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Dark photons and tachyonic instability induced by Barbero-Immirzi parameter and axion-torsion transmutation
Gao, Zhi-Fu1; Li, Biaopeng1,2; de Andrade, L. C. Garcia3,4
2025-04-18
Source PublicationEUROPEAN PHYSICAL JOURNAL C
ISSN1434-6044
Volume85Issue:4Pages:433
Contribution Rank1
AbstractIn this paper, we investigate Holst gravity by examining two different examples. The first example involves minimal coupling to torsion, while the second explores non-minimal coupling. The motivation for the first example stems from the recent work by Dombriz et al. (Phys Lett B 834:137488, 2022), which utilized a technique of imposing constraint constant coefficients to massive torsion in the model Lagrangian to determine parameters for the Einstein-Cartan-Holst gravity. We extend this methodology to investigate dark photons, where axial torsion transforms into axions. Interest in elucidating the abundance of dark photons within the framework of general relativity was sparked by Agrawal et al. (Phys Lett B 801:135136, 2020). Building on the work of Barman et al. (Phys Rev D 101:075017, 2020), who explored minimal coupling of massive torsion mediated by dark matter (DM) with light torsion on the order of 1.7 TeV, we have derived a Barbero-Immirzi (BI) parameter of approximately 0.775. This value falls within the range established by Panza et al. at TeV scales, specifically 0 <=beta <= 1.185\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$0\le {\beta } \le {1.185}$$\end{document} (Phys Rev D 90:125007, 2014). To the best of our knowledge, this is the first time a BI parameter has been induced by dark photons on a minimal Einstein-Cartan (EC) gravity. Very recently, implications of the finding of a BI parameter in cosmological bounces have appeared in the literature (Phys Dark Universe 44:141078, 2024). For a smaller BI parameter, a higher torsion mass of 1.51 TeV is obtained. Nevertheless, this figure is still a signature of light torsion which can be compatible with light dark photon masses. The magnetic helicity instability of the dark photons is investigated. The axion oscillation frequency is shown to depend on the BI parameter, and the BI spectra are determined by a histogram. This study not only broadens the understanding of Holst gravity but also provides crucial insights into the interplay between torsion, dark photons, and axions in the cosmological context.
DOI10.1140/epjc/s10052-025-14065-5
Indexed BySCI
Language英语
Funding ProjectNSFC[12288102] ; NSFC[12041304] ; NSFC[2023TSYCTD0013]
WOS Research AreaPhysics
WOS SubjectPhysics, Particles & Fields
WOS IDWOS:001471023000001
PublisherSPRINGER
Funding OrganizationNSFC
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7703
Collection射电天文研究室_脉冲星研究团组
Corresponding AuthorGao, Zhi-Fu; de Andrade, L. C. Garcia
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
2.Univ Chinese Acad Sci, Beijing, Peoples R China
3.Univ Estado Rio De Janeiro, Dept Fis Teor, Cosmol & Gravitat Grp, IF, Rua Sao Francisco Xavier 524, BR-20550 Rio De Janeiro, RJ, Brazil
4.Inst Cosmol & Philosophy Nat, Krizhevci, Croatia
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Gao, Zhi-Fu,Li, Biaopeng,de Andrade, L. C. Garcia. Dark photons and tachyonic instability induced by Barbero-Immirzi parameter and axion-torsion transmutation[J]. EUROPEAN PHYSICAL JOURNAL C,2025,85(4):433.
APA Gao, Zhi-Fu,Li, Biaopeng,&de Andrade, L. C. Garcia.(2025).Dark photons and tachyonic instability induced by Barbero-Immirzi parameter and axion-torsion transmutation.EUROPEAN PHYSICAL JOURNAL C,85(4),433.
MLA Gao, Zhi-Fu,et al."Dark photons and tachyonic instability induced by Barbero-Immirzi parameter and axion-torsion transmutation".EUROPEAN PHYSICAL JOURNAL C 85.4(2025):433.
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