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| Autores principales: | , , , , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| Materias: | |
| Acceso en línea: | https://arxiv.org/abs/2411.19401 |
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| _version_ | 1866915050985357312 |
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| author | Lira, Mariana Villegas, Laura O. Antelis, Javier M. Jaramillo, Víctor Moreno, Claudia Núñez, Darío |
| author_facet | Lira, Mariana Villegas, Laura O. Antelis, Javier M. Jaramillo, Víctor Moreno, Claudia Núñez, Darío |
| contents | In this work, we investigate head-on collisions of $\ell$-boson stars, potential candidates for dark matter compact objects. We begin with a review of the general properties and features of these stars, leveraging results from prior studies to analyze the gravitational wave signals generated by such collisions. Considering a maximum distance of 100 Mpc for potential events, we identify the range of masses and scalar field frequencies for these stars that would render the gravitational waves detectable by current gravitational wave observatories. Additionally, we process the resulting signals to generate simulated observatory images, highlighting their similarities and differences compared to those produced by black hole collisions. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2411_19401 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | On the detectability of gravitational waves emitted from head-on collisions of $\ell$-boson stars Lira, Mariana Villegas, Laura O. Antelis, Javier M. Jaramillo, Víctor Moreno, Claudia Núñez, Darío General Relativity and Quantum Cosmology In this work, we investigate head-on collisions of $\ell$-boson stars, potential candidates for dark matter compact objects. We begin with a review of the general properties and features of these stars, leveraging results from prior studies to analyze the gravitational wave signals generated by such collisions. Considering a maximum distance of 100 Mpc for potential events, we identify the range of masses and scalar field frequencies for these stars that would render the gravitational waves detectable by current gravitational wave observatories. Additionally, we process the resulting signals to generate simulated observatory images, highlighting their similarities and differences compared to those produced by black hole collisions. |
| title | On the detectability of gravitational waves emitted from head-on collisions of $\ell$-boson stars |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2411.19401 |