Projects per year
Abstract
Inspiraling binary neutron stars are expected to be one of the most significant sources of gravitational-wave signals for the new generation of advanced ground-based detectors. We investigate how well we could hope to measure properties of these binaries using the Advanced LIGO detectors, which began operation in September 2015. We study an astrophysically motivated population of sources (binary components with masses $1.2~\mathrm{M}_\odot$--$1.6~\mathrm{M}_\odot$ and spins of less than $0.05$) using the full LIGO analysis pipeline. While this simulated population covers the observed range of potential binary neutron-star sources, we do not exclude the possibility of sources with parameters outside these ranges; given the existing uncertainty in distributions of mass and spin, it is critical that analyses account for the full range of possible mass and spin configurations. We find that conservative prior assumptions on neutron-star mass and spin lead to average fractional uncertainties in component masses of $\sim 16\%$, with little constraint on spins (the median $90\%$ upper limit on the spin of the more massive component is $\sim 0.7$). Stronger prior constraints on neutron-star spins can further constrain mass estimates, but only marginally. However, we find that the sky position and luminosity distance for these sources are not influenced by the inclusion of spin; therefore, if LIGO detects a low-spin population of BNS sources, less computationally expensive results calculated neglecting spin will be sufficient for guiding electromagnetic follow-up.
Original language | English |
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Article number | 116 |
Journal | The Astrophysical Journal |
Volume | 825 |
Issue number | 2 |
DOIs | |
Publication status | Published - 11 Jul 2016 |
Bibliographical note
10 pages, 9 figuresKeywords
- gravitational waves
- methods: data analysis
- stars: neutron
- surveys
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Dive into the research topics of 'Parameter estimation on gravitational waves from neutron-star binaries with spinning components'. Together they form a unique fingerprint.Projects
- 3 Finished
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Ernest Rutherford Fellowship : Dr John Veitch - Surveying black holes and neutron stars with gravitational waves
Veitch, J.
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/02/14 → 30/04/17
Project: Research Councils
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Birmingham Astrophysics : Consolidated Grant 2013-2016
Vecchio, A., Ponman, T., Freise, A., Smith, G., Speake, C., Mandel, I., Cruise, M., Raychaudhury, S. & Stevens, I.
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/04/13 → 30/09/16
Project: Research Councils
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UK Involvement in the Operations of Advanced LIGO
Vecchio, A. & Freise, A.
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/08/11 → 31/12/15
Project: Research Councils