadian Institute for Advanced Research through the CIFAR Azrieli Global Scholars program. SS is supported by an Eberly postdoctoral fellowship at Pennsylvania State University and BSS is supported by NSF Grants PHYS-1836779, PHYS-2012083 and AST-2006384. Thanks are due to computational support provided by the Alice (ICTS-TIFR) and Sarathi (IUCAA) clusters and computing resources in SINP. In addition, the authors are also grateful for the computational resources provided by LIGO Laboratory and Leonard E Parker Center for Gravitation, Cosmology and Astrophysics at the University of Wisconsin-Milwaukee and supported by National Science Foundation Grants PHY-0757058, PHY-0823459, PHY-1626190 and PHY-1700765. This paper has been assigned the internal LIGO Preprint Number P2100073. Data availability statement: The data that support the findings of this study are available upon reasonable request from the authors.
Group:LIGO, TAPIR
Funders:
Funding AgencyGrant Number
Department of Science and Technology (India)DST/SJF/PSA-01/2017-18
Department of Atomic Energy (India)RTI4001
Infosys FoundationUNSPECIFIED
NSFPHY-1806630
NSFPHY-2010970
Department of Science and Technology (India)MTR/2019/001096
Science and Engineering Research Board (SERB)SPF/2021/000036
Science and Engineering Research Board (SERB)SRG/2020/001290
Max Planck SocietyUNSPECIFIED
Canadian Institute for Advanced Research (CIFAR)UNSPECIFIED
Eberly College of ScienceUNSPECIFIED
Pennsylvania State UniversityUNSPECIFIED
NSFPHYS-1836779
NSFPHYS-2012083
NSFAST-2006384
NSFPHY-0757058
NSFPHY-0823459
NSFPHY-1626190
NSFPHY-1700765
Subject Keywords:compact object binaries, LIGO-India, gravitational-waves
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentP2100073
Issue or Number:2
DOI:10.1088/1361-6382/ac3b99
Record Number:CaltechAUTHORS:20220126-260834800
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220126-260834800
Official Citation:M Saleem et al 2022 Class. Quantum Grav. 39 025004
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:113120
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:28 Jan 2022 18:59
Last Modified:12 Jul 2022 19:52

Repository Staff Only: item control page