Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants
Abstract Romano has recently found that frequency modulation of gravitational waves (GWs) could be used as a dark matter probe. Many candidates for dark matter (DM) of various sources have been proposed in the literature. In this work, we use a teleparallel modified GW model to obtain DM dark torsio...
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| Language: | English |
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SpringerOpen
2024-12-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | https://doi.org/10.1140/epjc/s10052-024-13481-3 |
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| author | L. C. Garcia de Andrade |
| author_facet | L. C. Garcia de Andrade |
| author_sort | L. C. Garcia de Andrade |
| collection | DOAJ |
| description | Abstract Romano has recently found that frequency modulation of gravitational waves (GWs) could be used as a dark matter probe. Many candidates for dark matter (DM) of various sources have been proposed in the literature. In this work, we use a teleparallel modified GW model to obtain DM dark torsion from LIGO data, where frequency modulation and frequency bands from various sources of GWs are investigated with regard to their suitability for DM dark torsion detection. In particular, nonhomogeneous and nonuniform chiral chemical potential generates GWs and dark torsion from primordial magnetic fields. It is shown that pulsar sources for GWs bathing the surface of the Earth on a contortion background of $$10^{-15}\,\textrm{s}^{-1}$$ 10 - 15 s - 1 possess amplitudes well within the parameters of LIGO capabilities of amplitudes on the order of $$10^{-22}$$ 10 - 22 . GWs are also investigated in the context of having been produced by a primordial magnetic field and inhomogeneity on the chiral chemical potential. The torsion signatures at LIGO correspond to the amplitude dependence of massive torsion by GWs. |
| format | Article |
| id | doaj-art-814f40fb07244e6e96568777bfa52122 |
| institution | Kabale University |
| issn | 1434-6052 |
| language | English |
| publishDate | 2024-12-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj-art-814f40fb07244e6e96568777bfa521222025-02-02T12:39:47ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522024-12-0184121910.1140/epjc/s10052-024-13481-3Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariantsL. C. Garcia de Andrade0Departamento de Física Teórica-IF-Universidade do Estado do Rio de Janeiro, UERJAbstract Romano has recently found that frequency modulation of gravitational waves (GWs) could be used as a dark matter probe. Many candidates for dark matter (DM) of various sources have been proposed in the literature. In this work, we use a teleparallel modified GW model to obtain DM dark torsion from LIGO data, where frequency modulation and frequency bands from various sources of GWs are investigated with regard to their suitability for DM dark torsion detection. In particular, nonhomogeneous and nonuniform chiral chemical potential generates GWs and dark torsion from primordial magnetic fields. It is shown that pulsar sources for GWs bathing the surface of the Earth on a contortion background of $$10^{-15}\,\textrm{s}^{-1}$$ 10 - 15 s - 1 possess amplitudes well within the parameters of LIGO capabilities of amplitudes on the order of $$10^{-22}$$ 10 - 22 . GWs are also investigated in the context of having been produced by a primordial magnetic field and inhomogeneity on the chiral chemical potential. The torsion signatures at LIGO correspond to the amplitude dependence of massive torsion by GWs.https://doi.org/10.1140/epjc/s10052-024-13481-3 |
| spellingShingle | L. C. Garcia de Andrade Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants European Physical Journal C: Particles and Fields |
| title | Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants |
| title_full | Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants |
| title_fullStr | Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants |
| title_full_unstemmed | Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants |
| title_short | Searching for dark torsion signatures at LIGO in Nieh–Yan teleparallel chiral gravitational waves and Chern–Simons invariants |
| title_sort | searching for dark torsion signatures at ligo in nieh yan teleparallel chiral gravitational waves and chern simons invariants |
| url | https://doi.org/10.1140/epjc/s10052-024-13481-3 |
| work_keys_str_mv | AT lcgarciadeandrade searchingfordarktorsionsignaturesatligoinniehyanteleparallelchiralgravitationalwavesandchernsimonsinvariants |