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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| Soggetti: | |
| Accesso online: | https://arxiv.org/abs/2412.14551 |
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| _version_ | 1866918062716878848 |
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| author | Iwaya, Masaki Kobayashi, Kazuya Morisaki, Soichiro Hotokezaka, Kenta Kinugawa, Tomoya |
| author_facet | Iwaya, Masaki Kobayashi, Kazuya Morisaki, Soichiro Hotokezaka, Kenta Kinugawa, Tomoya |
| contents | We derive an analytical form of the joint prior of effective spin parameters, $χ_\mathrm{eff}$ and $χ_\mathrm{p}$, assuming an isotropic and uniform-in-magnitude spin distribution. This is a vital factor in performing hierarchical Bayesian inference for studying the population properties of merging compact binaries observed with gravitational waves. In previous analyses, this was evaluated numerically using kernel density estimation (KDE). However, we find that this numerical approach is inaccurate in certain parameter regions, where both $|χ_\mathrm{eff}|$ and $χ_\mathrm{p}$ are small. Our analytical approach provides accurate computations of the joint prior across the entire parameter space and enables more reliable population inference. Employing our analytic prior, we reanalyze binary black holes in the Gravitational-Wave Transient Catalog 3 (GWTC-3) by the LIGO-Virgo-KAGRA collaboration. While the results are largely unchanged, log-likelihood errors due to the use of the inaccurate prior evaluations are $\mathcal{O}(1)$. Since these errors accumulate with the increasing number of events, our analytical prior will be crucial in the future analyses. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_14551 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | An analytical joint prior for effective spins for inference on the spin distribution of binary black holes Iwaya, Masaki Kobayashi, Kazuya Morisaki, Soichiro Hotokezaka, Kenta Kinugawa, Tomoya General Relativity and Quantum Cosmology We derive an analytical form of the joint prior of effective spin parameters, $χ_\mathrm{eff}$ and $χ_\mathrm{p}$, assuming an isotropic and uniform-in-magnitude spin distribution. This is a vital factor in performing hierarchical Bayesian inference for studying the population properties of merging compact binaries observed with gravitational waves. In previous analyses, this was evaluated numerically using kernel density estimation (KDE). However, we find that this numerical approach is inaccurate in certain parameter regions, where both $|χ_\mathrm{eff}|$ and $χ_\mathrm{p}$ are small. Our analytical approach provides accurate computations of the joint prior across the entire parameter space and enables more reliable population inference. Employing our analytic prior, we reanalyze binary black holes in the Gravitational-Wave Transient Catalog 3 (GWTC-3) by the LIGO-Virgo-KAGRA collaboration. While the results are largely unchanged, log-likelihood errors due to the use of the inaccurate prior evaluations are $\mathcal{O}(1)$. Since these errors accumulate with the increasing number of events, our analytical prior will be crucial in the future analyses. |
| title | An analytical joint prior for effective spins for inference on the spin distribution of binary black holes |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2412.14551 |