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| Content Provider | Springer Nature Link |
|---|---|
| Author | Cho, Hee Suk Lee, Chang Hwan |
| Copyright Year | 2018 |
| Abstract | We study gravitational wave searches for merging binary neutron stars (NSs). We use nonspinning template waveforms towards the signals emitted from aligned-spin NS-NS binaries, in which the spins of the NSs are aligned with the orbital angular momentum. We use the TaylorF2 waveform model, which can generate inspiral waveforms emitted from aligned-spin compact binaries. We employ the single effective spin parameter χ$_{eff}$ to represent the effect of two component spins (χ$_{1}$, χ$_{2}$) on the wave function. For a target system, we choose a binary consisting of the same component masses of 1.4M $_{⊙}$ and consider the spins up to χ$_{ i }$ = 0.4. We investigate fitting factors of the nonspinning templates to evaluate their efficiency in gravitational wave searches for the aligned-spin NS-NS binaries. We find that the templates can achieve the fitting factors exceeding 0.97 only for the signals in the range of −0.2 ≲ χ$_{eff}$ ≲ 0. Therefore, we demonstrate the necessity of using aligned-spin templates not to lose the signals outside that range. We also show how much the recovered total mass can be biased from the true value depending on the spin of the signal. |
| Starting Page | 1 |
| Ending Page | 5 |
| Page Count | 5 |
| File Format | |
| ISSN | 03744884 |
| Journal | Journal of the Korean Physical Society |
| Volume Number | 72 |
| Issue Number | 1 |
| e-ISSN | 19768524 |
| Language | English |
| Publisher | The Korean Physical Society |
| Publisher Date | 2018-01-07 |
| Publisher Place | Seoul |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Neutron star Gravitational waves Theoretical, Mathematical and Computational Physics Compact Binary Physics Particle and Nuclear Physics |
| Content Type | Text |
| Resource Type | Article |
| Subject | Physics and Astronomy |
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